default_study
default_study
000001 default_study
John Rainnie
Science
18-Oct-2006
Study 000001:
desc000001.txt
2255563
1
0
Quiet Sun
Scanning
32243712
0
0
0
1
1
81
Test_study_3
Test_study
000002 Test_study
John Rainnie
Science
7-Nov-2006
Study 000002:
desc000002.txt
147149
1
0
Active Region
Scanning
9830400
0
3
3
2
1
40
JTM001_256x512_60s_slit1
JTM001
000003 JTM001
John Mariska
Science
20-Nov-2006
Study 000003:
This study constructs a simple 256 step by 512 arcsec high raster
using 60 s exposures and a 1 arcsec slit. Only a limited line
list is used, most of them reasonably strong, so the study can be
used in both quiet regions and active regions. Repeated rasters
can be constructed by repeat raster parameter. Note that this study
was designed early in the mission and did not fully utilize the
EIS telemetry allocation. Better raster studies with more lines
should probably be used now. The study makes no slit/slot moves
and so can run through SAAs.
hello Mike
WARNING: none.
desc000003.txt
16653526
1
0
Quiet Sun
Scanning
181193935
0
0
0
3
1
256
JTM001_256x512_60s_slit1_2
JTM001_2
000004 JTM001_2
John Mariska
Science
20-Nov-2006
Study 000004:
desc000004.txt
16653526
1
0
Quiet Sun
Scanning
181193935
0
0
0
4
1
256
JTM002_256x256_30s_slit1
JTM002
000005 JTM002
John Mariska
Science
20-Nov-2006
Study 000005:
This study constructs a simple 256 step by 256 arcsec high raster
using 30 s exposures and a 1 arcsec slit. Only a limited line
list is used, most of them reasonably strong. The 30 s exposure
time should give good results in active regions. Repeated
rasters can be constructed by repeat raster parameter. Note that
this study was designed early in the mission and did not fully
utilize the EIS telemetry allocation. Better raster studies with
more lines should probably be used now. The study makes no
slit/slot moves and so can run through SAAs.
WARNING: none.
desc000005.txt
8589526
1
0
Quiet Sun
Scanning
90596967
0
0
0
5
1
256
JTM003_512x512_60s_slit1
JTM003
000006 JTM003
John Mariska
Science
20-Nov-2006
Study 000006:
This study constructs a simple 512 step by 512 arcsec high raster
using 60 s exposures and a 1 arcsec slit. Only a limited line
list is used, most of them reasonably strong. The 60 s exposure
time should give good results in quiet regions and some weak
active regions. Repeated rasters can be constructed by repeat raster
parameter. Note that this study was designed early in the
mission and did not fully utilize the EIS telemetry allocation.
Better raster studies with more lines should probably be used
now. Also note that this study takes a long time to run. The
study makes no slit/slot moves and so can run through SAAs.
WARNING: none.
desc000006.txt
33284552
1
0
Quiet Sun
Scanning
362387871
0
0
0
6
1
512
JTM004_512x256_30s_slit1
JTM004
000007 JTM004
John Mariska
Science
20-Nov-2006
Study 000007:
This study constructs a simple 512 step by 256 arcsec high raster
using 30 s exposures and a 1 arcsec slit. Only a limited line
list is used, most of them reasonably strong. The 30 s exposure
time should give good results in active regions. Repeated
rasters can be constructed by repeat raster parameter. Note that
this study was designed early in the mission and did not fully
utilize the EIS telemetry allocation. Better raster studies with
more lines should probably be used now. The study makes no
slit/slot moves and so can run through SAAs.
WARNING: none.
desc000007.txt
17156552
1
0
Quiet Sun
Scanning
181193935
0
0
0
7
1
512
Active Region Sit-and-Stare Hunt for Rapid Variability (neutral line, plage, sunspots and loops)
COMSCI_AR1
000008 COMSCI_AR1
David Williams
Science
20-Nov-2006
Study 000008:
desc000008.txt
10962853
5
0
Active Region
Scanning
331140303
2
3
3
8
1
240
9
1
1
10
1
1
11
1
1
8
1
240
Active Region Scan for Global Changes and Dynamic Phenomena
COMSCI_AR2
000009 COMSCI_AR2
David Williams
Science
20-Nov-2006
Study 000009:
desc000009.txt
4115503
4
0
Active Region
Scanning
130233139
2
3
3
8
1
240
12
1
256
13
1
60
8
1
240
Accurate Measurement of Velocity Shifts in an Active Region
COMSCI_AR3
000010 COMSCI_AR3
David Williams
Science
20-Nov-2006
Study 000010:
desc000010.txt
11430106
3
0
Active Region
Scanning
106640179
2
3
3
8
1
240
14
1
256
8
1
240
Evaporation in a Flare - Fast Raster
COMSCI_FLR1
000011 COMSCI_FLR1
David Williams
Science
20-Nov-2006
Study 000011:
desc000011.txt
1917606
1
0
Flare
Scanning
147456000
0
2
2
15
6
200
Flare Evaporation - spectral imaging
COMSCI_FLR2
000012 COMSCI_FLR2
David Williams
Science
20-Nov-2006
Study 000012:
desc000012.txt
1822940
1
0
Flare
Scanning
358612840
0
3
3
16
190
120
Detailed diagnostics of two supergranular cells in the quiet Sun
COMSCI_QS1
000013 COMSCI_QS1
David Williams
Science
20-Nov-2006
Study 000013:
desc000013.txt
22477060
11
0
Quiet Sun
Scanning
509607941
10
3
3
17
1
80
18
1
80
17
1
80
18
1
80
17
1
80
18
1
80
17
1
80
18
1
80
17
1
80
18
1
80
17
1
80
Changing morphology of the quiet Sun at high (one-minute) cadence using the narrow slot
COMSCI_QS2
000014 COMSCI_QS2
David Williams
Science
20-Nov-2006
Study 000014:
desc000014.txt
10806558
1
0
Quiet Sun
Scanning
124570830
0
3
3
19
3
40
Detailed, high-cadence spectra at a fixed location in the quiet Sun
COMSCI_QS3
000015 COMSCI_QS3
David Williams
Science
20-Nov-2006
Study 000015:
desc000015.txt
11033421
7
0
Quiet Sun
Scanning
251238806
6
3
3
20
1
40
21
3
1
20
1
40
21
3
1
20
1
40
21
3
1
20
1
40
Small spectral rasters for high-cadence observations of a network feature
COMSCI_QS4
000016 COMSCI_QS4
David Williams
Science
20-Nov-2006
Study 000016:
desc000016.txt
7441290
5
0
Quiet Sun
Scanning
506462208
4
3
3
17
1
80
22
40
10
17
1
80
22
40
10
17
1
80
Spectral atlas and diagnostics of quiet Sun, to be run on disc and both east and west limbs
COMSCI_QS5
000017 COMSCI_QS5
David Williams
Science
20-Nov-2006
Study 000017:
desc000017.txt
9765173
1
0
Quiet Sun
Scanning
402653190
0
0
0
23
1
10
Dark current, hot pixels and column defects
regcal015
000018 regcal015
Louisa Bradley
Engineering
Study 000018:
1) Acronym: regcal015
2) Repeats: 1
3) 8 dark exposures, full ccd (exposure times: 1,1,10,10,30,30,60,60 seconds)
4) Time required: 8 mins
5) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000018.txt
480000
0
0
Engineering
SnS
134217728
0
0
0
Dark current, hot pixels and column defects
regcal016
000019 regcal016
Louisa Bradley
Engineering
Study 000019:
1) Acronym: regcal016
2) Repeats: 1
3) 8 dark exposures, full ccd
(exposure times: 100,100,150,150,300,300,600,600 seconds)
4) Time required: 40 mins 4 secs
5) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000019.txt
2404000
0
0
Engineering
SnS
134217728
0
0
0
Flat fields, short exposures
regcal017
000020 regcal017
Louisa Bradley
Engineering
Study 000020:
1) Acronym: regcal017
2) Repeats: 1
3) 8 flat field exposures (1 sec), full ccd
(LED on times: 0,0,10,10,20,20,40,40ms)
4) Time required: 14 mins
5) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000020.txt
840000
0
0
Engineering
SnS
134217728
0
0
0
Flat fields, long exposures
regcal018
000021 regcal018
Louisa Bradley
Engineering
Study 000021:
1) Acronym: regcal018
2) Repeats: 1
3) 8 flat field exposures (1 sec exps), full ccd
(LED on times: 60,60,80,80,100,100,120,120ms)
4) Time required: 14 mins
5) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000021.txt
840000
0
0
Engineering
SnS
134217728
0
0
0
JTM005_120exp_512y_60s_slit1_ss
JTM005
000022 JTM005
John Mariska
Science
4-Dec-2006
Study 000022:
This study constructs a simple 120 exposure by 512 arcsec high
sit-and-stare data set using 60 s exposures and a 1 arcsec slit.
Only a limited line list is used, most of them reasonably strong.
The 60 s exposure time should give good results in both quiet
regions and active regions. Longer times can be covered by
repeating the raster. Pointing can be an issue. It would be good
to make some sort of context raster before doing this one. Note
that this study was designed early in the mission and did not
fully utilize the EIS telemetry allocation. Better raster
studies with more lines should probably be used now. The study
makes no slit/slot moves and so can run through SAAs.
WARNING: none.
desc000022.txt
7818293
1
0
Quiet Sun
Scanning
113246209
0
0
0
24
1
1
JTM006_120exp_512y_90s_slit1_ss
JTM006
000023 JTM006
John Mariska
Science
4-Dec-2006
Study 000023:
This study constructs a simple 120 exposure by 512 arcsec high
sit-and-stare data set using 90 s exposures and a 1 arcsec slit.
Only a limited line list is used, most of them reasonably strong.
The 90 s exposure time should give good results in quiet regions.
Longer times can be covered by repeating the raster. Pointing can
be an issue. It would be good to make some sort of context
raster before doing this one. Note that this study was designed
early in the mission and did not fully utilize the EIS telemetry
allocation. Better raster studies with more lines should
probably be used now. The study makes no slit/slot moves and so
can run through SAAs.
WARNING: none.
desc000023.txt
11598293
1
0
Quiet Sun
Scanning
113246209
0
0
0
25
1
1
ADC offset
regcal014
000024 regcal014
Louisa Bradley
Engineering
Study 000024:
1) Acronym: regcal014
2) Repeats: 1
3) 1 dark exposure, full ccd (0 sec exp)
4) Time required: 1 min
5) Target: None (shutter closed)
WARNING:
None
desc000024.txt
60000
0
0
Engineering
SnS
33554432
0
0
0
Intensity calibration
regcal019
000025 regcal019
Louisa Bradley
Engineering
Study 000025:
1) Acronym: regcal019
2) Repeats: 1
3) 1 exposure (100 secs), full ccd, 1" slit
4) Time required: 3 mins 16 secs
5) Target: QS
WARNING:
None
desc000025.txt
196000
0
0
Engineering
SnS
33554432
0
0
0
Flat field with overscan pixels (50*8)
regcal070
000026 regcal070
Louisa Bradley
Engineering
Study 000026:
1) Acronym: regcal070
2) Repeats: 1
3) 2 flat field exposures (1 sec exps), full ccd (including overscan pixels)
(LED on time = 100ms)
4) Time required: 2 mins
5) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000026.txt
120000
0
0
Engineering
SnS
33554432
0
0
0
Dark exposures, CCD bottom rows (100s exposures)
regcal071
000027 regcal071
Louisa Bradley
Engineering
Study 000027:
1) Acronym: regcal071
2) Repeats: 1
3) 2 dark exposures (100 sec exps), full ccd, bottom 512 rows of CCDs
4) Time required: 4m 20s
5) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000027.txt
260000
0
0
Engineering
SnS
33612416
0
0
0
Dark exposures, top CCD rows (100s exposures)
regcal072
000028 regcal072
Louisa Bradley
Engineering
Study 000028:
1) Acronym: regcal072
2) Repeats: 1
3) 2 dark exposures (100 sec exps), full ccd, top 512 rows of CCDs
4) Time required: 4m 20s
5) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000028.txt
260000
0
0
Engineering
SnS
33612416
0
0
0
COMP_TEST_AR_SLIT
COMP_TEST_AR_SLIT
000029 COMP_TEST_AR_SLIT
Shin Imada
Test
14-Dec-2006
Study 000029:
desc000029.txt
1101890
10
0
Active Region
Scanning
454164480
0
0
0
26
1
5
26
1
5
26
1
5
26
1
5
26
1
5
26
1
5
26
1
5
26
1
5
26
1
5
26
1
5
COMP_TEST_AR_SLOT
COMP_TEST_AR_SLOT
000030 COMP_TEST_AR_SLOT
Shin Imada
Test
14-Dec-2006
Study 000030:
desc000030.txt
249180
10
0
Active Region
Scanning
30277632
0
3
3
27
1
40
27
1
40
27
1
40
27
1
40
27
1
40
27
1
40
27
1
40
27
1
40
27
1
40
27
1
40
COMP_TEST_QS_SLIT
COMP_TEST_QS_SLIT
000031 COMP_TEST_QS_SLIT
Shin Imada
Test
14-Dec-2006
Study 000031:
desc000031.txt
2645620
10
0
Quiet Sun
Scanning
454164480
0
0
0
28
1
5
28
1
5
28
1
5
28
1
5
28
1
5
28
1
5
28
1
5
28
1
5
28
1
5
28
1
5
COMP_TEST_QS_SLOT
COMP_TEST_QS_SLOT
000032 COMP_TEST_QS_SLOT
Shin Imada
Test
14-Dec-2006
Study 000032:
desc000032.txt
557920
10
0
Quiet Sun
Scanning
30277632
0
3
3
29
1
40
29
1
40
29
1
40
29
1
40
29
1
40
29
1
40
29
1
40
29
1
40
29
1
40
29
1
40
HPW001_FULLCCD_RAST_128x128_90S_SLIT1
HPW001_FULLCCD_RAST
000033 HPW001_FULLCCD_RAST
Harry Warren
Science
20-Dec-2006
Study 000033:
desc000033.txt
12370013
1
0
Quiet Sun
Scanning
429496736
0
0
0
30
1
128
SYNOP001_40arcsec_1arcsec_30s_90s
SYNOP001
000034 SYNOP001
John Mariska
Science
20-Dec-2006
Study 000034:
ACRONYM: SYNOP001
*** DO NOT *** run more than once a day!
Target:
-------
Sun center or near Sun center ** Do not use elsewhere **
Instruction to planners:
-----------------------
1) Run SYNOP001 daily if there is an XRT synoptic
2) If there is a ***second*** XRT synoptic for that day:
* DO NOT run SYNOP001 again
* Run SYNOP005_A (ID #265) as the second SYNOP of the day
WARNING:
--------
DO NOT run more than once a day
desc000034.txt
287206
2
0
Quiet Sun
Scanning
26843546
1
3
0
31
1
40
32
1
1
HH_AR+FLR_RAS_H01 (EWxNS=240"x240", 5.0sec exp, different FMIR init. pos. for ea
HH_AR+FLR_RAS_H01
000035 HH_AR+FLR_RAS_H01
Hiro Hara
Science
22-Dec-2006
Study 000035:
ACRONYM: H_AR_FLR_RAW_H01
*** RECURSIVE STUDY ***
Description:
This is the infinite-loop Study that contains 10 rasters for AR targets.
The step size of the raster is 10 arcsec and it covers the area of
EWxNS=240x240 arcsec2. 1 arcsec width slit is used for 5 sec
exposure duration. The line list contains 17 windows including
Fe XXIII and Fe XXIV lines. The initial scanning position should be
different among 10 rasters. By assembling 10 rasters a single raster
of full-spatial sampling can be reproduced. Each raster finishes
for 2.6 min. A high-cadence observation for flares is possible.
HH_AR_FLR_RAS_H02 is better for flare observations. Density
diagnostics can be made by line ratios of Fe XII, Fe XIII, Fe XIV
TARGET: AR
WARNING:
None
desc000035.txt
1767590
10
1
Active Region
Scanning
339591168
0
0
0
33
1
231
33
1
231
33
1
231
33
1
231
33
1
231
33
1
231
33
1
231
33
1
231
33
1
231
33
1
231
HH_AR+FLR_RAS_N01 (EWxNS=240"x240", 5.0sec exp, continuous raster)
HH_AR+FLR_RAS_N01
000036 HH_AR+FLR_RAS_N01
Hiro Hara
Science
22-Dec-2006
Study 000036:
desc000036.txt
1754087
1
0
Active Region
Scanning
361267200
0
0
0
34
1
240
HH_AR+FLR_RAS_N03 (EWxNS=240"x240", 5.0sec exp, continuous raster)
HH_AR+FLR_RAS_N03
000037 HH_AR+FLR_RAS_N03
Hiro Hara
Science
22-Dec-2006
Study 000037:
desc000037.txt
888293
1
0
Active Region
Scanning
180633600
0
2
2
35
1
240
HH_QS_RASTER (EWxNS=40"x120", 60sec exp, different FMIR init. pos. for each rast
HH_QS_RAS_H01
000038 HH_QS_RAS_H01
Hiro Hara
Science
22-Dec-2006
Study 000038:
desc000038.txt
2634600
10
1
Quiet Sun
Scanning
125829120
0
0
0
36
1
31
36
1
31
36
1
31
36
1
31
36
1
31
36
1
31
36
1
31
36
1
31
36
1
31
36
1
31
HH_QS_RASTER (EWxNS=60"x120", 60sec exp, continuous raster from West to East)
HH_QS_RAS_N01
000039 HH_QS_RAS_N01
Hiro Hara
Science
22-Dec-2006
Study 000039:
desc000039.txt
3920397
1
0
Quiet Sun
Scanning
188743682
0
0
0
37
1
60
HPW005_QS_SLOT_060m
HPW005_QS_SLOT_060m
000040 HPW005_QS_SLOT_060m
Harry Warren
Science
22-Dec-2006
Study 000040:
desc000040.txt
3270747
1
0
Quiet Sun
Scanning
91750401
0
3
3
38
1
40
HPW006_QS_SLOT_120m
HPW006_QS_SLOT_120m
000041 HPW006_QS_SLOT_120m
Harry Warren
Science
22-Dec-2006
Study 000041:
desc000041.txt
7168644
1
0
Quiet Sun
Scanning
201850883
0
3
3
39
1
40
HPW007_QS_SLOTW_060m
HPW007_QS_SLOTW_060m
000042 HPW007_QS_SLOTW_060m
Harry Warren
Science
8-Jan-2007
Study 000042:
DO NOT USE. OBSOLETE.
USE #000043
desc000042.txt
3530610
1
0
Quiet Sun
Scanning
99090432
0
3
3
40
18
116
HPW007_QS_SLOTW_060m_v2
HPW007_QS_SLOTW_v2
000043 HPW007_QS_SLOTW_v2
Harry Warren
Science
15-Jan-2007
Study 000043:
desc000043.txt
3530610
1
0
Quiet Sun
Scanning
99090432
0
3
3
40
18
116
HPW002_QS_SAS_060m
HPW002_QS_SAS_060m
000044 HPW002_QS_SAS_060m
Harry Warren
Science
15-Jan-2007
Study 000044:
desc000044.txt
3270747
1
0
Quiet Sun
Scanning
66846720
0
0
0
41
1
1
HPW004_QS_RAST_120m
HPW004_QS_RAST_120m
000045 HPW004_QS_RAST_120m
Harry Warren
Science
15-Jan-2007
Study 000045:
desc000045.txt
8338013
1
0
Quiet Sun
Scanning
171127605
0
0
0
42
1
128
GAD001_AR_rast
GAD001_AR_rast
000046 GAD001_AR_rast
George Doschek
Science
29-Mar-2007
Study 000046:
This study is a modification of a commissioning study such as
COMSCI_AR2. The purpose is to include cooler transition region lines with
the coronal lines already present in the commissioning study. Fe XXIV is
not included in this study. The purpose of this study is to map an active
region in many lines so that an active region map can be made for
temperature, density, nonthermal motions, and bulk motions. It should be
run only on an active region. There are no slit/slot motions.
WARNING: None.
desc000046.txt
4557526
1
0
Active Region
Scanning
134217730
0
0
0
43
1
256
High cadence sit-and-stare in ARs; 5s exposure; Fe XIII dens; 40" context before
PRY_fast_dens
000047 PRY_fast_dens
Peter Young
Science
15-Jan-2007
Study 000047:
Consists of three rasters:
(1) a context raster covering 40x304 arcsec2 with 1" slit
(2) sit-and-stare with 1" slit taking 304" along slit (100 exposures)
(3) repeat of context raster
Exposure times are 5 seconds, and five lines are included: the core
lines plus the Fe XIII 203.8/202.0 density diagnostic.
USE: The aim is search for high cadence density variations in active
regions.
NOTES: the number of repeats of (2) should be adjusted to fill the
available time slot.
WARNING: because of the 2nd context raster (3), care has to be taken
that the change from (2) to (3) does not take place during an SAA. For
this reason the planner is requested to run the study
PRY_fast_dens_v2.
desc000047.txt
1338620
3
0
Active Region
Scanning
56655872
0
0
0
44
1
41
45
1
1
44
1
41
Cool lines for study of loop footpoints (e.g., near sunspot); 80" raster, 20 lin
PRY_loop_footpoints
000048 PRY_loop_footpoints
Peter Young
Science
15-Jan-2007
Study 000048:
*** OBSOLETE ***
Requested by the author on 27/06/2007
desc000048.txt
1695747
1
0
Active Region
Scanning
69120001
0
2
2
46
1
100
Study for FOV alignment purpose with 266"-width slit
HH_FOV_Alignment
000049 HH_FOV_Alignment
Hiro Hara
Engineering
17-Jan-2007
Study 000049:
desc000049.txt
178606
1
0
Quiet Sun
Scanning
53687092
0
1
1
47
1
396
HPW008_FULLCCD_RAST_128x128_25s_SLIT1
HPW008_FULLCCD_RAST
000050 HPW008_FULLCCD_RAST
Harry Warren
Science
17-Jan-2007
Study 000050:
desc000050.txt
3634013
1
0
Active Region
Scanning
429496736
0
0
0
48
1
128
HPW009_FULLCCD_RAST_1x128_25s_SLIT1
HPW009_FULLCCD_SAS
000051 HPW009_FULLCCD_SAS
Harry Warren
Science
17-Jan-2007
Study 000051:
desc000051.txt
3267219
1
0
Active Region
Scanning
385875973
0
0
0
49
1
1
HPW010_FULLCCD_RAST_40x128_25s_SLIT40
HPW010_FULLCCD_SAS
000052 HPW010_FULLCCD_SAS
Harry Warren
Science
17-Jan-2007
Study 000052:
desc000052.txt
3267219
1
0
Active Region
Scanning
385875973
0
3
3
50
1
40
QCMs 6 seconds measurement
regeng020
000053 regeng020
Jason Tandy
Engineering
Study 000053:
desc000053.txt
180000
0
0
Engineering
SnS
0
0
0
0
GAD002_AR_rast
GAD002_AR_rast
000054 GAD002_AR_rast
George Doschek
Science
29-Mar-2007
Study 000054:
This study is the same as GAD001_AR_rast except that the
exposure time has been increased from 15s to 60s. Time resolution is
sacrificed in order to obtain better counting statistics in weak lines.
This study should be run only on an active region. There are no slit/slot
motions.
WARNING: None.
desc000054.txt
16653526
1
0
Active Region
Scanning
134217730
0
0
0
51
1
256
HPW011_HR_AR_SAS_1x512_10s_SLIT1_18WINDOWS
HPW011_HR_AR_SAS
000055 HPW011_HR_AR_SAS
Harry Warren
Science
30-Jan-2007
Study 000055:
desc000055.txt
3761983
1
0
Active Region
Scanning
456130566
0
0
0
52
1
1
HPW012_AR_SAS_060M
HPW012_AR_SAS_060M
000056 HPW012_AR_SAS_060M
Harry Warren
Science
30-Jan-2007
Study 000056:
desc000056.txt
1695747
1
0
Active Region
Scanning
62464000
0
0
0
53
1
1
HPW013_AR_RAS_23m
HPW013_AR_RAS_23m
000057 HPW013_AR_RAS_23m
Harry Warren
Science
30-Jan-2007
Study 000057:
desc000057.txt
1394563
1
0
Active Region
Scanning
51220480
0
0
0
54
1
41
Context SLOT images
IUU_SLOT_Context_001
000058 IUU_SLOT_Context_001
Ignacio Ugarte
Science
30-Jan-2007
Study 000058:
desc000058.txt
218678
1
0
Quiet Sun
Scanning
3145728
0
3
3
55
1
40
Sit-and-Stare with wide temperature coverage. QS, BPs and loops.
IUU_QS_SNS_001
000059 IUU_QS_SNS_001
Ignacio Ugarte
Science
30-Jan-2007
Study 000059:
desc000059.txt
3920397
1
0
Quiet Sun
Scanning
113246209
0
0
0
56
1
1
Pointing and Alignment (266" slot) East Limb, North Pole
regcal020
000060 regcal020
Louisa Bradley
Engineering
Study 000060:
1) Acronym: regcal020
2) Repeats: 1
3) Pointing and alignment study throughout 4 orbits, QS line list
4) Time required: 347 mins
5) Target: East limb and north pole
WARNING:
This study is no longer required as science studies are used instead.
desc000060.txt
20790000
0
0
Engineering
SnS
4429185024
0
0
0
Pointing and Alignment (266" slot) Active Region
regcal022
000061 regcal022
Louisa Bradley
Engineering
Study 000061:
1) Acronym: regcal022
2) Repeats: 1
3) Pointing and alignment study throughout 4 orbits, AR line list
4) Time required: 347 mins
5) Target: AR
WARNING:
This study is no longer required as science studies are used instead.
desc000061.txt
20790000
0
0
Engineering
SnS
2430861312
0
0
0
Slot Image (40" and 266") - Quiet Sun Raster
regcal067
000062 regcal067
Louisa Bradley
Engineering
Study 000062:
1) Acronym: regcal067
2) Repeats: 1
3) EUV flat fields using 40" and 266" slots across entire FOV, QS line list
4) Time required: 167 mins
5) Target: QS
WARNING:
DO NOT run within SAA
desc000062.txt
10038000
0
0
Engineering
SnS
191201280
0
0
0
Slot Image (40" and 266") - Active Region Raster
regcal068
000063 regcal068
Louisa Bradley
Engineering
Study 000063:
1) Acronym: regcal068
2) Repeats: 1
3) EUV flat fields using 40" and 266" slots across entire FOV, full ccd
4) Time required: 34 mins 17 secs
5) Target: AR
WARNING:
DO NOT run within SAA
High DR
desc000063.txt
2057000
0
0
Engineering
SnS
219217920
0
0
0
Wavelength calibration, qs, 1" slit, full ccd bottom
regcal001
000064 regcal001
Louisa Bradley
Engineering
Study 000064:
1) Acronym: regcal001
2) Repeats: 1
3) 6 exposures, full ccd, 1" slit, bottom 512 rows of CCDs
(exposure times: 10,20,40,80,160,600 seconds)
4) Time required: 17 mins 18 secs
5) Target: QS
WARNING:
This study is no longer required as science studies are used instead.
desc000064.txt
1038000
0
0
Engineering
SnS
201326592
0
0
0
Wavelength calibration, qs, 1" slit, full ccd top
regcal002
000065 regcal002
Louisa Bradley
Engineering
Study 000065:
1) Acronym: regcal002
2) Repeats: 1
3) 6 exposures, full ccd, 1" slit, top 512 rows of CCDs
(exposure times: 10,20,40,80,160,600 seconds)
4) Time required: 17 mins 18 secs
5) Target: QS
WARNING:
This study is no longer required as science studies are run instead.
desc000065.txt
1038000
0
0
Engineering
SnS
201326592
0
0
0
Wavelength calibration, qs, 2" slit, full ccd middle
regcal003
000066 regcal003
Louisa Bradley
Engineering
Study 000066:
1) Acronym: regcal003
2) Repeats: 1
3) 6 exposures, full ccd, 2" slit
(exposure times: 10,20,40,80,160,600 seconds)
4) Time required: 17 mins 32 secs
5) Target: QS
WARNING:
This study is no longer required as science studies are run instead.
desc000066.txt
1052000
0
0
Engineering
SnS
201326592
0
0
0
Wavelength cal, QS, 40" slot
regcal004
000067 regcal004
Louisa Bradley
Engineering
Study 000067:
1) Acronym: regcal004
2) Repeats: 1
3) 6 exposures, full ccd, 40" slot
(exposure times: 10,20,40,80,160,600 seconds)
4) Time required: 17 mins
5) Target: QS
WARNING:
This study is no longer required as science studies are run instead.
desc000067.txt
1020000
0
0
Engineering
SnS
201326592
0
0
0
Wavelength cal, QS, 266" slot
regcal005
000068 regcal005
Louisa Bradley
Engineering
Study 000068:
1) Acronym: regcal005
2) Repeats: 1
3) 6 exposures, full ccd, 266" slot
(exposure times: 10,20,40,80,160,600 seconds)
4) Time required: 17 mins
5) Target: QS
WARNING:
This study is no longer required as science studies are run instead.
desc000068.txt
1020000
0
0
Engineering
SnS
201326592
0
0
0
Wavelength cal, AR, 1" slit
regcal006
000069 regcal006
Louisa Bradley
Engineering
Study 000069:
1) Acronym: regcal006
2) Repeats: 1
3) 7 exposures, full ccd, 1" slit
(exposure times: 0.25,0.5,1,2,4,8,16 seconds)
4) Time required: 4 mins
5) Target: AR
WARNING:
This study is no longer required as science studies are used instead.
desc000069.txt
240000
0
0
Engineering
SnS
234881024
0
0
0
Line width calibration with Slit0 (1" width) [EWxNS = 10"x512, 1"step raster, 30 and 120 sec exp.] b
hh_linewidth_cal_01b
000070 hh_linewidth_cal_01b
Hiro Hara
Engineering
Study 000070:
desc000070.txt
1440000
0
0
Engineering
SnS
139198464
0
0
0
Line width calibration with Slit0 (1" width) [EWxNS = 10"x512, 1"step raster, 30 and 120 sec exp.] t
hh_linewidth_cal_01t
000071 hh_linewidth_cal_01t
Hiro Hara
Engineering
Study 000071:
desc000071.txt
1440000
0
0
Engineering
SnS
139198464
0
0
0
40 arcsec slot study for waves and spicules with SOT (sit n stare)
VHH001_SLOT40_30M
000072 VHH001_SLOT40_30M
Viggo Hansteen
Science
11-Feb-2007
Study 000072:
desc000072.txt
1695747
1
0
Quiet Sun
Scanning
91750400
0
3
3
57
1
40
50s sit and stare, meant for very quiet region oscillation studies
VHH002_SLIT1_1H
000073 VHH002_SLIT1_1H
Viggo Hansteen
Science
11-Feb-2007
Study 000073:
desc000073.txt
3835046
1
0
Quiet Sun
Scanning
302776320
0
0
0
58
1
1
30s sit and stare for quiet sun and active region oscillation study
VHH003_SLIT1_1H
000074 VHH003_SLIT1_1H
Viggo Hansteen
Science
11-Feb-2007
Study 000074:
desc000074.txt
3703644
1
0
Active Region
Scanning
475791360
0
0
0
59
1
1
Line width calibration with Slit0 (1"width) [EWxNS = 10"x512, 1"step raster, 30
HH_LINE_WIDTH_CAL_01
000075 HH_LINE_WIDTH_CAL_01
Hiro Hara
Calibration
11-Feb-2007
Study 000075:
desc000075.txt
1653531
1
0
Quiet Sun
Scanning
154664960
0
0
0
60
1
10
Wavelength cal, AR, 2" slit
regcal007
000076 regcal007
Louisa Bradley
Engineering
Study 000076:
1) Acronym: regcal007
2) Repeats: 1
3) 7 exposures, full ccd, 2" slit
(exposure times: 0.25,0.5,1,2,4,8,16 seconds)
4) Time required: 4 mins
5) Target: AR
WARNING:
This study is no longer required as science studies are used instead.
desc000076.txt
240000
0
0
Engineering
SnS
234881024
0
0
0
Wavelength cal, AR, 40" slot
regcal008
000077 regcal008
Louisa Bradley
Engineering
Study 000077:
1) Acronym: regcal008
2) Repeats: 1
3) 7 exposures, full ccd, 40" slot
(exposure times: 0.25,0.5,1,2,4,8,16 seconds)
4) Time required: 4 mins
5) Target: AR
WARNING:
This study is no longer required as science studies are used instead.
desc000077.txt
240000
0
0
Engineering
SnS
234881024
0
0
0
Wavelength cal, AR, 266" slot
regcal009
000078 regcal009
Louisa Bradley
Engineering
Study 000078:
1) Acronym: regcal009
2) Repeats: 1
3) 7 exposures, full ccd, 266" slot
(exposure times: 0.25,0.5,1,2,4,8,16 seconds)
4) Time required: 4 mins
5) Target: AR
WARNING:
This study is no longer required as science studies are used instead.
desc000078.txt
240000
0
0
Engineering
SnS
234881024
0
0
0
Wavelength cal, AR, 1" slit
regcal010
000079 regcal010
Louisa Bradley
Engineering
Study 000079:
1) Acronym: regcal010
2) Repeats: 1
3) 3 exposures, full ccd, 1" slit
(exposure times: 32, 64 and 128 seconds)
4) Time required: 6 mins
5) Target: AR
WARNING:
This study is no longer required as science studies are used instead.
desc000079.txt
360000
0
0
Engineering
SnS
100663296
0
0
0
Wavelength cal, AR, 2" slit
regcal011
000080 regcal011
Louisa Bradley
Engineering
Study 000080:
1) Acronym: regcal011
2) Repeats: 1
3) 3 exposures, full ccd, 2" slit
(exposure times: 32, 64 and 128 seconds)
4) Time required: 6 mins
5) Target: AR
WARNING:
This study is no longer required as science studies are used instead.
desc000080.txt
360000
0
0
Engineering
SnS
100663296
0
0
0
Wavelength cal, AR, 40" slot
regcal012
000081 regcal012
Louisa Bradley
Engineering
Study 000081:
1) Acronym: regcal012
2) Repeats: 1
3) 3 exposures, full ccd, 40" slot
(exposure times: 32, 64 and 128 seconds)
4) Time required: 6 mins
5) Target: AR
WARNING:
This study is no longer required as science studies are used instead.
desc000081.txt
360000
0
0
Engineering
SnS
100663296
0
0
0
Wavelength cal, AR, 266" slot
regcal013
000082 regcal013
Louisa Bradley
Engineering
Study 000082:
1) Acronym: regcal013
2) Repeats: 1
3) 3 exposures, full ccd, 266" slot
(exposure times: 32, 64 and 128 seconds)
4) Time required: 6 mins
5) Target: AR
WARNING:
This study is no longer required as science studies are used instead.
desc000082.txt
360000
0
0
Engineering
SnS
100663296
0
0
0
Wavelength cal, QS, 1" slit, middle CCD rows
regcal000
000083 regcal000
Louisa Bradley
Engineering
Study 000083:
1) Acronym: regcal000
2) Repeats: 1
3) 6 exposures, full ccd, 1" slit
(exposure times: 10,20,40,80,160 and 600 seconds)
4) Time required: 17 mins
5) Target: QS
WARNING:
This study is no longer required as science studies are used instead.
desc000083.txt
1020000
0
0
Engineering
SnS
201326592
0
0
0
TW; active region study (1)
TW_AR110
000084 TW_AR110
Tetsuya Watanabe
Science
2-Apr-2007
Study 000084:
desc000084.txt
2778293
1
0
Active Region
Scanning
267386880
0
0
0
61
1
120
TW active regio iron study
TW_AR111
000085 TW_AR111
Tetsuya Watanabe
Science
29-Mar-2007
Study 000085:
desc000085.txt
3213526
1
0
Active Region
Scanning
570425344
0
0
0
62
1
256
High cadence sit-and-stare in ARs (improved version of PRY_fast_dens)
PRY_fast_dens_v2
000086 PRY_fast_dens_v2
Peter Young
Science
27-Feb-2007
Study 000086:
Consists of two rasters:
(1) a context raster covering 40x304 arcsec2 with 1" slit
(2) sit-and-stare with 1" slit taking 304" along slit (100 exposures)
Exposure times are 5 seconds, and five lines are included: the core
lines plus the Fe XIII 203.8/202.0 density diagnostic.
USE: The aim is search for high cadence density variations in active
regions.
NOTES: the number of repeats of (2) should be adjusted to fill the
available time slot.
NOTES: this study is preferred to PRY_fast_dens.
desc000086.txt
1041307
2
0
Active Region
Scanning
43892736
0
0
0
44
1
41
45
1
1
Detailed diagnostic study, with slot context. All regions, 30s exposures, slit 0
Diag_40x180_s0_30s
000087 Diag_40x180_s0_30s
Peter Young
Science
2-Apr-2007
Study 000087:
Consists of two rasters:
(1) 230x360 arcsec2 raster with 40" slit; 30 s exposure time
(2) 40X180 arcsec2 raster with 1" slit; 30 s exposure time
Raster (1) gives context information in 16 wavelength windows.
Raster (2) has a very extensive line list that covers virtually all
major EIS lines.
USE: for taking detailed diagnostics at a good cadence over a small
field-of-view. All targets (including flares) are suitable.
WARNING: raster (1) should only be repeated once. Raster (2) should be
repeated to fill available time slot.
WARNING: The study should be placed on the timeline such that the
change from raster (1) to raster (2) does not take place during an SAA
period. Raster (1) lasts for less than 5 minutes so this should be
straightforward to evaluate.
desc000087.txt
1594888
2
0
Active Region
Scanning
73887744
1
3
0
63
1
230
64
1
40
Detailed raster to produce active region velocity map in many lines; has slot context
AR_velocity_map
000088 AR_velocity_map
Peter Young
Science
29-Mar-2007
Study 000088:
Consists of two rasters:
(1) 230x360 arcsec2 raster with 40" slit; 30 s exposure time
(2) 330X304 arcsec2 raster with 1" slit; 40 s exposure time
Raster (1) gives context information in 16 wavelength windows.
Raster (2) has a very extensive line list that covers virtually all
major EIS lines.
USE: produces very detailed diagnostic information over a large
area. Should be run on medium-to-large active regions.
WARNING: raster (1) should only be repeated once.
WARNING: The study should be placed on the timeline such that the
change from raster (1) to raster (2) does not take place during an SAA
period. Raster (1) lasts for less than 5 minutes so this should be
straightforward to evaluate.
desc000088.txt
18922722
2
0
Active Region
Scanning
904900621
1
3
0
63
1
230
65
1
330
Spectral Atlas 3, with slot context raster, 120x120, slit 2, 40s exposure
AR_spectral_atlas_3
000089 AR_spectral_atlas_3
Peter Young
Science
8-May-2007
Study 000089:
desc000089.txt
4154187
2
0
Active Region
Scanning
199913474
1
3
2
63
1
230
66
1
120
Five-arcsecond rapid scan for TR and coronal brightenings (H. Isobe)
DRW001_HI_BRT_SCAN
000090 DRW001_HI_BRT_SCAN
David Williams
Science
27-Feb-2007
Study 000090:
This study is intended to be run on patches of nominally unipolar quiet
Sun or plage, to search for jets and other features at cool temperatures
caused by the churning of the magnetic field.
The study consists of a single raster, with 5 contiguous positions
of EIS's narrow slit, making a narrow but tall scan with 60-second
exposures at each position. This scanning raster is repeated 12 times
to make an approximately one-hour duration study.
It should be run, where possible, in co-ordinated observations with SOT.
This study was originally requested by Hiroaki Isobe of the University of Tokyo.
desc000090.txt
3920400
1
0
Quiet Sun
Scanning
241459200
0
0
0
67
12
5
Alignment slot 266
Alignment_266
000091 Alignment_266
S. Kamio
Science
27-Feb-2007
Study 000091:
Alignment study. One raster, 266" slot, SNS, 2 expoure time (20 and 60) seconds
desc000091.txt
153578
1
0
Quiet Sun
Scanning
24510464
0
1
1
68
1
266
Slot raster
Slot_raster
000092 Slot_raster
Suguru Kamio
Science
29-Mar-2007
Study 000092:
Alignment study, raster scan, 40" slot, 16 exposures (30S) each.
desc000092.txt
557939
1
0
Quiet Sun
Scanning
5662310
0
3
3
69
1
580
GAD003_AR_slot30_SAS
GAD003_AR_slot30_SAS
000093 GAD003_AR_slot30_SAS
George Doschek
Science
29-Mar-2007
Study 000093:
desc000093.txt
2030397
1
0
Active Region
Scanning
77070337
0
3
3
70
1
40
GAD004_AR_slot15_SAS
GAD004_AR_slot15_SAS
000094 GAD004_AR_slot15_SAS
George Doschek
Science
29-Mar-2007
Study 000094:
desc000094.txt
1085397
1
0
Active Region
Scanning
38535168
0
3
3
71
1
40
JAK_256_AR_STUDY
JAK_256_AR_STUDY
000095 JAK_256_AR_STUDY
James Klimchuk
Science
29-Mar-2007
Study 000095:
desc000095.txt
8622991
1
0
Active Region
Scanning
327486264
0
0
0
72
1
257
JAK_40_AR_STUDY
JAK_40_AR_STUDY
000096 JAK_40_AR_STUDY
James Klimchuk
Science
29-Mar-2007
Study 000096:
desc000096.txt
1394563
1
0
Active Region
Scanning
52244890
0
0
0
73
1
41
JAK_SAS_AR_STUDY
JAK_SAS_AR_STUDY
000097 JAK_SAS_AR_STUDY
James Klimchuk
Science
29-Mar-2007
Study 000097:
desc000097.txt
4038293
1
0
Active Region
Scanning
152911874
0
0
0
74
1
1
SI001_FULLCCD_RAST
SI001FullRast
000098 SI001FullRast
Shin Imada
Science
2-Apr-2007
Study 000098:
desc000098.txt
13965526
1
0
Quiet Sun
Scanning
4294967296
0
0
0
75
1
256
Transition Region Brightenings
tr_bright
000099 tr_bright
Danielle Bewsher
Science
29-Mar-2007
Study 000099:
desc000099.txt
4256546
2
0
Quiet Sun
Scanning
116391937
0
2
2
76
1
120
77
1
20
EE study
EE_SUMER_EIS
000100 EE_SUMER_EIS
Gerry Doyle
Science
26-Mar-2007
Study 000100:
*** DO NOT USE ***
Use ee_sumer_eis_p1 and ee_sumer_eis_p2 instead
desc000100.txt
20717861
3
0
Quiet Sun
Scanning
744004002
1
0
3
78
1
101
79
1
40
79
1
40
SYNOP002
SYNOP002
000101 SYNOP002
John Mariska
Science
26-Mar-2007
Study 000101:
Replaced by SYNOP006
desc000101.txt
12370013
1
0
Quiet Sun
Scanning
617401558
0
0
0
80
1
128
SYNOP003_150x_96y_45s_2arcsec_fullCCD
SYNOP003
000102 SYNOP003
John Mariska
Science
26-Mar-2007
Study 000102:
ACRONYM: SYNOP003
desc000102.txt
7404742
1
0
Quiet Sun
Scanning
377487365
0
2
2
81
1
300
raster_before_sit_stare_above_limb_active_region
inn_ar_lmb_sr01
000103 inn_ar_lmb_sr01
Davina Innes
Science
29-Mar-2007
Study 000103:
ACRONYM: inn_ar_lmb_sr01
desc000103.txt
1423362
1
0
Active Region
Scanning
67061351
0
2
2
82
1
122
Sit_n_stare_above_limb_active_region
inn_ar_lmb_ss03
000104 inn_ar_lmb_ss03
Davina Innes
Science
29-Mar-2007
Study 000104:
ACRONYM: inn_ar_lmb_ss03
desc000104.txt
4156190
1
0
Active Region
Scanning
208576515
0
2
2
83
1
2
Raster_across_limb_active_region
inn_ar_lmb_ra01
000105 inn_ar_lmb_ra01
Davina Innes
Science
29-Mar-2007
Study 000105:
ACRONYM: inn_ar_lmb_ra01
desc000105.txt
4138688
1
0
Active Region
Scanning
210370563
0
0
0
84
1
60
Raster_in_the_corona_above_limb_active_region
inn_ar_cor_ra03
000106 inn_ar_cor_ra03
Davina Innes
Science
29-Mar-2007
Study 000106:
ACRONYM: inn_ar_cor_ra03
desc000106.txt
4180485
1
0
Active Region
Scanning
212447235
0
2
2
85
1
60
Slot_Raster_above_limb_active_region
inn_ar_lmb_sl03
000107 inn_ar_lmb_sl03
Davina Innes
Science
29-Mar-2007
Study 000107:
ACRONYM: inn_ar_lmb_sl03
desc000107.txt
635657
1
0
Active Region
Scanning
30932992
0
3
3
86
1
130
Full EIS CCD readout with 12"x512" FOV
EL_FULL_CCD_RASTER
000108 EL_FULL_CCD_RASTER
Enrico Landi
Science
28-Mar-2007
Study 000108:
ACRONYM: EL_FULL_CCD_RASTER
desc000108.txt
2241255
1
0
Active Region
Scanning
93952411
0
2
2
87
1
14
Full EIS CCD readout at single position
EL_FULL_CCD_SINGLE
000109 EL_FULL_CCD_SINGLE
Enrico Landi
Science
28-Mar-2007
Study 000109:
ACRONYM: EL_FULL_CCD_SINGLE
desc000109.txt
4334436
1
0
Active Region
Scanning
161061276
0
2
2
88
1
4
AVERAGE DOPPLER SHIFT IN QS AND AR
RED_SUM_EIS_RAST
000110 RED_SUM_EIS_RAST
Luca Teriac
Science
31-Mar-2007
Study 000110:
ACRONYM: RED_SUM_EIS_RAST
desc000110.txt
3398773
1
0
Quiet Sun
Scanning
161996802
0
0
0
89
1
69
OFF LIMB REFERENCE SPECTRUM
RED_SUM_EIS_SNS_OL
000111 RED_SUM_EIS_SNS_OL
Luca Teriaca
Science
31-Mar-2007
Study 000111:
ACRONYM: RED_SUM_EIS_SNS_OL
desc000111.txt
1951799
1
0
Quiet Sun
Scanning
92569601
0
0
0
90
1
1
Flows in active region
madj_ar_slot
000112 madj_ar_slot
Maria Madjarska
Science
31-Mar-2007
Study 000112:
ACRONYM: madj_ar_slot
desc000112.txt
3555694
1
0
Active Region
Scanning
173408256
0
3
3
91
49
70
Flows in the quiet Sun
madj_qs_slot
000113 madj_qs_slot
Maria Madjraska
Science
31-Mar-2007
Study 000113:
ACRONYM: madj_qs_slot
desc000113.txt
3589856
1
0
Quiet Sun
Scanning
179424440
0
3
3
92
26
70
AR loop abundances with SUMER
el_abund_loop_sumer
000114 el_abund_loop_sumer
Enrico Landi
Science
31-Mar-2007
Study 000114:
ACRONYM: el_abund_loop_sumer
desc000114.txt
3344862
1
0
Active Region
Scanning
138170370
0
0
0
93
1
61
AR loop diagnostics with SUMER
el_loop_diagn_sumer
000115 el_loop_diagn_sumer
Enrico Landi
Science
31-Mar-2007
Study 000115:
ACRONYM: el_loop_diagn_sumer
desc000115.txt
3344862
1
0
Active Region
Scanning
152162306
0
0
0
94
1
61
Abundances in polar plumes with raster and SUMER
EL_abund_plume_SUMER
000116 EL_abund_plume_SUMER
Enrico Landi
Science
2-Apr-2007
Study 000116:
ACRONYM: EL_abund_plume_sumer
desc000116.txt
3338413
1
0
Coronal Hole
Scanning
128398133
0
2
2
95
1
62
Diagnostics of polar plumes with SUMER
EL_loop_plume_SUMER
000117 EL_loop_plume_SUMER
Enrico Landi
Science
2-Apr-2007
Study 000117:
ACRONYM: EL_loop_plume_SUMER
desc000117.txt
3338413
1
0
Coronal Hole
Scanning
145463707
0
2
2
96
1
62
WAVES in CHs, SUMER-EIS study
CH_SUM_EIS
000118 CH_SUM_EIS
Unknown
Science
2-Apr-2007
Study 000118:
ACRONYM: CH_SUM_EIS
desc000118.txt
3595965
2
0
Coronal Hole
Scanning
177356800
0
3
3
97
1
200
98
173
60
Blinker study
BL_SUMER_EIS
000119 BL_SUMER_EIS
Gerry Doyle
Science
5-Apr-2007
Study 000119:
ACRONYM: BL_SUMER_EIS
*** DO NOT USE ***
Use bl_sumer_eis_p1 and bl_sumer_eis_p2 instead
desc000119.txt
11115297
3
0
Quiet Sun
Scanning
434831365
1
0
2
99
1
1
100
1
2
100
1
2
sit_n_slot_on_quiet_region
inn_qr_dsk_sso03
000120 inn_qr_dsk_sso03
Davina Inees
Science
5-Apr-2007
Study 000120:
ACRONYM: inn_qr_dsk_sso03
desc000120.txt
4038293
1
0
Quiet Sun
Scanning
204472323
0
3
3
101
1
40
Energy transport and dynamics in/above chromospheric network
dyn_network
000121 dyn_network
P. Gomory
Science
5-Apr-2007
Study 000121:
ACRONYM: dyn_network
desc000121.txt
12362800
1
0
Quiet Sun
Scanning
506880000
0
3
3
102
10
40
slot_across_disk_active_region
inn_ar_dsk_rso01
000122 inn_ar_dsk_rso01
Unknown
Science
5-Apr-2007
Study 000122:
ACRONYM: inn_ar_dsk_rso01
desc000122.txt
3458412
1
0
Active Region
Scanning
172523520
0
3
3
103
9
192
Blinker study part 1
BL_SUMER_EIS_p1
000123 BL_SUMER_EIS_p1
Gerry Doyle
Science
5-Apr-2007
Study 000123:
ACRONYM: BL_SUMER_EIS_p1
desc000123.txt
252160
1
0
Quiet Sun
Scanning
8257536
0
0
0
99
1
1
Blinker study part2
BL_SUMER_EIS_p2
000124 BL_SUMER_EIS_p2
Gerry Doyle
Science
5-Apr-2007
Study 000124:
ACRONYM: BL_SUMER_EIS_p2
desc000124.txt
462160
1
0
Quiet Sun
Scanning
17612800
0
2
2
100
1
2
EE study part 1
EE_SUMER_EIS_p1
000125 EE_SUMER_EIS_p1
Gerry Doyle
Science
5-Apr-2007
Study 000125:
ACRONYM: EE_SUMER_EIS_p1
desc000125.txt
252160
1
0
Quiet Sun
Scanning
8257536
0
0
0
78
1
101
EE study part 2
EE_SUMER_EIS_p2
000126 EE_SUMER_EIS_p2
Gerry Doyle
Science
5-Apr-2007
Study 000126:
ACRONYM: EE_SUMER_EIS_p2
desc000126.txt
252160
1
0
Quiet Sun
Scanning
8257536
0
3
3
79
1
40
Explosive event study with EIS, SUMER and IBIS
EE_SUM_EIS
000127 EE_SUM_EIS
L. Teriaca
Science
6-Apr-2007
Study 000127:
ACRONYM: EE_SUM_EIS
desc000127.txt
3595965
2
0
Quiet Sun
Scanning
169898734
0
3
3
104
1
200
105
173
60
BP SoHO/Hinode run part 1
BP_SUMER_EIS_p1
000128 BP_SUMER_EIS_p1
Gerry Doyle
Science
6-Apr-2007
Study 000128:
ACRONYM: BP_SUMER_EIS_p1
desc000128.txt
2040356
1
0
Active Region
Scanning
92431975
0
2
2
106
1
82
BP SoHO/Hinode run part 2
BP_SUMER_EIS_p2
000129 BP_SUMER_EIS_p2
Gerry Doyle
Science
6-Apr-2007
Study 000129:
ACRONYM: BP_SUMER_EIS_p2
desc000129.txt
4419099
1
0
Active Region
Scanning
176128002
0
2
2
100
1
2
Active Region Transient Brightenings
cam_artb_cds_a
000130 cam_artb_cds_a
Durgesh Tripathi
Science
13-Apr-2007
Study 000130:
1) Acronym: cam_artb_cds_a_1
2) Target: On-disk active region
3) Type of observation: raster, 2 arcsec slit
4) Exposure time: 10 sec
5) XSIZE = 200 arcsec, YSIZE = 200 ARCSEC
6) Number of exposures: 100
7) Time Required: 21m9s
8) Line List: CAM_LINE_1_CDS
desc000130.txt
1268994
1
0
Active Region
Scanning
97280001
0
2
2
107
1
200
Active Region Transient Brightenings (40 arcsec)
cam_artb_cds_b
000131 cam_artb_cds_b
Durgesh Tripathi
Science
13-Apr-2007
Study 000131:
1) Acronym: cam_artb_cds_b_1
2) Target: On-disk active region, pointing overlying the neutral line
3) Type of observation: sit'n'stare, 40 arcsec slot
4) Exposure time: 20 sec
5) XSIZE = 40 arcsec, YSIZE = 200 ARCSEC
6) Number of Repeats: 1, 60 Exposures (KFJ in consultation with Durgesh)
7) Time Required: 23m20s
8) Line List: CAM_LINE_2_CDS
desc000131.txt
1400400
1
0
Active Region
Scanning
71270400
0
3
3
108
1
40
Active_Region_Transient_Brightenings_v2
cam_artb_cds_c
000132 cam_artb_cds_c
Durgesh Tripathi
Science
13-Apr-2007
Study 000132:
1) Acronym: cam_artb_cds_c_1
2) Target: On-disk active region, pointing overlying the neutral line
3) Type of observation: Raster, 1 arcsec slot
4) Exposure time: 20 sec
5) XSIZE = 120 arcsec, YSIZE = 200 ARCSEC
6) Number of exposures: 120
7) Time Required: 46m18s
8) Line List: CAM_LINE_1_CDS
desc000132.txt
2778293
1
0
Active Region
Scanning
116736001
0
0
0
109
1
120
AR microflares and TR response - joint observations with RHESSI; CONTEXT raster
CAM_ARTB_RHESSI_a_1
000133 CAM_ARTB_RHESSI_a_1
Cristina Chifor
Science
13-Apr-2007
Study 000133:
1) Acronym: CAM_ARTB_RHESSI_a_1
2) Target: on-disk ARs; pointing over the neutral line
3) Type of observation: context raster for the CAM_ARTB_b_1 study; 2 arcsec slit
4) Exposure time: 15 sec
5) XSIZE = 240 arcsec, YSIZE = 240 arcsec
6) Number of exposures: 120
7) Time required: 35m38s
8) Line list: CAM_LINE_1_RHESSI
desc000133.txt
2148293
1
0
Active Region
Scanning
134184961
0
2
2
110
1
240
AR microflares and TR response - joint observations with RHESSI
CAM_ARTB_RHESSI_b_1
000134 CAM_ARTB_RHESSI_b_1
Cristina Chifor
Science
13-Apr-2007
Study 000134:
1) Acronym: CAM_ARTB_RHESSI_b_1
2) Target: on-disk ARs
3) Type of observation: raster; 2 arcsec slit
4) Exposure time: 10 sec
5) XSIZE = 40 arcsec, YSIZE = 120 arcsec
6) Number of repeats: 12, 20 Exposures per raster
7) Time required: 4m9s per raster x 12 repeats = 50m14s
8) Line list: CAM_LINE_1_RHESSI
desc000134.txt
3014088
1
0
Active Region
Scanning
134184960
0
2
2
111
12
40
Fine mirror pzt test
regeng007
000135 regeng007
Louisa Bradley
Engineering
Study 000135:
Engineering study: Fine mirror PZT test
desc000135.txt
270000
0
0
Engineering
SnS
0
0
0
0
Simple and quick 240 arcsec raster for studying filament and its environment with slit 2
fil_rast_s2
000136 fil_rast_s2
Nicolas Labrosse
Science
19-Apr-2007
Study 000136:
ACRONYM: fil_rast_s2
desc000136.txt
6612758
1
0
Filament
Scanning
266443165
0
2
2
112
1
242
HPW014_SLOT266_MOVIE
HPW014_SLOT266_MOVIE
000137 HPW014_SLOT266_MOVIE
Harry Warren
Science
26-Apr-2007
Study 000137:
ACRONYM: HPE014_SLOT266_MOVIE
desc000137.txt
3565489
1
0
Active Region
Scanning
188743682
0
1
1
113
1
266
Active Region context SLOT images.
IUU_SLOT_cntxt_AR_01
000138 IUU_SLOT_cntxt_AR_01
Unknown
Science
26-Apr-2007
Study 000138:
ACRONYM: IUU_SLOT_cntxt_AR_01
desc000138.txt
107116
1
0
Active Region
Scanning
3145728
0
3
3
114
1
40
Quiet Sun context SLOT images.
IUU_SLOT_cntxt_QS_01
000139 IUU_SLOT_cntxt_QS_01
Unknown
Science
26-Apr-2007
Study 000139:
ACRONYM: IUU_SLOT_cntxt_QS_01
desc000139.txt
218678
1
0
Quiet Sun
Scanning
5242880
0
3
3
115
1
40
coronal_wave_study
coronal_wave_study
000140 coronal_wave_study
Gemma Attrill
Science
1-May-2007
Study 000140:
Coronal wave study
The second raster should be repeated as many times as possible. Typical run
is around 5h (3 rasters repeat of the second raster).
The slit/slot should be positioned over quiet Sun, not directly over the
active region of interest. If the active region is in the northern
(southern) hemisphere, please position the slit/slot over quiet Sun,
just south (north) of the active region.
WARNING:
First and second raster runs with 40" slot and 2" slit, respectively.
desc000140.txt
6620889
2
0
Quiet Sun
Scanning
106430465
1
3
2
116
1
120
117
1
200
Off limb study bottom of the ccd
gdz_off_limb1_60
000141 gdz_off_limb1_60
Giulio Del Zanna
Engineering
Study 000141:
Off limb engineering study (CCD bottom 512 rows)
desc000141.txt
4165000
0
0
Engineering
SnS
193488489
0
0
0
SI002_HiCadence_AR
SI002_HiCadence_AR
000142 SI002_HiCadence_AR
Unknown
Science
4-May-2007
Study 000142:
Fast cadence study. Contains 9 rasters
WARNINGS:
--------
*** Multiple slit/slot ****
***********************************************
Add a couple of minutes to the study run time:
6 rasters runs at 10 seconds cadence and more time is needed
for rasters synchronizations
**********************************************
desc000142.txt
1676143
9
0
Active Region
Scanning
458227712
2
3
3
69
1
580
118
1
1
118
1
1
118
1
1
118
1
1
118
1
1
118
1
1
119
1
241
69
1
580
MHC heater settings (pre-eclipse), heaters 1 to 6, May 2010
default_htrs1_6
000143 default_htrs1_6
Khalid al Janabi
Engineering
Study 000143:
Engineering study which performs the following operations:
1) Turn all structure heaters *** OFF ***
2) Configures heaters 1 to 6
WARNING:
*** MUST RUN FIRST (BEFORE default_htrs7_12) ***
desc000143.txt
12000
0
0
Engineering
SnS
0
0
0
0
MHC heater settings (pre-eclipse), heaters 7 to 12, May 2010
default_htrs7_12
000144 default_htrs7_12
Khalid al Janabi
Engineering
Study 000144:
Engineering study which performs the following operations:
1) Configures heaters 7 to 12
2) Set heaters cycle time (100 seconds)
3) Turn all structure heaters *** ON ***
Instructions to planners:
1) run default_htrs1_6
2) Run default_htrs7_12
3) Run regeng015 (trace dump) to verify the heaters setting in the future
WARNING:
*** MUST RUN SECOND (AFTER default_htrs1_6) ***
desc000144.txt
12000
0
0
Engineering
SnS
0
0
0
0
Off-limb quiet Sun spectral atlas; steps 10 arcsec, 21 positions
QS_atlas_offlimb
000145 QS_atlas_offlimb
Peter Young
Science
17-May-2007
Study 000145:
This study consists of one raster:
Full CCD readout; 60s exposures; 1" slit; FOV 211"x512"; step size
10"; duration: 46mins
This study takes complete EIS spectra at different heights above the
limb and will be useful for categorising the EIS spectra in this
region and helping with line identification.
ECLIPSE SEASON: during the eclipse season this study can be scheduled
for the day-time and, if nothing else is run during the orbit, then
the average data rate over the orbit will be the nominal value of 50
kbits/s (since the study duration is half the orbit period).
POINTING: preferably this study should be run at Y=0 (i.e., near the
equator) and the raster field-of-view should extend from just above
the limb (say 10-20 arcsec) out to 220-230 arcsec above the limb. If
the satellite pointing allows, greater heights would also be useful.
WARNING: this study has a data-rate of 100kbits/s. If you run it for 3
hours (for example) you will need to leave a 3 hour gap to prevent EIS
going over its data recorder allocation.
desc000145.txt
2837729
1
0
Quiet Sun
Scanning
295279006
0
0
0
120
1
211
Eclipse raster: takes 60percent of spectrum at enhanced data rate
Eclipse_raster1
000146 Eclipse_raster1
Peter Young
Science
17-May-2007
Study 000146:
A study specially designed for the eclipse season. It consists of two
rasters:
(1) 230x360 arcsec^2 raster with 40" slit; 30s exposure time
(2) 105x178 arcsec^2 raster with 1" slit; 40s exposure time
The study is designed to be run once during the day period of the
eclipse season. For 6-7 weeks of the eclipse period, the day-time part
of the orbit lasts about 80-85 minutes. This study lasts for about 82
minutes, so will fit in the day period with minimal loss of data. By
running at 60 kbits/s, it makes use of the dead-time during night to
take data at a higher rate.
The study has four very large wavelength windows that take the parts
of the spectrum with the highest effective area. About 60% of the
entire spectrum is taken.
WARNING:
1 - Multiple Slit/Slot
2 - Data rate > 50 Kbit/sec
desc000146.txt
4960539
2
0
Active Region
Scanning
308142903
1
3
0
63
1
230
121
1
107
kpd01_qs_1slit_55stp_1ac_60s
kpd01_qs_slit_60s
000147 kpd01_qs_slit_60s
Ken Dere
Science
21-May-2007
Study 000147:
This study is for viewing the quiet sun.
It consists of a single raster at 1 arc-sec steps with 60s exposure
times. The length of the sequence is limited so that it can be placed
between SAA crossings and no data is lost. With a series of
these studies, the evolution of the quiet sun can be
followed at all positions in the raster without interference from
the SAA. Data rate is low so 48 pixel windows, at the minimum,
are used. High temperature lines are included in case
something interesting happens.
In the end, the author would like a series of these studies run over
the course of 1 day for suitable pointings in the quiet sun. Each
study should be started after the end of an SAA or a sun-center repointing.
Warning:
None
desc000147.txt
3660537
1
0
Quiet Sun
Scanning
189372828
0
0
0
122
1
56
kpd01_qs_slot40_3stp_15as_60s_0rpt
kpd01_qs_slot_60m
000148 kpd01_qs_slot_60m
Ken Dere
Science
21-May-2007
Study 000148:
desc000148.txt
282360
1
0
Quiet Sun
Scanning
7340032
0
3
3
123
1
85
CMEO slot study
cmeo_slot_study
000149 cmeo_slot_study
Danielle Bewsher
Science
21-May-2007
Study 000149:
CME Onset slot study:
Slit/slot: 40" slot
No of fine mirror steps: 5
Step size: 40"
Total spatial width: 240"
Window height (solar-y): 328 pixels
Exposure time: 30 seconds
Cadence 3m 20s
Compression: DCPM
Data rate: 49.4965 kbits/second
Notes to planners
-----------------
Both of the CME onset studies:
cmeo_slot and
cmeo_slit
are designed to observe coronal dimming (on
the limb of the Sun) which is associated with mass ejection. Pointing should
be at an active region on the solar limb. In solar-y, the raster should be
centred on the active region. In solar-x, the raster should overlap the limb
slightly, but have the majority of the raster above the limb.
We are trying both slit and slot rasters to observe coronal dimming. They do
not have to be run at the same time. However, it would be beneficial for
both studies to be run on the same active region once (minimum 6 hours
each), so that we can determine which study is best for this type of
observation.
In each study, there is one raster, which should be repeated to fill the
available time.
WARNING:
None
desc000149.txt
223290
1
0
Active Region
Scanning
10176921
0
3
3
124
1
240
CME onset slit study
cmeo_slit_study
000150 cmeo_slit_study
Danielle Bewsher
Science
21-May-2007
Study 000150:
CME Onset slit study:
Slit/slot: 2" slit
No of fine mirror steps: 119
Step size: 2"
Total spatial width: 240"
Window height (solar-y): 504 pixels
Exposure time: 30 seconds
Cadence 1h 6m 6 seconds
Compression: DCPM
Data rate: 49.6998 kbits/second
Notes to planners
-----------------
Both of the CME onset studies:
cmeo_slot and
cmeo_slit
are designed to observe coronal dimming (on
the limb of the Sun) which is associated with mass ejection. Pointing should
be at an active region on the solar limb. In solar-y, the raster should be
centred on the active region. In solar-x, the raster should overlap the limb
slightly, but have the majority of the raster above the limb.
We are trying both slit and slot rasters to observe coronal dimming. They do
not have to be run at the same time. However, it would be beneficial for
both studies to be run on the same active region once (minimum 6 hours
each), so that we can determine which study is best for this type of
observation.
In each study, there is one raster, which should be repeated to fill the
available time.
WARNING:
None
desc000150.txt
4038293
1
0
Active Region
Scanning
204374019
0
2
2
125
1
240
SK_AR1_31x256c
SK_AR1_31x256c
000151 SK_AR1_31x256c
Suguru Kamio
Science
22-May-2007
Study 000151:
FOV: 31"x 256"
slit: 1"
exposure: 3 sec
cadence: 20sec
scan step: 10"
number of slit positions: 4
desc000151.txt
42960
1
0
Active Region
Scanning
961194
0
0
0
126
1
31
SK_AR1_50x320c
SK_AR1_50x320c
000152 SK_AR1_50x320c
Suguru Kamio
Science
22-May-2007
Study 000152:
FOV: 50"x320"
slit: 1"
exposure: 5 sec
cadence: 180sec
scan step: 2"
number of slit positions: 25
date rate: 38kbps with 20% compression (JPEG95)
desc000152.txt
202874
1
0
Active Region
Scanning
7509333
0
0
0
127
1
49
SK_AR2_32x200c
SK_AR2_32x200c
000153 SK_AR2_32x200c
Suguru Kamio
Science
22-May-2007
Study 000153:
FOV: 32" x 200"
slit: 2"
exposure: 1.5sec
cadence: 15sec
scan step: 10"
number of slit positions: 4
desc000153.txt
37334
1
0
Active Region
Scanning
750933
0
2
2
128
1
32
Chromospheric Evaporation During Solar Flares
chromo_evap_rm
000154 chromo_evap_rm
Ryan Milligan
Science
24-May-2007
Study 000154:
The chromo_evap_rm study comprises 15 repeats of the above raster
totaling one hour of observing time. This can be increased if there is
an exceptional target. The spectral windows are wide enough to allow
the detection to Doppler velocities up to 500 km/s. Lossless compression
has been applied resulting in a data rate of 48 kbit/s.
We request that the chromo_evap_rm study be run only when an active
region with a complex magnetic topology is within approximately
600 arcseconds of disc centre (for accurate line-of-sight velocity
measurements). Joint observations with SOT will provide
information on the magnetic field topology of the flaring region that
can be compared with theoretical models. XRT observations will enable
density and temperature measurements of the flaring plasma.
WARNING:
None
desc000154.txt
3623205
1
0
Flare
Scanning
177438720
0
2
2
129
15
152
SK_AR1_40x256i_ss10
SK_AR1_40x256i
000155 SK_AR1_40x256i
Suguru Kamio
Science
24-May-2007
Study 000155:
SK_AR1_40x256i
FOV: 40" x 256" (interleaved)
cadence: 20sec * 10 times
200 sec to compose a complete raster
WARNING:
None
desc000155.txt
240600
10
0
Active Region
Scanning
9611940
0
0
0
126
1
31
126
1
31
126
1
31
126
1
31
126
1
31
126
1
31
126
1
31
126
1
31
126
1
31
126
1
31
SK_AR1_4x256p
SK_AR1_4x256p
000156 SK_AR1_4x256p
Suguru Kamio
Science
24-May-2007
Study 000156:
SK_AR1_4x256p
FOV: 4"x 256"
slit: 1"
exposure: 3 sec
cadence: 20sec
scan step: 1"
number of slit positions: 4
WARNING:
None
desc000156.txt
42960
1
0
Active Region
Scanning
961194
0
0
0
130
1
4
SK_AR2_40x200i_ss10
SK_AR2_40x200i
000157 SK_AR2_40x200i
Suguru Kamio
Science
24-May-2007
Study 000157:
SK_AR2_40x200i
FOV: 40" x 200" (interleaved)
cadence: 15sec * 5 times
75 sec to compose a complete raster
WARNING:
None
desc000157.txt
102670
5
0
Active Region
Scanning
3754665
0
2
2
128
1
32
128
1
32
128
1
32
128
1
32
128
1
32
FILL001_40arcsec_1arcsec_30s_90s
FILL001
000158 FILL001
John Mariska
Science
24-May-2007
Study 000158:
FILL001: Cloned from SYNOP001
Description: Short gaps filling study, Full CCD.
Instructions to planners:
Use SYNOP001 for *REAL* SYNOP studies. Use this study for timeline gaps
filling. This study consists of:
1) 40" context raster
2) 1" slit SNS raster
The second raster run-time can be increased by increasing the raster repeat.
WARNING:
SLIT/SLOT exchange
desc000158.txt
287206
2
0
Quiet Sun
Scanning
67108864
1
3
0
31
1
40
32
1
1
SK_AR40_movie
SK_AR40_movie
000159 SK_AR40_movie
Suguru Kamio
Science
25-May-2007
Study 000159:
SK_AR40_movie
FOV: 40" x 200"
slot: 40"
exposure: 3 sec
cadence: 5 sec
date rate: 45kbps with 15% compression (JPEG92)
WARNING:
None
desc000159.txt
534000
1
0
Active Region
Scanning
28160000
0
3
3
131
100
40
SK_AR2_40x200i_ss10_DONT_USE
SK_AR2_40x200i_NULL
000160 SK_AR2_40x200i_NULL
Suguru Kamio
Science
25-May-2007
Study 000160:
SK_AR2_40x200i
** DO NOT USE ** (imported by a mistake). Use ID 157
desc000160.txt
102670
5
0
Active Region
Scanning
3754665
0
2
2
128
1
32
128
1
32
128
1
32
128
1
32
128
1
32
SK_AR2_8x200p
SK_AR2_8x200p
000161 SK_AR2_8x200p
Suguru Kamio
Science
25-May-2007
Study 000161:
SK_AR2_8x200p
FOV: 8" x 200"
slit: 2"
exposure: 1.5sec
cadence: 15sec
scan step: 2"
number of slit positions: 4
WARNING:
None
desc000161.txt
37334
1
0
Active Region
Scanning
750933
0
2
2
132
1
8
SK_AR2_50x240p
SK_AR2_50x240p
000162 SK_AR2_50x240p
Suguru Kamio
Science
25-May-2007
Study 000162:
SK_AR2_50x240p
FOV: 50"x240"
slit: 2"
exposure: 2sec
cadence: 106 sec
scan step 2"
number of slit positions: 25
date rate: 49kbps with 20% compression (JPEG95)
WARNING:
None
desc000162.txt
128963
1
0
Active Region
Scanning
5632000
0
2
2
133
1
50
Quiet Sun Network Brightening
cam_qs_40as_slot
000163 cam_qs_40as_slot
Giulio Del Zanna
Science
31-May-2007
Study 000163:
1) Acronym: cam_qs_40as_slot_1
2) Repeats: 40
3) Fast raster (120" x 360") with 40" slot
4) Total Time required: 1 hr, 7 mins
5) Target: Quiet Sun
Instruction toplanners:
1) Run cam_qs_2as_context_1 before and after this study
2) SUPPORTING OBSERVATIONS
Hinode/SOT vector magnetograms of the target active region are
fundamental to measure the evolution of the magnetic fields
at the network boundaries.
Imaging support by Hinode/XRT is requested, to cover an area of
360"x360" in high-cadence (1m). They will provide important additional
information on high-temperature events.
WARNING:
None
desc000163.txt
4038300
1
0
Quiet Sun
Scanning
193536000
0
3
3
134
40
120
Quiest Sun Network Brightening
cam_qs_2as_context
000164 cam_qs_2as_context
Giulio Del Zanna
Science
7-Feb-2008
Study 000164:
1) Acronym: cam_qs_2as_context_1
2) repeats: 1
3) Context raster (120" x 360") using 2 arcsec slit
4) Time required: 33 mins 28 secs
5) Target: Quiet Sun
WARNING:
None
desc000164.txt
2030397
1
0
Quiet Sun
Scanning
108060846
0
2
2
135
1
120
Quiet Sun Network Brightening Velocity
cam_qs_2as_velo
000165 cam_qs_2as_velo
Giulio Del Zanna
Science
31-May-2007
Study 000165:
1) Acronym: cam_qs_2as_velo_1
2) Repeats: 20
3) Fast, small raster (20" x 200") using 2" slit
4) Total Time required: 59 mins 25 secs
5) Target: Quiet Sun
Instructions to planner:
1) Run cam_qs_2as_context_1 before and after this study
2) SUPPORTING OBSERVATIONS
Hinode/SOT vector magnetograms of the target active region are
fundamental to measure the evolution of the magnetic fields
at the network boundaries.
Imaging support by Hinode/XRT is requested, to cover an area of
360"x360" in high-cadence (1m). They will provide important additional
information on high-temperature events.
WARNING:
None
desc000165.txt
3565480
1
0
Quiet Sun
Scanning
189440000
0
2
2
136
20
20
Dark exposures (100s, 100s, 150s, 150s)
regcal073
000166 regcal073
Louisa Bradley
Engineering
Study 000166:
1) Acronym: regcal073
2) Repeats: 1
3) 4 dark exposures (100s, 100s, 150s, 150s), full ccd
4) Time required: 12 mins
5) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000166.txt
720000
0
0
Engineering
SnS
67108864
0
0
0
Dark exposures including overscan pixels
regcal074
000167 regcal074
Louisa Bradley
Engineering
Study 000167:
1) Acronym: regcal074
2) Repeats: 1
3) 2 dark exposures, full ccd including overscan pixels
4) Time required: 5 mins
5) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000167.txt
300000
0
0
Engineering
SnS
33554432
0
0
0
AR microflares and TR response - joint observations with RHESSI (v2)
CAM_ARTB_RHESSI_b_2
000168 CAM_ARTB_RHESSI_b_2
Peter Young
Science
13-Jun-2007
Study 000168:
An updated version of CAM_ARTB_RHESSI_b_1 that makes better use of the
EIS data rate. The FOV in Y has been increased to 144 arcsec (from
120), and the line list has been expanded.
This version has been designed for a coronal hole jet campaign (June
2007).
1) Acronym: CAM_ARTB_RHESSI_b_2
2) Target: on-disk ARs
3) Type of observation: raster; 2 arcsec slit
4) Exposure time: 10 sec
5) XSIZE = 40 arcsec, YSIZE = 144 arcsec
6) Number of repeats: 12, 20 Exposures per raster
7) Time required: 4m9s per raster x 12 repeats = 50m14s
8) Line list: CAM_LINE_2_RHESSI
Target: on-disk ARs
WARNING:
None
desc000168.txt
271799
1
0
Active Region
Scanning
12902400
0
2
2
137
1
40
GDZ_SLOT_AR1_480x360_2"slit
GDZ_SLOT_AR1_480x360
000169 GDZ_SLOT_AR1_480x360
Giulio Del Zanna
Science
13-Jun-2007
Study 000169:
ACRONYM: GDZ_SLOT_AR1_480x360
A fast context raster covering 480"x360" with the 40" slit in 6m,
25s exposures. This should provide context images.
TARGET:
Any small/medium-size quiescent active region.
It is important that the AR fits the 360"x288" FOV of
the context raster.
WARNING:
Part of three studies
a) Run GDZ_360x288_AR_CONT2 context raster (17m)
b) Run GDZ_SLOT_AR1_480x360 context raster (6m)
c) Run GDZ_DENS_20x240_ARL1 10 times (25m)
d) Run GDZ_SLOT_AR1_480x360 once (6m)
e) Run GDZ_360x288_AR_CONT2 once (17m)
f) Run GDZ_SLOT_AR1_480x360 once (6m)
g) Run GDZ_DENS_20x240_ARL1 10 times (25m)
h) Run GDZ_SLOT_AR1_480x360 once (6m)
i) Run GDZ_360x288_AR_CONT2 once (17m)
TOTAL DURATION: 2h 5m
desc000169.txt
361079
1
0
Active Region
Scanning
16588800
0
3
3
138
1
480
GDZ_360x288_AR_CONT2_2"slit
GDZ_360x288_AR_CONT2
000170 GDZ_360x288_AR_CONT2
Giulio Del Zanna
Science
13-Jun-2007
Study 000170:
ACRONYM: GDZ_360x288_AR_CONT2
A context raster, large enough (360"x288) to cover a medium-size
active region, in less than 17m with the 2" slit (it is a sparse
raster with 6s exposure times).
This should cover the entire extent of the active region loops.
It is important that the loop legs are observed.
This study will provide densities in the legs of the loops (Mg VII)
and along the loop (Fe X, XII), plus velocity measurements.
Target:
Any small/medium-size quiescent active region.
It is important that the AR fits the 360"x288" FOV of
the context raster.
WARNING:
Part of three studies
a) Run GDZ_360x288_AR_CONT2 context raster (17m)
b) Run GDZ_SLOT_AR1_480x360 context raster (6m)
c) Run GDZ_DENS_20x240_ARL1 10 times (25m)
d) Run GDZ_SLOT_AR1_480x360 once (6m)
e) Run GDZ_360x288_AR_CONT2 once (17m)
f) Run GDZ_SLOT_AR1_480x360 once (6m)
g) Run GDZ_DENS_20x240_ARL1 10 times (25m)
h) Run GDZ_SLOT_AR1_480x360 once (6m)
i) Run GDZ_360x288_AR_CONT2 once (17m)
TOTAL DURATION: 2h 5m
desc000170.txt
1014293
1
0
Active Region
Scanning
51609601
0
2
2
139
1
359
GDZ_DENS_20x240_ARL1_2"slit
GDZ_DENS_20x240_ARL1
000171 GDZ_DENS_20x240_ARL1
Giulio Del Zanna
Science
13-Jun-2007
Study 000171:
ACRONYM: GDZ_DENS_20x240_ARL1
Covers a small area (20"x240") with high cadence (2m 30s) with the 2"
slit and 10s exposures. This should be pointed near quiescent loop-tops
(centre of the active region)
Target:
Any small/medium-size quiescent active region.
It is important that the AR fits the 360"x288" FOV of
the context raster.
WARNING:
Part of three studies
a) Run GDZ_360x288_AR_CONT2 context raster (17m)
b) Run GDZ_SLOT_AR1_480x360 context raster (6m)
c) Run GDZ_DENS_20x240_ARL1 10 times (25m)
d) Run GDZ_SLOT_AR1_480x360 once (6m)
e) Run GDZ_360x288_AR_CONT2 once (17m)
f) Run GDZ_SLOT_AR1_480x360 once (6m)
g) Run GDZ_DENS_20x240_ARL1 10 times (25m)
h) Run GDZ_SLOT_AR1_480x360 once (6m)
i) Run GDZ_360x288_AR_CONT2 once (17m)
TOTAL DURATION: 2h 5m
desc000171.txt
147149
1
0
Active Region
Scanning
7270400
0
2
2
140
1
20
Wide Slot Full FOV Fast Raster
DHB_DRW_001
000172 DHB_DRW_001
David Brooks
Science
15-Jun-2007
Study 000172:
ACRONYM: dhb_drw_001
Wide Slot Full FOV Fast Raster:
This study uses the wide slot to raster across the extended wide slot
field of view (856"x512") taking images in He II 256A and Fe XV 284A with
a 91s cadence. It can be used on any target but was intended for covering
a large region of the poles, either for an entire coronal hole or polar
jet studies. The study duration is just under 30 mins in total so that it
can be used to fill awkward gaps and also be repeated to fill most
observation blocks in the daily plan.
WARNING:
High data rate
desc000172.txt
1767840
1
0
Coronal Hole
Scanning
143445193
0
1
1
141
19
854
AR microflares and TR response - ** HIGH DATA RATE STUDY **
CAM_ARTB_RHES_b_2_HI
000173 CAM_ARTB_RHES_b_2_HI
Peter Young
Science
15-Jun-2007
Study 000173:
This is identical to CAM_ARTB_RHESSI_b_2 except that it takes 368
arcsec along the slit instead of 144 arcsec.
1) Acronym: CAM_ARTB_RHESSI_b_2_hi
2) Target: on-disk ARs
3) Type of observation: raster; 2 arcsec slit
4) Exposure time: 10 sec
5) XSIZE = 40 arcsec, YSIZE = 368 arcsec
6) Number of repeats: 1, 20 Exposures per raster
7) Time required: 4m9s per raster x 12 repeats = 50m14s
8) Line list: CAM_LINE_2_RHESSI
TARGET: on-disk ARs
WARNING:
This study has a high data rate (120 kbits/second post-data compression) and
is *ONLY* for use when SOT is switched off and thus EIS has a 50% allocation
on the DR.
desc000173.txt
271799
1
0
Active Region
Scanning
32972800
0
2
2
142
1
40
A search for fast magnetoacoustic waves in active region loops
arm_fastslot_waves
000174 arm_fastslot_waves
Gerry Doyle
Science
22-Jun-2007
Study 000174:
ACRONYM: arm_fastslot_wave
Search for fast magnetoacoustic waves in active region loops
Target: Active region on disk showing many distinct loops, area to be imaged must include evidence of loops
Seven rasters study:
arm_raster_ar duration 20m
arm_fastslot duration 1h11m
arm_fastslot duration 1h11m
arm_raster_ar duration 20m
arm_fastslot duration 1h11m
arm_fastslot_ar duration 1h11m
arm_raster_ar duration 20m
Total Duration: 5h42m
WARNING:
Multiple SLA use
desc000174.txt
20535995
7
0
Active Region
Scanning
987989358
4
2
2
143
1
82
144
1
40
144
1
40
143
1
82
144
1
40
144
1
40
143
1
82
Off-limb line width measurements
arm_line_width
000175 arm_line_width
Gerry Doyle
Science
22-Jun-2007
Study 000175:
ACRONYM: arm_line_width
DESCRIPTION: Off-limb line width measurements
TARGET: Off-limb region at the solar poles. Slit to be positioned so
that all of the slit is off-limb with the end of the slit just touching the
limb... duration 4h28m
Observe both the N. & S.
WARNING:
None
desc000175.txt
16128459
1
0
Coronal Hole
Scanning
198574085
0
2
2
145
1
202
Loop electron density measurements
arm_loop_ne
000176 arm_loop_ne
Gerry Doyle
Science
22-Jun-2007
Study 000176:
ACRONYM: arm_loop_ne
Loop density measurement
Target: Active region on disk showing many distinct loops, area to be imaged must include evidence of loops
arm_raster_ar 20m
arm_loop_ne_slot 1h28m
arm_loop_ne_slit 24m
arm_loop_ne_slot 1h28m
arm_loop_ne_slit 24m
arm_raster_ar 20m
Total Duration: 4h25m
WARNING:
Multiple SLA use
desc000176.txt
15925574
6
0
Active Region
Scanning
680686950
4
2
2
146
1
82
147
1
40
148
1
2
147
1
40
148
1
2
146
1
82
AR loop temperature and density analysis - sns
ARdiag_sns
000177 ARdiag_sns
Jane Noglik
Science
22-Jun-2007
Study 000177:
ACRONYM: ardiag_sns
This study is intended to be run on an active region. It begin by taking
a context raster with the 40" slot of the active region.
The study ardiag_sns_1 then moves to a sit and stare mode with the 1" slit
to obtain high temporal cadence data (10 secs) of a particular point
along a visible loop structure within the active region. Either the apex
or the footpoint of a structure is preferable depending on what can be seen.
The duration and data rate for this study is 52mins 52secs and 30.02 kbps
respectively.
The context raster is then run again at the end of study. The
DCPM (lossless) data compression scheme is used for the study.
If the active region is on the disk, SOT magnetograms are required. At all
times concurrent XRT data is required.
WARNING:
1) Multiple SLA use
2) This study uses 1, 10s exposure raster, repeated 200 times. Raster
synchronisation needs more time time.
**** Add 10% to the study run time **** and re-adjust % if necessary.
desc000177.txt
3172080
3
0
Active Region
Scanning
117021040
2
3
3
149
1
240
150
200
1
149
1
240
AR temperature and density diagnostics - high cadence rasters
ARdiagn_hcadrast
000178 ARdiagn_hcadrast
Jane Noglik
Science
22-Jun-2007
Study 000178:
ACRONYM: ardiagn_hcadrast
This study is intended to be run on an active region. It begin by taking
a context raster with the 40" slot of the active region.
Study ardiagn_hcadrast_1 uses also uses the 1" slit. This time a rastered
scan of the central 120" of the active region, using both a 10 second
cadence and a 5 second candence are taken. The duration and data rate
for this study is 51mins 2secs and 30.36 kbps respectively.
The context raster is then run again at the end of study. The
DCPM (lossless) data compression scheme is used for the study.
If the active region is on the disk, SOT magnetograms are required.
At all times concurrent XRT data is required.
WARNING:
Multiple SLA use
desc000178.txt
3061846
4
0
Active Region
Scanning
114239078
2
3
3
149
1
240
151
1
121
152
1
121
149
1
240
Loop footpoints study - many cool lines plus coronal lines
PRY_footpoints_v2
000179 PRY_footpoints_v2
Peter Young
Science
27-Jun-2007
Study 000179:
ACRONYM: PRY_footpoints_v2
USAGE: intended for the observation of footpoints of TRACE loops, so CO
should use EIT or TRACE 171 images for pointing. The 2nd raster should
be repeated to fill the available time slot.
Consists of two rasters:
(1) 560x512 arcsec2 context raster with 40" slit; 10 s exposures
(2) 100x240 arcsec2 raster with 2" slit; 25 s exposure
The line list contains many cool lines and so is suitable for the
study of loop footpoints and TR brightenings. It also contains all
useful flare and coronal lines, and so it can be used for other AR
observations.
WARNINGS:
1) the initial context raster has a high data rate and should
only be run once once.
2) Multiple SLA use
desc000179.txt
1621721
2
0
Active Region
Scanning
90296322
1
3
2
153
1
600
154
1
100
1"slit, FOV: EWxNS=180"x512", 3" step, 60 raster positions, 50sec exp.
HH_FWHM_CAL_Norikura
000180 HH_FWHM_CAL_Norikura
Hiro Hara
Science
27-Jun-2007
Study 000180:
ACRONYM: hh_fwhm_cal_norikura
TARGET: AR at the limb
DESCRIPTION: This study is used for calibration of line width by using the
visible light coronal emission lines of the same Fe ionization. Fe X,
Fe XI, Fe XIII, and Fe XIV lines are the lines to be compared. Hot
lines for flares are also contained.
1"slit, FOV: EWxNS=180"x512", 3" step, 60 raster positions, 50sec exp.
WARNING:
None
desc000180.txt
3290397
1
0
Active Region
Scanning
157286404
0
0
0
155
1
178
1" slit, FOV: EWxNS=200"x256", 1" step, 200 raster positions, 6.0 sec exp.
HH_AR+FLR_RAS_N02
000181 HH_AR+FLR_RAS_N02
Hiro Hara
Science
27-Jun-2007
Study 000181:
ACRONYM: hh_ar+flr_ras_n02
TARGET: AR
DESCRIPTION: This is used for observations of active regions. Hot lines for
flares are also contained. The window size for hot lines is wider
than that of the previous version, HH_AR+FLR_RAS_N01, to detect high speed
flows.
1" slit, FOV: EWxNS=200"x256", 1" step, 200 raster positions, 6.0
sec exp.
WARNING:
None
desc000181.txt
1675489
1
0
Active Region
Scanning
69905068
0
0
0
156
1
200
1" slit, FOV: EWxNS=200"x256", 10" step, 20 raster positions, 6sec exp.
HH_AR+FLR_RAS_H02
000182 HH_AR+FLR_RAS_H02
Hiro Hara
Science
27-Jun-2007
Study 000182:
ACRONYM: hh_ar+flr_ras_h02
*** RECURSIVE ***
TARGET: AR
DESCRIPTION: This is used for observations of active regions. Hot lines for
flares are also contained. The window size for hot lines is wider
than that of the previous version, HH_AR+FLR_RAS_H01, to detect high speed
flows.
1" slit, FOV: EWxNS=200"x256", 1" step, 200 raster positions, 6.0 sec exp.
WARNING:
None
desc000182.txt
1688990
10
1
Active Region
Scanning
76895567
0
0
0
157
1
191
158
1
191
159
1
191
160
1
191
161
1
191
162
1
191
163
1
191
164
1
191
165
1
191
166
1
191
St Andrews Loop Oscillations
StA_loop
000183 StA_loop
Danielle Bewsher
Science
9-Jul-2007
Study 000183:
ACRONYM: STA_loop
Objective:
----------
to investigate the morphology of coronal loops which support longitudinal
intensity perturbations, the nature of the (quasi-) periodic driver and
the evolution of the perturbation as they travel through the different
temperature regions of the solar atmosphere.
Conditions Necessary to Run & Pointing:
---------------------------------------
Occurrence of a relatively quiescent (non-flaring) coronal loop system
either on the disk or limb. Involvement of, at a minimum, Hinode/EIS,
SOHO/CDS and TRACE. Additional support from Hinode/XRT and Hinode/SOT/FPP
NOTES to planners:
-----------------
(i) The planner should use the study as defined, with one 'StA_loop
2" raster, followed by n repeats of 'StA_loop1' raster to fill the available
time slot.
(ii) The planner should not repeatedly switch between these
rasters 1 and 2 in a study during a SAA would be extremely beneficial.
(iii) When being run as part of a JOP, the high-cadence (single slit) runs
of Hinode/EIS should occur at the same time as the TRACE and Hinode/XRT
high-cadence runs.
Raster 2
Slit/slot: 2" slit
No of slit positions: 60
Total Spatial Width: 120"
Pixels in solar-y: 512
Exposure time: 30 seconds
Cadence: 33 minutes 27 seconds
Data rate: 38 kbits/s
Raster 1
Slit/slot: 40" slot
No of pointing positions: 1
Total spatial width: 80"
Pixels in solar-y: 416
Exposure time: 30 seconds
Cadence: 1 minute 6 seconds
Data rate: 38 kbits/s
WARNING:
Avoid rasters switching within SAA
desc000183.txt
2098827
2
0
Active Region
Scanning
99350938
1
2
3
167
1
120
168
1
80
Fe_Opacity
Fe_Opacity
000184 Fe_Opacity
Unknown
Science
9-Jul-2007
Study 000184:
**** OBSOLETE *** USE STUDY #185
desc000184.txt
5020943
1
0
Active Region
Scanning
283823313
0
0
0
169
1
41
Fe_Opacity_v2
Fe_Opacity_v2
000185 Fe_Opacity_v2
Unknown
Science
9-Jul-2007
Study 000185:
ACRONYM: Fe_Opacity
The goal of this project is to study the opacity characteristics of coronal
loops. We plan to examine line ratios of Fe XV ions and search for signatures
of intensity enhancements, within the loop structures, which will indicate
optically thick plasma conditions. The degree of intensity enhancement is
predicted to depend on the plasma geometry and angle of observation, and
hence it is necessary to study emission features in an active region loop as
it rotates from the solar limb to disk centre (or vice-versa). Such data,
combined with simultaneous observations from other Hinode instrumentation,
will provide detailed information on the loop morphology, and aid in the
evaluation of 3-dimensional loop parameters.
TARGET: Coronal loop (same loop for all observations)
Since it is necessary to image the same coronal loop structure as it
rotates from limb to disk centre (or vice-versa), a time delay between
successive observations of approximately 24 hours would be very beneficial.
This will allow us to build up an accurate picture of the 3-D structure of
the loop.
Frequency of Observations: One complete raster per day using 1" slit
Raster detail:
Exposure Time: 10 sec
XSIZE = 400"
YSIZE = 512"
Number of Exposures per raster = 400
Slit step size = 1"
Time Required = 1hr 23m 18s per day
WARNING:
None
desc000185.txt
5020943
1
0
Active Region
Scanning
283823313
0
0
0
170
1
401
AR Loop Movie With 40" Slot in Cooler Coronal Lines
COOL_AR_MOVIE_r100x1
000186 COOL_AR_MOVIE_r100x1
Mike Marsh
Science
9-Jul-2007
Study 000186:
ACRONYM: COOL_AR_MOVIE_r100x1
Target: Quiescent active region loops.
Study duration: 21m8s (3+ study repeats 1h2m41s)
Hinode support:
XRT observations are requested to provide 'Dynamics' observations. High
cadence 512x512, no binning, observations are requested in the Ti_poly
filter with 20s exposure and ~30s cadence, or alternatively 368x368
images if required to obtain high cadence.
SOT observations are requested, allowing simultaneous observations of the
photospheric G-band & Ca H intensity, Doppler velocity and vector magnetic
field.
HINODE/SOT Observables: High cadence BFI optical filtergrams full FOV - Ca
II H, G-band, WL; Dopplergrams; SP maps 164"x164", 0.16" sampling.
WARNING:
None
desc000186.txt
1268994
1
0
Active Region
Scanning
131072000
0
3
3
171
1
40
SK_CH1_55x512
SK_CH1_55x512
000187 SK_CH1_55x512
Suguru Kamio
Science
9-Jul-2007
Study 000187:
ACRONYM: SK_CH1_55x512
Aimed at studying dynamics in coronal hole.
55"x512" normal raster followed by coarse rasters of 6" step.
Use 1" slit with 30 sec exposure.
desc000187.txt
5211062
2
0
Coronal Hole
Scanning
176073385
0
0
0
172
1
55
173
10
55
SK_CH2_56x512
SK_CH2_56x512
000188 SK_CH2_56x512
Suguru Kamio
Science
9-Jul-2007
Study 000188:
ACRONYM: SK_CH2_56x512
Aimed at studying dynamics in coronal hole with high cadence.
56"x512" normal raster followed by coarse rasters of 6" step.
Use 2" slit with 15 sec exposure.
desc000188.txt
2291508
2
0
Coronal Hole
Scanning
117440512
0
2
2
174
1
56
175
10
56
Dark exposures (0s, 0s, 100s, 100s)
regcal075
000189 regcal075
Louisa Bradley
Engineering
Study 000189:
1) Acronym: regcal075
2) Repeats: 1
3) 4 dark exposures (0s, 0s, 100s, 100s), full ccd
4) Time required: 8 mins
5) Target: None (shutter closed)
WARNING:
None
desc000189.txt
480000
0
0
Engineering
SnS
67108864
0
0
0
Initialise the MHC (V 20-AUG-08)
mhc_init
000190 mhc_init
Khalid al Janabi
Engineering
Study 000190:
Acronym: mhc_init
Initialise the MHC (e.g. enable watchdog, enable motor .. etc). To be used
when requested by the engineering team
WARNING:
None
desc000190.txt
60000
0
0
Engineering
SnS
0
0
0
0
MHC trace buffer dumps (20/AUG/08)
regeng015
000191 regeng015
Jason Tandy
Engineering
Study 000191:
Acronym: regeng015
A study to request MHC trace buffers dumps (runs an ORL file). To be used when
a Mechanical move is NACKED or when requested by engineers.
WARNING:
None
desc000191.txt
180000
0
0
Engineering
SnS
0
0
0
0
Active region high cadence study 12"x200" with 2" slit
SK_AR2_12x200p
000192 SK_AR2_12x200p
Suguru Kamio
Science
28-Jul-2007
Study 000192:
ACRONYM: SK_AR2_12x200p
Target: AR
High cadence study for transient brightenings in active regions.
12"x200" with 2" slit
WARNING:
High data rate
Add 10% to the study run time
desc000192.txt
44751
1
0
Active Region
Scanning
1152000
0
2
2
176
1
12
Ellerman bombs study 16"x200" with 2" slit
SK_AR2_16x200p
000193 SK_AR2_16x200p
Suguru Kamio
Science
28-Jul-2007
Study 000193:
ACRONYM: SK_AR2_16x200p
Target: AR
Ellerman bombs study in active regions with 30 sec cadence
16"x200" with 2" slit
WARNING:
High data rate
Add 10% to the study run time
desc000193.txt
52168
1
0
Active Region
Scanning
1536000
0
2
2
177
1
16
HPW001_FULLCCD_RAST_128x456_90S_SLIT1_JPEG
HPW001_FULLCCD_v2
000194 HPW001_FULLCCD_v2
Harry Warren
Science
28-Jul-2007
Study 000194:
ACRONYM: HPW001_FULLCCD_v2
This is a small raster that takes the full CCD in
both channels. The objective of this raster is to obtain a full EIS
spectral atlas over a small region. This raster can be used on active
regions but the relatively long exposure times (90s) may lead to
saturation in the strongest lines.
TARGET : Quiet Sun or Active Region
EXPOSURE TIME : 90s
SLIT : 1"
FOV : 128"x456"
DATA RATE : 50 kBits/s
TOTAL TIME : 3h25m
Note: USES JPEG COMPRESSION.
WARNING:
None
desc000194.txt
12370013
1
0
Quiet Sun
Scanning
637534227
0
0
0
178
1
128
HPW008_FULLCCD_RAST_128x256_25s_SLIT1_JPEG
HPW008_FULLCCD_v2
000195 HPW008_FULLCCD_v2
Harry Warren
Science
28-Jul-2007
Study 000195:
ACRONYM: HPW008_FULLCCD_V2
This is a small raster that takes the full CCD in
both channels. The objective of this raster is to obtain a full EIS
spectral atlas over a small region. This raster uses 25s exposures and
consumes 100 kBits/s of telemetry. Thus this study needs to be run
during a rare high data rate period or during a time where there are
periods of no observations (such as eclipse). The 25s also make the
raster more suitable for active region observations.
TARGET : Active Region
EXPOSURE TIME : 25s
SLIT : 1"
FOV : 128"x256"
DATA RATE : 97 kBits/s
TOTAL TIME : 1h0m
Note: USES JPEG COMPRESSION.
WARNING:
None
desc000195.txt
3634013
1
0
Active Region
Scanning
357913952
0
0
0
179
1
128
Solar microflares and network dynamics - relevance for coronal heating_context
Microflr+network_1
000196 Microflr+network_1
Jan Rybak
Science
28-Jul-2007
Study 000196:
ACRONYM: microflr+network_1
This is a context raster that should be used with microflr+network_2
desc000196.txt
533563
1
0
Active Region
Scanning
24994475
0
2
2
180
1
82
Solar microflares and network dynamics - relevance for coronal heating_sns
Microflr+network_2
000197 Microflr+network_2
Jan Rybak
Science
28-Jul-2007
Study 000197:
ACRONYM: microflr+network_2
** Context raster microflr+network_1 should be run before and after this
study **
This proposal merges together attempts to observe two kinds of solar
structures - solar microflares and supergranular network - which are
planned to be investigated to address common open questions on their
relevance for the heating and dynamics of the solar corona.
Target: AR
Instruction to planners:
This study should run from 8 till 12 UT
1) Run context microflr+network_1 (~8 UT)
2) Run microflr+network_2 (SNS * N times)
3) Stop for ~15 minutes (~9:30 UT) for EIS tables upload. NOTIFY the authors:
Jan Rybak: choc@astro.sk
Peter Gomory: gomory@astro.sk
The day before, if possible so that the stop time is used for collecting auxiliary at DOT.
4) Run microflr+network_2 (SNS * M times)
5) run context microflr+network_1 just before 12 UT
6) Stop at ~12 UT
WARNING:
None
desc000197.txt
1705268
1
0
Active Region
Scanning
82298882
0
2
2
181
1
2
Detailed, large format active region map
AR_velocity_map_v2
000198 AR_velocity_map_v2
Peter Young
Science
28-Jul-2007
Study 000198:
ACRONYM: ar_velocity_map_v3
The aim is take a fairly deep exposure of an active region over a large
area (7.5 x 6.5 arcmin2) for the purposes of velocity measurements and
diagnostics. I've set the duration to be about 5hr 40min so it should
fit nicely between the XRT synoptics. This type of study was one of the
original ones developed by the EIS Science Working Group and was
implemented as COMSCI_AR3 for the 90 day plan.
Consists of two rasters:
(1) 560x512 arcsec2 raster with 40" slit; 10 s exposure time
(2) 460x384 arcsec2 raster with 1" slit; 40 s exposure time
Raster (1) gives context information in 15 wavelength windows.
Raster (2) has a very extensive line list that covers virtually all
major EIS lines.
USE: produces very detailed diagnostic information over a large
area. Should be run on medium-to-large active regions.
WARNING: raster (1) should only be repeated once.
WARNING: The study should be placed on the timeline such that the
change from raster (1) to raster (2) does not take place during an SAA
period. Raster (1) lasts for 3 minutes so this should be
straightforward to evaluate.
desc000198.txt
20434849
2
0
Active Region
Scanning
1086259231
1
3
0
153
1
600
182
1
460
Recursive engineering test
REC_TEST
000199 REC_TEST
Harry Warren
Science
31-Aug-2007
Study 000199:
ACRONYM: REC_TEST
*** Recursive study testing ***
WARNINGS:
1) Must be followed by time tagged study
2) Must *not* be the last study in a daily plan
desc000199.txt
3530610
1
1
Quiet Sun
Scanning
247726080
0
3
3
40
18
116
SLOT 266 Sit&Stare movie with 10 sec exp., 512 CCD height, Fe XII195, He II256, Fe XV284
HH_SLOT266_JPEG_Q75
000200 HH_SLOT266_JPEG_Q75
Hiro Hara
Science
4-Sep-2007
Study 000200:
ACRONYM: HH_SLOT266_JPEG_Q75
Description:
This study is to be used for imaging observations of dynamic feature
of active regions
TARGET : Active Region
RASTER TYPE : SNS
SLIT : 266"
No. OF EXPOSURES: 100
EXPOSURE TIME : 10s
EXPOSURE DELAY : 5s
TOTAL TIME : 29m54s
COMPRESSION : JPEG
WARNINGS:
None
desc000200.txt
1793994
1
0
Active Region
Scanning
27428029
0
1
1
183
1
266
1" slit, FOV: EWxNS=200"x256", 10" step, 20 raster pos., 6 sec exp. [1 ras], DPCM
HH_AR+FLR_RAS_H10
000201 HH_AR+FLR_RAS_H10
Hiro Hara
Science
13-Sep-2007
Study 000201:
ACRONYM: HH_AR+FLR_RAS_H10
Description:
TARGET: AR
DESCRIPTION: As in H02, but with a single raster. This is used for
observations of active regions. Hot lines for
flares are also contained. The window size for hot lines is wider
than that of the previous version, HH_AR+FLR_RAS_H01, to detect high speed
flows.
WARNING:
None
desc000201.txt
187799
1
0
Active Region
Scanning
13981013
0
0
0
157
1
191
HH_AR+FLR_RAS_H01 (EWxNS=240"x240", 5.0sec exp, different FMIR init. pos. for each raster)
HH_AR+FLR_RAS_H012
000202 HH_AR+FLR_RAS_H012
Hiro Hara
Science
13-Sep-2007
Study 000202:
*** DO NOT USE ***
Imported by a mistake.
desc000202.txt
1767590
10
0
Active Region
Scanning
339148800
0
0
0
33
1
231
184
1
231
185
1
231
186
1
231
187
1
231
188
1
231
189
1
231
190
1
231
191
1
231
192
1
231
1" slit, FOV: EWxNS=200"x256", 10" step, 20 raster pos., 6 sec exp. [2 ras], JPEG(Q=95)
HH_AR+FLR_RAS_H11
000203 HH_AR+FLR_RAS_H11
Hiro Hara
Science
13-Sep-2007
Study 000203:
ACRONYM: HH_AR+FLR_RAS_H11
*** RECURSIVE ***
Description:
As in HH_H02 but with two rasters only.
DESCRIPTION: This is used for observations of active regions. Hot lines for
flares are also contained. The window size for hot lines is wider
than that of the previous version, HH_AR+FLR_RAS_H01, to detect high speed
flows.
WARNING:
None
desc000203.txt
354598
2
1
Active Region
Scanning
13981012
0
0
0
193
1
191
194
1
191
1" slit, FOV: EWxNS=200"x256", 10" step, 20 raster pos., 6 sec exp. [5 ras]
HH_AR+FLR_RAS_H03
000204 HH_AR+FLR_RAS_H03
Hiro Hara
Science
13-Sep-2007
Study 000204:
ACRONYM: HH_AR+FLR_RAS_H03
*** RECURSIVE ***
Description:
As in HH_H02 but with five rasters only.
DESCRIPTION: This is used for observations of active regions. Hot lines for
flares are also contained. The window size for hot lines is wider
than that of the previous version, HH_AR+FLR_RAS_H01, to detect high speed
flows.
WARNING:
None
desc000204.txt
854995
5
1
Active Region
Scanning
41943037
0
0
0
157
1
191
195
1
191
196
1
191
197
1
191
198
1
191
Active Region On Limb Study
AR_LIMB_V1
000205 AR_LIMB_V1
Helen Mason
Science
19-Sep-2007
Study 000205:
ACRONYM: AR_LIMB_V1
The objective of this study is to determine the thermal structure
of an active region as a function of height above the AR. In addition,
the electron density distribution will be derived.
A new line list has been devised to cover coronal emission over an
extensive range of temperatures. The 2" slit is used with a 45sec
exposure, using the full FoV of EIS, full length of slit and 6' wide
raster. Total time is about 2.5 hours.
TARGET: AR
An AR just as it approaches the limb, with the FoV such that the
AR core (still just on the disk) is included, but most of the FoV
is above the limb. An AR close to the equator would be best.
Other Hinode Observations:
If possible, it would be good to co-ordinate with XRT
(Temp diagnostics from filter ratios).
Other Observations:
It would also be useful (but not essential) to have co-ordinated
observations with CDS and TRACE.
WARNING:
None
desc000205.txt
8881190
1
0
Active Region
Scanning
487587854
0
2
2
199
1
360
Scan 30x512 area in 5 steps. 2" slit.
IUU_SCAN_STEPS_001
000206 IUU_SCAN_STEPS_001
Ignacio Ugarte
Science
19-Sep-2007
Study 000206:
ACRONYM: iuu_scan_steps_001
Intended to take repeated rastered images of quiet Sun structures:
e.g. coronal bright points and jets. To cover a wider sampling area,
in the shortest time, we take five 30s exposures in 6" steps.
Cadence is expected to be under 3 minutes. 2" slit used to increase
count numbers. Spectral windows are selected for their broad temperature
coverage and diagnostic (density) capabilities.
TARGET : Quiet Sun
EXPOSURE TIME : 30s
SLIT : 2"
FOV : 30"x512"
SPECTRAL WIND.: 24
WARNING:
None
desc000206.txt
3369000
1
0
Quiet Sun
Scanning
157286400
0
2
2
200
20
26
Sit-And-Stare 15s cadence SLOT movie. JPEG98.
IUU_SLOT_SNS_AR_001
000207 IUU_SLOT_SNS_AR_001
Ignacio Ugarte
Science
19-Sep-2007
Study 000207:
ACRONYM: IUU_SLOT_SNS_AR_001
Intended to take sit-and-stare observations of an active region
at a relatively short cadence (15s). Spectral windows are selected
for their spectral purity, diagnosed from previous 40" slit FULL CCD
observations. In order to be able to retrieve a sufficiently large
number of spectral lines with wide temperature coverage, JPEG98
compression is used. Spectral width is 48 pixels to account for the
wavelength orbital drift.
TARGET : Active Region
EXPOSURE TIME : 15s
SLIT : 40"
FOV : 40"x512"
SPECTRAL WIND.: 12
Note: USES JPEG COMPRESSION.
WARNING:
High data rate resulting from reducing the JPEG compression factor
desc000207.txt
3565489
1
0
Active Region
Scanning
157286404
0
3
3
201
1
40
Sit-And-Stare 30s cadence SLOT movie. JPEG98. Extended linelist.
IUU_SLOT_SNS_AR_02
000208 IUU_SLOT_SNS_AR_02
Ignacio Ugarte
Science
19-Sep-2007
Study 000208:
ACRONYM: iuu_slot_sns_ar_02
Intended to take sit-and-stare observations of an active region
or quiet Sun for a large sample (20) of clean spectral windows.
Spectral windows are selected for their spectral purity, diagnosed
from previous 40" slit FULL CCD observations. In order to be able to
retrieve a sufficiently large number of spectral lines with wide
temperature coverage, JPEG98 compression is used. Spectral width is
48 pixels to account for the wavelength orbital drift.
TARGET : Quiet Sun or Active Region
EXPOSURE TIME : 30s
SLIT : 40"
FOV : 40"x512"
SPECTRAL WIND.: 20
Note: USES JPEG COMPRESSION.
WARNING:
High data rate resulting from reducing the JPEG compression factor
desc000208.txt
3368994
1
0
Active Region
Scanning
131072003
0
3
3
202
1
40
EUNIS_EIS_Cross_Calibration
EUNIS_EIS_CrossCal
000209 EUNIS_EIS_CrossCal
Jeff Brosius
Science
1-Oct-2007
Study 000209:
ACRONYM: EUNIS_EIS_CrossCal
EUNIS sounding rocket / EIS calibration study
TARGET : Quiet Sun with a piece of AR (Sun cooperating), otherwise
Quiet Sun only
EXPOSURE TIME : 50 S
SLIT : 2"
FOV : 122"x512"
WINDOWS : 22
COMP : DPCM
Run time: ~56 Minutes per raster
REQUIRED RASTER REPEAT: 3 (~3H run time is required)
POINTING:
Sun center. QS with a piece of AR (small portion), otherwise QS
WARNING:
109 KBS Data Rate
desc000209.txt
3344862
1
0
Quiet Sun
Scanning
169902085
0
2
2
203
1
122
quiet sun study
quiet_sun_slot
000210 quiet_sun_slot
David Williams
Science
8-Oct-2007
Study 000210:
ACRONYM: quiet_sun_studies_slot
Context raster to be used with quiet_sun_studies (#211) and
quiet_sun_studies_1 (#212)
SLOT: 40"
TYPE: SNS
No. of Exposures: 1
FOV: 40"X512"
EXPOS. TIME: 60s
WARNING:
None
desc000210.txt
87465
1
0
Quiet Sun
Scanning
1070421
0
3
3
204
1
40
quiet_sun_study_v2
quiet_sun_studies
000211 quiet_sun_studies
G. Tsiropula
Science
8-Oct-2007
Study 000211:
ACRONYM: quiet_sun_studies (HOP0028)
Intended to take N repeated raster scans of a quiet region at the Sun's disk
center and at the limb. 10 spectral windows (including the core lines) have
been selected. ''Cold'' lines have been selected with windows widths of
32 pixels.
Slot images (context rasters), helpful for locating features, should be
taken at the beginning and at the end of the repeated rasters.
TARGET: Quiet sun --Sun center --limb (middle of the slit to be
positioned at the limb).
SLIT: 2"
EXPOS. TIME: 60s
FOV: 82" x 384"
SPECTRAL WIND: 96 pixels for OVI+FeVIII , 32 pixels for the other lines
LINES: OVI (184.12)+ Fe VIII (185.21), CaXVII (192.82), FeXII (195.12),
HeII (256.32), MgVI(269), MgVI (270.4), SiVII (275.35), MgV (276.57),
MgVII (278.39), MgVII (280.75)
INSTRUCTIONS TO PLANNES:
Run between 8UT - 11UT
Run context raster study (ACRONYM: quiet_sun_studies_slot) (#210)
Run quiet_sun_studies. Adjust the run time for the available time slot
Run context raster study (ACRONYM: quiet_sun_studies_slot) (#210)
WARNING:
None
desc000211.txt
2686063
1
0
Quiet Sun
Scanning
32243712
0
2
2
205
1
82
quiet_sun_study_v2
quiet_sun_studies_1
000212 quiet_sun_studies_1
G. Tsiropula
Science
8-Oct-2007
Study 000212:
ACRONYM: quiet_sun_studies_1 (HOP0028)
Intended to take N repeated raster scans of a quiet region at the Sun's disk
center and at the limb. 10 spectral windows (including the core lines) have
been selected. ''Cold'' lines have been selected with windows widths of
32 pixels.
Slot images (context rasters), helpful for locating features, should be
taken at the beginning and at the end of the repeated rasters.
TARGET: Quiet sun --Sun center --limb (middle of the slit to be
positioned at the limb).
SLIT: 1"
EXPOS. TIME: 60s
FOV: 41" x 360"
SPECTRAL WIND: 96 pixels for OVI+FeVIII , 32 pixels for the other lines
LINES: OVI (184.12)+ Fe VIII (185.21), CaXVII (192.82), FeXII (195.12),
HeII (256.32), MgVI(269), MgVI (270.4), SiVII (275.35), MgV (276.57),
MgVII (278.39), MgVII (280.75)
INSTRUCTION TO PLANNERS:
Run between 15UT - 17UT
Run context raster study (ACRONYM: quiet_sun_studies_slot) (#210)
Run quiet_sun_studies_1. Adjust the run time for the available time slot
Run context raster study (ACRONYM: quiet_sun_studies_slot) (#210)
WARNING:
None
desc000212.txt
5269063
1
0
Quiet Sun
Scanning
30228480
0
0
0
206
1
41
PZT forward stepping part 1
regeng021
000213 regeng021
Khalid al Janabi
Engineering
Study 000213:
ACRONYM: regeng021
Step the PZT in the forward direction, part 1
USAGE:
1) regeng021, regeng022, regeng023 and regeng024 should run consecutively,
hence should be chained together (append to highlighted entry)
2) The above chain **must** be followed by regeng015 (MHC trace dumps)
WARNING:
None
desc000213.txt
330000
0
0
Engineering
SnS
0
0
0
0
PZT forward stepping part 2
regeng022
000214 regeng022
Khalid al Janabi
Engineering
Study 000214:
ACRONYM: regeng022
Step the PZT in the forward direction, part 2
USAGE:
1) regeng021, regeng022, regeng023 and regeng024 should run consecutively,
hence should be chained together (append to highlighted entry)
2) The above chain **must** be followed by regeng015 (MHC trace dumps)
WARNING:
None
desc000214.txt
360000
0
0
Engineering
SnS
0
0
0
0
PZT backward stepping part 1
regeng023
000215 regeng023
Khalid al Janabi
Engineering
Study 000215:
ACRONYM: regeng023
Step the PZT in the backward direction, part 1
USAGE:
1) regeng021, regeng022, regeng023 and regeng024 should run consecutively,
hence should be chained together (append to highlighted entry)
2) The above chain **must** be followed by regeng015 (MHC trace dumps)
WARNING:
None
desc000215.txt
300000
0
0
Engineering
SnS
0
0
0
0
PZT backward stepping part 2
regeng024
000216 regeng024
Khalid al Janabi
Engineering
Study 000216:
ACRONYM: regeng024
Step the PZT in the backward direction, part 2
USAGE:
1) regeng021, regeng022, regeng023 and regeng024 should run consecutively,
hence should be chained together (append to highlighted entry)
2) The above chain **must** be followed by regeng015 (MHC trace dumps)
WARNING:
None
desc000216.txt
360000
0
0
Engineering
SnS
0
0
0
0
CHW_Context2_SI004
CHW_Context2_SI004
000217 CHW_Context2_SI004
Shin Imada
Science
15-Oct-2007
Study 000217:
ACRONYM: CHW_Context2_SI004
*Context* raster to be used with CHW_SNS2_SI003 (#218).
This study was designed to do alignment with other spacecrafts using
40 arcsec slots. In this study we choose the spectral windows to observe
cold emission lines (< 1MK).
TARGET : Polar Coronal Hole Region
EXPOSURE TIME : 45s
SLIT : 40"
FOV : 328"x512"
SPECTRAL WIND.: 15
Note: We recommend using with CHW_Context2_SI004
Example how to use: CHW_Context2_SI004
CHW_SNS2_SI003
CHW_Context2_SI004
POINTING: Polar coronal hole region.
WARNING: None
desc000217.txt
465435
1
0
Coronal Hole
Scanning
17694720
0
3
3
207
1
328
CHW_SNS2_SI003
CHW_SNS2_SI003
000218 CHW_SNS2_SI003
Shin Imada
Science
15-Oct-2007
Study 000218:
ACRONYM: CHW_SNS2_SI003
This study was designed to observe coronal hole waves with 40 arcsec slots
sit'n stare.
In this study we choose the spectral windows to observe cold emission
lines (< 1MK).
TARGET : Polar Coronal Hole Region
EXPOSURE TIME : 45s
SLIT : 40"
FOV : 40"x512"
SPECTRAL WIND.: 15
USAGE:
1) Run CHW_Context2_SI004
2) Run CHW_SNS2_SI003. Fill existing time slot
3) Run CHW_Context2_SI004
POINTING: Polar coronal hole region.
WARNING: None
desc000218.txt
6912592
1
0
Coronal Hole
Scanning
275251208
0
3
3
208
1
40
EL_SUMER_UVCS
EL_SUMER_UVCS
000219 EL_SUMER_UVCS
Enrico Landi
Science
17-Oct-2007
Study 000219:
ACRONYM: el_sumer_uvcs_1
Intended to take 50"-wide rasters of the boundary between coronal holes
and streamers outside the solar disk, using the full wavelength range
allowed by EIS and a 400"-long section of the EIS slit. The raster
is preferred over a sit'n'stare observation to ensure that the
field of view of the simultaneous SUMER observation is included in the
EIS field of view. Exposure time is chosen as a compromise
between high signal-to-noise observations and a compact study of the
same length as the SUMER study.
TARGET : Boundary between coronal holes and streamers
EXPOSURE TIME : 150s
SLIT : 2"
FOV : 50"x400"
SPECTRAL WIND.: 1024
DATA COMP. : JPEG
POINTING:
Target: Off-limb region at the solar polar holes. Slit to be positioned
at several heights whose coordinates will be chosen to follow the
boundary between coronal hole and streamer at many heights above the limb.
WARNING:
None
desc000219.txt
4009124
1
0
Coronal Hole
Scanning
218453339
0
2
2
209
1
2
SK_CH1 70x512 45sec in sync with SUMER
SK_CH1_70x512p
000220 SK_CH1_70x512p
Suguru Kamio
Science
17-Oct-2007
Study 000220:
ACRONYM: SK_CH1_70x512p
Intended to study the evolution of coronal bright points with
moderate cadence. It is designed to minimize observing time
difference of EIS and SUMER by repeating 1-hour narrow scans.
Line list consists of a wide range of iron lines (Fe VIII - Fe XV)
to cover lower corona and high temperature corona.
It also includes weak transition region lines to help
co-alignement with SUMER.
TARGET: Coronal Hole or Quiet Sun
EXPOSURE TIME: 45s
SLIT: 1"
FOV: 70"x512"
SPECTRAL WIND: 15
DATA COMP. : DPCM
POINTING:
POINTING:
Primary target is a bright point in polar coronal holes.
The 512" slit height allows to observe coronal hole boundary
and jets on the limb at the same time.
WARNING:
None
desc000220.txt
3467546
1
0
Coronal Hole
Scanning
97867096
0
0
0
210
1
70
AR dynamics with 2" slit
dei_arb_24_slit2
000221 dei_arb_24_slit2
Davina Innes
Science
23-Oct-2007
Study 000221:
ACRONYM: dei_arb_24_slit2
Small fast rasters across active region plage, to study microflare
footpoint dynamics. Wide temperature coverage and density diagnostics.
Long, for active region, exposure time to obtain a good signal on
transition region line OVI for comparision with SUMER OVI lines which
pump molecular hydrogen at microflare footpoints.
TARGET: Active region plage/sunspot
EXPOSURE TIME: 20 s
SLIT: 2"
FOV: 24"x224"
SPECTRAL WIND: 20
DATA COMP.: DCPM Lossless
Target: Fast small raster for AR dynamics. To be run with SUMER
WARNING:
None
desc000221.txt
298079
1
0
Active Region
Scanning
14336000
0
2
2
211
1
24
Small AR dynamics with slot
dei_arq_240_slot40
000222 dei_arq_240_slot40
Davina Innes
Science
23-Oct-2007
Study 000222:
ACRONYM: dei_arq_240_slot40
Six slot positions, separated by 40". A small sample of clean slot windows.
Windows are wide, not less than 56 pixels, except for CaXVII (set to 8).
TARGET: Active region
EXPOSURE TIME: 15 s
SLIT: 40"
FOV: 240"x272"
SPECTRAL WIND: 10
DATA COMP.: DCPM Lossless
Target: Active Region. To be run with SUMER
WARNING:
None
desc000222.txt
872820
1
0
Active Region
Scanning
43450368
0
3
3
212
8
240
Quiet Sun dynamics with slot
dei_qs_80_slot40
000223 dei_qs_80_slot40
Davina Innes
Science
23-Oct-2007
Study 000223
ACRONYM: dei_qs_80_slot40
Takes two neighbouring slot positions, separated by 40". The aim is to
put the left and right window edges repetitively at the same position on
the Sun, so that both wings of high Doppler shift events at the window edge
appear beyond the main line window. A small sample of clean slot windows
have been chosen. Windows are wide, not less than 56 pixels,
except for CaXVII (set to 8).
TARGET: Quiet Region of Sun
EXPOSURE TIME: 30 s
SLIT: 40"
FOV: 80"x512"
SPECTRAL WIND: 10
DATA COMP.: DCPM Lossless
POINTING: Filaments, Prominences, Quiet Sun. To be run with SUMER
WARNING:
None
desc000223.txt
892590
1
0
Quiet Sun
Scanning
44870306
0
3
3
213
13
80
GDZ_PLUME1
GDZ_PLUME1_2_300_50s
000224 GDZ_PLUME1_2_300_50s
Giulio del Zanna
Science
23-Oct-2007
Study 000224:
ACRONYM: GDZ_PLUME1_2_300_50s
Intended to sparse-raster a large area with the 2" slit and step size
4" (75 exposures), for a large sample (23) of spectral windows.
Spectral windows are selected to include mostly transition region lines,
however they include also Fe XIV, XV and XVI.
TARGET : Coronal Hole
EXPOSURE TIME : 50s
SLIT : 2"
FOV : 298"x512"
SPECTRAL WIND.: 23
DATA COMP. : DCPM
POINTING:
Off-limb region at the solar poles. The centre of the field of view
must be as close to the solar limb as possible, so at least 200" of
the slit are off-limb.
WARNING:
None
desc000224.txt
4107371
1
0
Coronal Hole
Scanning
199884805
0
2
2
214
1
298
ECH boundaries small raster
madj_ech_small
000225 madj_ech_small
Maria Madjarska
Science
23-Oct-2007
Study 000225:
ACRONYM: madj_ech_small
The study is designed to take a small (24"x512") raster observations with
2" x 512" slit of the quiet Sun, coronal hole boundaries both equatorial
and polar or an off-limb region above coronal holes. The new study is
covering a large number of spectral lines some covered with large spectral
windows. The selection is based on the results of already ongoing study.
TARGET : Quiet Sun, Coronal hole boundaries or off-limb region
EXPOSURE TIME : 60s
SLIT : 2"
FOV : 24"x512"
SPECTRAL WIND.: various size spectral windows
DATA COMP. : lossless
Repetition : to be repeated to fill 5 hours of observations.
POINTING:
Target: quiet Sun, coronal hole boundaries both polar and equatorial and
off-limb region of the Sun (west limb). If a target of opportunity is available
such as a filament or a prominence showing signs of forthcoming activation,
this study could be used. The study requires compensation for the
solar rotation i.e. we would like to follow one and the same region from the
Sun.
WARNING:
None
desc000225.txt
802079
1
0
Coronal Hole
Scanning
37486593
0
2
2
215
1
24
ECH boundaries
madj_ech
000226 madj_ech
Maria Madjarska
Science
23-Oct-2007
Study 000226:
ACRONYM: madj_ech
The study is designed to take a larger raster (120"x512")
observations with 2"x512" slit of the quiet Sun, coronal
hole boundaries, both equatorial and polar, or an off-limb
region above coronal holes. The new study is covering a large
number of spectral lines some covered with large spectral windows.
The selection is based on the results of already ongoing study.
TARGET : Quiet Sun, Coronal hole boundaries or off-limb region
EXPOSURE TIME : 60s
SLIT : 2"
FOV : 120"x512"
SPECTRAL WIND.: various size spectral windows
DATA COMP. : lossless
Repetitoin: : 1
POINTING:
quiet Sun, coronal hole boundaries both polar and equatorial and
off-limb region of the Sun (west limb). If a target of opportunity is
available such as a filament or a prominence showing signs of forthcoming
activation, this study could be used. The study requires compensation for
the solar rotation i.e. we would like to follow one and the same region
from the Sun.
WARNING:
None
desc000226.txt
3920397
1
0
Coronal Hole
Scanning
187432965
0
2
2
216
1
120
KM_FULLCCD_128x512_1slit_80sec
KM_FULLCCD_128x512
000227 KM_FULLCCD_128x512
Keiichi Matsuzaki
Science
6-Nov-2007
Study 000227:
ACRONYM: km_fullccd_128x512_1
Description:
Full CCD raster scan observation with exposure time of 80s prepared for
observation for HOP 51 [Multi temperature observation of the Quiet Sun
with EIS and SUMER].
Consists of one raster:
128x512 arcsec raster with 1" slit ; 80 s exposure time ; Full CCD ; DPCM
TOTAL TIME 182 min
WARNING:
* High datarate study (126 Kbit/second)
desc000227.txt
11026013
1
0
Quiet Sun
Scanning
1431655808
0
0
0
217
1
128
KM_FULLCCD_128x256_1slit_80sec
KM_FULLCCD_128x256
000228 KM_FULLCCD_128x256
Keiichi Matsuzaki
Science
6-Nov-2007
Study 000228:
ACRONYM: km_fullccd_128x256_1
Description:
Full CCD raster scan observation with exposure time of 80s prepared for
observation for HOP 51 [Multi temperature observation of the Quiet Sun
with EIS and SUMER].
Consists of one raster:
(1) 128x256 arcsec2 raster with 1" slit ; 80 s exposure time ; Full CCD ; DPCM
TOTAL TIME 182 min
WARNING:
* High data rate (63 Kbit/second)
desc000228.txt
11026013
1
0
Quiet Sun
Scanning
715827904
0
0
0
218
1
128
Slot imaging, 70s cadence, 148x400 FOV.
IUU_SLOT_148X400
000229 IUU_SLOT_148X400
Ignacio Ugarte
Science
14-Nov-2007
Study 000229:
ACRONYM: IUU_SLOT_148X400
Slot imaging. Four 15s exposures at adjacent pointing positions
sampling a 148"x400" FOV in around 70s. 17 repeats totaling around
20min. Spectral windows are selected for their spectral purity,
diagnosed from previous 40" slit FULL CCD observations.
TARGET : Active region (AR)
EXPOSURE TIME : 15s
SLIT : 40"
FOV : 148"x400"
SPECTRAL WIND.: 18
ESTIMATED CADENCE : ~70 s per full FOV.
ESTIMATED DURATION: ~20 m
NOTES:
To study AR loop dynamics, recommended to run for at least 2h.
WARNING:
- JPEG98 compression.
- High telemetry rate (83 kbs)
desc000229.txt
1227120
1
0
Active Region
Scanning
104448000
0
3
3
219
17
148
SYNOP004_400x400_30
SYNOP004_400x400_30
000230 SYNOP004_400x400_30
Harry Warren
Science
14-Nov-2007
Study 000230:
ACRONYM: SYNOP004_400x400_30
This raster is designed to be run routinely on
both quiet Sun and active region targets. The raster covers a
relatively large area (400"x400") and a significant fraction of the
CCD (180-205 and 248-285). To keep the duration reasonable the 2" slit
is used with 2" steps. The exposure time is 30s and there is a 30s
delay between exposures. Despite the delay the data rate is about 75
kbs.
TARGET : Quiet Sun or Active Region
EXPOSURE TIME : 30s, 30s delay
SLIT : 2"
FOV : 400"x400" (2" steps)
WINDOWS : 180-205, 248-285
TOTAL TIME : 3h36m
NOTE : USES JPEG 98 COMPRESSION.
WARNING:
High data rate (89 kbs)
desc000230.txt
13015489
1
0
Active Region
Scanning
1003865142
0
2
2
220
1
400
kpd01_qs_1slit_55stp_1ac_60s_v2
kpd01_qs_slit_60s_v2
000231 kpd01_qs_slit_60s_v2
Ken Dere
Science
14-Nov-2007
Study 000231:
ACRONYM: kpd01_qs_slit_60s_v2
This study is for viewing the quiet sun.
It consists of a single raster at 1 arc-sec steps with 60s exposure
times. The length of the sequence is limited so that it can be placed
between SAA crossings and no data is lost. With a series of
these studies, the evolution of the quiet sun can be
followed at all positions in the raster without interference from
the SAA. Data rate is low so 48 pixel windows, at the minimum,
are used. High temperature lines are included in case
something interesting happens.
In the end, the author would like a series of these studies run over
the course of 1 day for suitable pointings in the quiet sun. Each
study should be started after the end of an SAA or a sun-center repointing.
WARNING:
None
desc000231.txt
3660537
1
0
Quiet Sun
Scanning
157810692
0
0
0
221
1
56
Active Filaments
Romano
000232 Romano
Paolo Romano
Science
26-Nov-2007
Study 000232:
ACRONYM: Romano
******** OBSOLETE ******* (No DC which resulted in 112 kbs)
desc000232.txt
85282720
1
0
Eruptive Filament
Scanning
9861857280
0
0
0
222
19
360
Active filaments (DPCM) V2
Romano_v2
000233 Romano_v2
Paolo Romano
26-Nov-2007
Study 000233:
ACRONYM: Romano_v2
Note: Modified to use DPCM
This study is designed to observe wide regions of the solar disc waiting
for eruptions of active region filaments. Spectral windows are selected
to be able to retrieve a sufficient number of spectral lines with wide
temperature coverage. The exposure time is selected in order to obtain
useful data during the quiet and active phases of the filament life.
The goal of this observation is to study the mass motion
in the upper layers of the solar atmosphere, to do plasma diagnostics and
to obtain information about the emission variations related to the
activation processes.
SLIT : 1"
STEP SIZE : 1"
EXPOSURE TIME : 10s
FOV : 360"x512"
TIME REQUIRED : 1hr 14m 47s
REPEATS : 19 times
DATA RATE : 35 kbs
TARGET: Eruptive filaments
WARNING:
None
desc000233.txt
85282720
1
0
Eruptive Filament
Scanning
3287285855
0
0
0
223
19
360
Five-arcsecond rapid scan for TR and coronal brightenings (H. Isobe) (V2, 30s)
DRW001_HI_BRT_V2
000234 DRW001_HI_BRT_V2
David Williams
30-Nov-2007
Study 000234:
ACRONYM: DRW001_HI_BRT_V2
*************************
This study is a modified version of DRW001_HI_BRT_SCAN
Modifications: 30 second exposure time
1 Raster Repeat (instance)
Raster run time = 2m 47s
*************************
This study is intended to be run on patches of nominally unipolar quiet
Sun or plage, to search for jets and other features at cool temperatures
caused by the churning of the magnetic field.
The study consists of a single raster, with 5 contiguous positions
of EIS's narrow slit (1"), making a narrow but tall scan with *30 second*
exposures at each position. Each raster run time is ~ 2m 47s.
It should be run, where possible, in co-ordinated observations with SOT.
This study was originally requested by Hiroaki Isobe of the University
of Tokyo.
WARNING:
None
desc000234.txt
189825
1
0
Quiet Sun
Scanning
6707200
0
0
0
224
1
5
Large format, general purpose 40" slot raster
PRY_slot_context
000235 PRY_slot_context
Peter Young
Science
3-Jan-2008
Study 000235:
ACRONYM: PRY_slot_context
A slot context raster covering 600"x512". This is a general purpose
raster suitable for quiet Sun and active regions. The lines cover a
wide temperature range and include the Mg VI 269 and Si VII 275 lines
and the Fe XIII 203/202 and Si X 258/261 density diagnostics.
Duration: 3 minutes
TARGET: AR, QS
WARNING:
this study has a data rate of 163 kbps. Running it once is
not a problem as the duration is so short. Running it repeatedly will,
however, quickly fill the data recorder.
desc000235.txt
209474
1
0
Active Region
Scanning
34905043
0
3
3
153
1
600
High cadence study for loop footpoints
PRY_footpoints_HI
000236 PRY_footpoints_HI
Peter Young
Science
3-Jan-2008
Study 000236:
ACRONYM: PRY_footpoints_HI
This study is a further version of PRY_loop_footpoints and
PRY_footpoints_v2, but has a much enhanced data rate. It is intended
for a special campaign where EIS is given a greater share of the
Hinode data recorder.
To achieve the high data rate, the field-of-view in solar-Y has been
extended from 240 pixels to 512 pixels. The line list has been
slightly tweaked from PRY_footpoints_v2 to add in extra lines.
TARGET: AR
WARNING:
The data rate for this study is 121 kbps.
desc000236.txt
2561845
1
0
Active Region
Scanning
317757299
0
2
2
225
1
180
Quiet Sun, 50min cadence, detailed raster, *HI data rate*
QS_diagnostic_HI
000237 QS_diagnostic_HI
Peter Young
Science
15-Jan-2008
Study 000237:
ACRONYM: QS_diagnostic_HI
This study consists of 2 rasters:
(1) 2" raster covering 180"x360", large line list (50min; 133kbps)
(2) 2" raster covering 180"x360", reduced line list (50min; 74kbps)
This study is designed to obtain detailed diagnostics of a patch of
quiet Sun of size 180"x360" at a moderate cadence. It is for studying
the evolution of network structures and bright points over long
periods (preferably > 1 day).
It is recommended to run the study 'PRY_slot_context' once before this
study, and once after it in order to obtain large format context
images.
IMPORTANT: raster (1) has a higher data rate than raster (2). By
changing the relative number of raster repeats one can optimise the
EIS data recorder allocation. E.g., if the time slot allows 6
repeats, then one can set the repeats of raster (1) to 4 and the
repeats of raster (2) to 2. If the data recorder allocation is
exceeded by doing this, then the repeats can be set to 3 and 3, or 2
and 4.
WARNING: this study was designed assuming an EIS data recorder
allocation of 23% instead of the usual 15%.
desc000237.txt
6047690
2
0
Quiet Sun
Scanning
635222542
0
2
2
226
1
180
227
1
180
Chromospheric_Evaporation_During_Solar_Flares_-_V2
CHROMO_EVAP_RM_V2
000238 CHROMO_EVAP_RM_V2
Ryan Milligan
Science
15-Jan-2008
Study 000238:
ACRONYM: CHROMO_EVAP_RM_V2
This study is designed to detect Doppler shifts in several high temperature
emission lines as signatures of chromospheric evaporation. It also includes
a pair of density sensitive Fe XII lines for density diagnostics.
TARGET: Flare
EXPOSURE TIME: 1s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 152"x152"
RASTER DURATION: 4m 00s
Note: Uses JPEG95 compression.
Pointing:
Any flaring active region within approximately ±600" of disk center
for accurate line-of-sight velocity measurements.
Use/Instructions to planners:
The CHROMO_EVAP_RM_V2 study is one hour in duration (15 repeats of a 4 minute
raster). It should be run in large blocks of several hours
(e.g. 12 repeats for 12 hours) to increase the probability of jointly
observing a flare with RHESSI.
WARNING
None.
desc000238.txt
3623205
1
0
Flare
Scanning
184831995
0
2
2
228
15
152
Slot imaging, 70s cadence, 168x512 FOV. JPEG95.
IUU_SLOT_168X512
000239 IUU_SLOT_168X512
Ignacio Ugarte
Science
15-Jan-2008
Study 000239:
ACRONYM: IUU_SLOT_168X512
It's a modified version of study IUU_SLOT_148X400. It allows
more spatial overlap (8") between adjacents pointings.
Slot imaging. Five 12s exposures at adjacent pointing positions
sampling a 168"x512" FOV in around 70s. 17 repeats totaling around
20min. Spectral windows are selected for their spectral purity,
diagnosed from previous 40" slit FULL CCD observations.
TARGET : Active region (AR)
EXPOSURE TIME : 12s
SLOT : 40"
FOV : 168"x512"
SPECTRAL WIND.: 18
ESTIMATED CADENCE : ~70 s per full FOV.
Note : JPEG95 compression.
NOTES:
To study AR loop dynamics, recommended to run for at least 2h.
********* WARNING ********
Short raster duration (~1m).
*** Add 5 seconds per raster repeat to allow for rasters synchronization ***
For example: 10 raster repeats.
allow a 50 seconds GAP after 10 rasters repeat run (10*5) before
inserting a new study on the timeline
desc000239.txt
1260525
1
0
Active Region
Scanning
71315833
0
3
3
229
17
168
SYNOP004_400x400_v2
SYNOP004_400x400_v2
000240 SYNOP004_400x400_v2
Harry Warren
Science
15-Jan-2008
Study 000240:
ACRONYM: SYNOP004_400x400_v2
This raster is designed to be run routinely on both quiet Sun and
active region targets. The raster covers a relatively large area
(400"x400") and a significant fraction of the CCD (180-205 and
248-285). To keep the duration reasonable the 2" slit is used with 2"
steps. The exposure time is 30s and there is a 11s delay between
exposures. Relatively high compression is used and the data rate is
about 55 kbps.
TARGET : Quiet Sun or Active Region
EXPOSURE TIME : 30s, 11s delay
SLIT : 2"
FOV : 400"x400" (2" steps)
WINDOWS : 180-205, 248-285
TOTAL TIME : 2h30m25s
NOTE : USES JPEG 95 COMPRESSION.
WARNING:
None
desc000240.txt
9025489
1
0
Active Region
Scanning
508358471
0
2
2
230
1
400
Low data rate study for coronal loop footpoints
PRY_footpoints_lite
000241 PRY_footpoints_lite
Peter Young
Science
18-Jan-2008
Study 000241:
ACRONYM: PRY_footpoints_lite
This is a variation on the study PRY_footpoints_v2 designed for
periods when EIS has a *low data rate*. The study has a wide range of
lines and diagnostics and is suitable as a general purpose AR study.
TARGET: Active region
EXPOSURE TIME: 30s
SLOT: 2"
FOV: 100"x240"
ESTIMATED CADENCE: 28mins
DATE RATE: 27 kbps
USAGE:
If the contacts allow a period of high data rate, please supplement
this study with PRY_footpoints_v2.
As a context raster, please use PRY_slot_context (duration: 3min).
WARNING:
None
desc000241.txt
1695747
1
0
Active Region
Scanning
46512676
0
2
2
231
1
100
Narrow, high cadence study for microflares in active regions (low DR)
cam_artb_rhessi_lite
000242 cam_artb_rhessi_lite
Peter Young
Science
18-Jan-2008
Study 000242:
ACRONYM: cam_artb_rhessi_lite
This is a variation on the study CAM_ARTB_RHESSI_b_2 designed for
periods when EIS has a *low data rate*. The study has a wide range of
lines and diagnostics and is a general purpose study for AR dynamics.
TARGET: Active region
EXPOSURE TIME: 10s (3s delay)
SLOT: 2"
FOV: 40"x120"
ESTIMATED CADENCE: 5min 30s
DATE RATE: 25 kbps
USAGE:
If the contacts allow a period of high data rate, please supplement
this study with either CAM_ARTB_RHESSI_b_1 (40 kbps) or
CAM_ARTB_RHESSI_b_2 (50 kbps) to optimise the DR usage.
As a context raster, please use PRY_slot_context (duration: 3min).
WARNING:
None
desc000242.txt
334799
1
0
Active Region
Scanning
7896338
0
2
2
232
1
40
HPW015_DETAILED_MAP_1_45s_200x360
HPW015_DETAILED_MAP
000243 HPW015_DETAILED_MAP
Harry Warren
Science
4-Feb-2008
Study 000243:
ACRONYM: HPW015_DETAILED_MAP
This raster is designed as a large field of view context raster for an
active region. The line list includes both hot lines (Fe XVII, Fe
XXIII, Fe XXIV) and cool lines (Mg V, Mg VI, Mg VII). A number of
density diagnostics (e.g., Fe XII 187/195) are also included. If there
is sufficient telemetry the study AR_velocity_map_v2 should also be
considered as it has somewhat wider spectral windows but runs at about
55 kbs.
TARGET: Active Region
EXPOSURE TIME: 45s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 200"x360"
RASTER DURATION: 2h 44m
Note: data rate of 28 kbs
Pointing:
The raster width is set to be 200" to allow for some flexibility in
the planning. Ideally two rasters should be used to cover a greater
extent of the active region.
Use/Instructions to planners:
The exposures times are 45s, which should allow for this study to be
run in the quiet Sun.
Warning
None.
desc000243.txt
9865489
1
0
Active Region
Scanning
285566200
0
0
0
233
1
200
HPW016_DETAILED_SAS_1_45s_1x360
HPW016_DETAILED_SAS
000244 HPW016_DETAILED_SAS
Harry Warren
Science
4-Feb-2008
Study 000244:
ACRONYM: HPW016_DETAILED_SAS
This is a sit-and-stare version of HPW016_DETAILED_MAP. The line list
includes both hot lines (Fe XVII, Fe XXIII, Fe XXIV) and cool lines
(Mg V, Mg VI, Mg VII). A number of density diagnostics (e.g., Fe XII
187/195) are also included.
TARGET: Active Region
EXPOSURE TIME: 45s
RASTER: Sit-and-Stare
SLIT: 1"
FOV: 1"x360"
RASTER DURATION: ~10m
Note: data rate of 28 kbs
Pointing:
This is a sit-and-stare observation with the 1" slit. It is important
to be aware that there is an offset between the two detectors so that
the same plasma may not be imaged on both CCDs. A context raster
should be run in conjunction with this study. Note that
HPW013_AR_RAS_23m covers about 40" in 23m
Use/Instructions to planners:
The exposures times are 45s, which should allow for this study to be
run in the quiet Sun. Long, continuous runs of this study are
desirable as transient heating events can take a significant fraction
of an hour to evolve.
Warning
None.
desc000244.txt
3565974
1
0
Active Region
Scanning
102803832
0
0
0
234
6
1
qs-dynamics-small
qs-dynamics-small
000245 qs-dynamics-small
Karin Muglach
Science
12-Feb-2008
Study 000245:
ACRONYM: qs-dynamics-small
This study should be run in areas of quiet Sun, plage and
moderately active regions (e.g. a decaying AR).
Well developed ARs and coronal holes should be avoided.
We are looking for small-scale, short-term variation of
quiet sun structures primarily in the cooler EIS lines.
It should be run together with qs-dynamics-large_1.def
which procuces a larger context scan for the small
scan in the same spectral windows.
TARGET: Quiet Sun, plage, small AR
EXPOSURE TIME: 20s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 10"x464"
2) Pointing
anywhere on disk
3) Instructions to planners
- qs-dynamics-large
- qs-dynamics-small
- qs-dynamics-large
4) WARNING
None
desc000245.txt
137325
1
0
Quiet Sun
Scanning
5960112
0
2
2
235
1
10
QS-dynamics-large
QS-dynamics-large
000246 QS-dynamics-large
Karin Muglach
Science
12-Feb-2008
Study 000246:
ACRONYM: QS-dynamics-large
This study should be run in areas of quiet Sun, plage and
moderately active regions (e.g. a decaying AR).
Well developed ARs and coronal holes should be avoided.
It should be run together with qs-dynamics-small
and procuces a larger context scan for the small
scan in the same spectral windows.
TARGET: Quiet Sun, plage, small AR
EXPOSURE TIME: 40s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 90"x464"
2) Pointing
anywhere on disk
3) Use/Instructions to planners
- qs-dynamics-large
- qs-dynamics-small
- qs-dynamics-large
4) WARNING
None
desc000246.txt
2000923
1
0
Quiet Sun
Scanning
53641014
0
2
2
236
1
90
kpd01_qs_1slit_55stp_1ac_60s_v3
kpd01_qs_slit_60s_v3
000247 kpd01_qs_slit_60s_v3
Ken Dere
Science
12-Feb-2008
Study 000247:
ACRONYM: kpd01_qs_slit_60s_v3
*** V2 was missing a key line *** Addded in this version ***
This study is for viewing the quiet sun.
It consists of a single raster at 1 arc-sec steps with 60s exposure
times. The length of the sequence is limited so that it can be placed
between SAA crossings and no data is lost. With a series of
these studies, the evolution of the quiet sun can be
followed at all positions in the raster without interference from
the SAA. Data rate is low so 48 pixel windows, at the minimum,
are used. High temperature lines are included in case
something interesting happens.
In the end, the author would like a series of these studies run over
the course of 1 day for suitable pointings in the quiet sun. Each
study should be started after the end of an SAA or a sun-center repointing.
WARNING:
None
desc000247.txt
3660537
1
0
Quiet Sun
Scanning
166701433
0
0
0
237
1
56
QS slot image/movie. 104x512 FOV. JPEG85. Low data rate.
IUU_SLOT_104x512_Q85
000248 IUU_SLOT_104x512_Q85
Ignacio Ugarte
Science
23-Feb-2008
Study 000248:
ACRONYM: IUU_SLOT_104x512_Q85
Slot imaging. Low data rate. Three 28s exposures at adjacent pointing
positions sampling a 104"x512" FOV in around 90s. 8" spatial overlap. 13
repeats totaling around 20min. Spectral windows are selected for their
spectral purity,diagnosed from previous 40" observations.
TARGET : Quiet Sun (QS)
EXPOSURE TIME : 28s
SLIT : 40"
FOV : 104"x512"
SPECTRAL WIND.: 11
COMPRESSION: JPEG85
ESTIMATED CADENCE : ~90 s per full FOV.
ESTIMATED DURATION: ~20 m
WARNING:
Short raster duration (1.5m).
*** Add 5 seconds per raster repeat to allow for rasters synchronization ***
For example: 10 raster repeats.
allow a 50 seconds GAP after 10 rasters repeat run (10*5) before
inserting a new study on the timeline
desc000248.txt
1245735
1
0
Quiet Sun
Scanning
11842857
0
3
3
238
13
104
Heavily compressed (Q=50) slot context raster, 520"x512"
PRY_slot_context_v2
000249 PRY_slot_context_v2
Peter Young
Science
23-Feb-2008
Study 000249:
ACRONYM: PRY_slot_context_v2
A slot context raster covering 520"x512". This is a general purpose
raster suitable for quiet Sun and active regions. The lines cover a
wide temperature range and include the Mg VI 269 and Si VII 275. The
Fe XIII 203/202 density diagnostic is also included.
Compared to PRY_slot_context, this routine is heavily compressed
(JPEG50), contains less lines, and covers a smaller area. This reduces
the data rate down to about 12 kbits/s.
Duration: 3 minutes
TARGET: AR, QS
Note: Using JPEG50
WARNING:
None
desc000249.txt
184544
1
0
Active Region
Scanning
856536
0
3
3
239
1
520
St Andrews loop oscillations - slot sit 'n' stare - lo telemetry rate
sta_loop_slot_lo
000250 sta_loop_slot_lo
Danielle Bewsher
Science
23-Feb-2008
Study 000250:
ACRONYM: STA_loop_slot_v2
Objective:
----------
to investigate the morphology of coronal loops which support longitudinal
intensity perturbations, the nature of the (quasi-) periodic driver and
the evolution of the perturbation as they travel through the different
temperature regions of the solar atmosphere.
Conditions Necessary to Run & Pointing:
---------------------------------------
Occurrence of a relatively quiescent (non-flaring) coronal loop system
either on the disk or limb. Involvement of, at a minimum, Hinode/EIS,
SOHO/CDS and TRACE. Additional support from Hinode/XRT and Hinode/SOT/FPP
Study summary
-------------------
Slit/slot: 40" slot
No of pointing positions: 0
Total spatial width: 40"
Pixels in solar-y: 248
Exposure time: 20 seconds
No. of exposures: 100
Cadence: 38 minutes 39 seconds
Data rate: 3.9 kbits/s
Compression: JPG75
WARNING:
None
desc000250.txt
2318994
1
0
Active Region
Scanning
9237671
0
3
3
240
1
40
Transition Region Brightenings - lo telemetry rate
tr_bright_lo
000251 tr_bright_lo
Danielle Bewsher
Science
23-Feb-2008
Study 000251:
ACRONYM: tr_bright_lo
20"x144" raster using 2" slit
Objective:
----------
To observe small scale QS brightenings (blinkers, explosive events,
nanoflares, bright points etc.)
Conditions Necessary to Run & Pointing:
---------------------------------------
A patch of QS near to disk centre
Study summary
-------------------
Slit/slot: 2" slit
No of pointing positions: 9
Total spatial width: 20"
Pixels in solar-y: 144
Exposure time: 30 seconds
Cadence: 5 minutes 57 seconds
Data rate: 3.5 kbits/s
Compression: DPCM
WARNING:
None
desc000251.txt
357149
1
0
Quiet Sun
Scanning
1298028
0
2
2
241
1
20
Flatfield, 1 exposure, led 100ms, ccd left halves
regcal076
000252 regcal076
Louisa Bradley
Engineering
Study: 000252
Acronym: regcal076
Intensity variation measurements. Flat Fiels data used to determine changes
in intensity levels with time.
1) Repeats: 1
2) 1 flat field exposure (1 sec exp), left halves of both ccds
(LED on time: 100ms)
3) Time required: 30 seconds
4) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000252.txt
30000
0
0
Engineering
SnS
8388608
0
0
0
Flatfield, 2 exposures, led 80ms, full ccd
regcal077
000253 regcal077
Louisa Bradley
Engineering
Study: 000253
Acronym: regcal077
CCD "flatness" measurments. Data used to monitor PRNU (non-uniformity)
and PR defects
1) Repeats: 1
2) 2 flat field exposures (1 sec exps), full ccd
(LED on time: 80ms)
3) Time required: 90 seconds
4) Target: None (shutter closed)
WARNING:
DO NOT run within SAA
High DR
desc000253.txt
90000
0
0
Engineering
SnS
33554432
0
0
0
filament study: slot raster for context image
cme_slot_red_lkh
000254 cme_slot_red_lkh
Louise Harra
Science
29-Feb-2008
Study: 000254
ACRONYM: CME_slot_red_lkh
TARGET: Quiet Sun (or region close to Limb)
Study description:
Context raster for CME_slit_red_lkh.
This study can be run for quiet Sun filaments (or just for the quiet Sun).
It should be run it before and after the study CME_slit_red_lkh to provide
context image. It ideally should run for around 30 mins (if possible) to
get the temporal variations.
40"slot, 2 raster positions, 30sec exp.
A compression of JPEG Q=50 is used.
WARNING:
None
desc000254.txt
122895
1
0
Quiet Sun
Scanning
250372
0
3
3
242
1
120
filament study: slit raster
cme_slit_red_lkh
000255 cme_slit_red_lkh
Louise Harra
Science
29-Feb-2008
Study: 000255
Acronym: CME_slit_red_lkh
TARGET: Quiet Sun (or region close to Limb)
Study description:
This study can be run for quiet Sun filaments (or just for the quiet Sun).
It provides spectral information following the context study CME_slot_red_lkh.
Slot context/slit scan studies line lists are similar.
2"slit, 60 raster positions and with 4" steps in order to cover as
large a field of view as possible, 30sec exp.
A compression of JPEG Q=90 is used.
Instructions:
1) Run context raster study CME_slot_red_lkh, ideally for 30 minutes
(15 raster repeat)
2) Run CME_slit_red_lkh
3) Run context raster study CME_slot_red_lkh, ideally for 30 minutes
(15 raster repeat)
WARNING:
None
desc000255.txt
2063862
1
0
Quiet Sun
Scanning
27927451
0
2
2
243
1
242
SYNOP005
SYNOP005
000256 SYNOP005
John Mariska
Science
4-Mar-2008
Study: 000256
******* Replaced by SYNOP005_A ********
Acronym: SYNOP005 (SYNOP001 low data volume replacement)
Study Description:
Low data volume version of SYNOP001. Take one 90 s slot exposure
and one 90 s slit exposure while XRT is making its synoptic
exposures. Only the CCD windows that are analyzed for SYNOP001
and SYNOP002 are included. Slot/slit placement should be over
quiet Sun near Sun-center.
Duration: 3 min 37 s.
Target: Quiet Sun near Sun-center. Please do not use elsewhere.
Warning: none.
desc000256.txt
216930
2
0
Quiet Sun
Scanning
1603785
1
3
0
244
1
40
245
1
1
HPW004_Q95
HPW004_Q95
000257 HPW004_Q95
Harry Warren
Science
10-Mar-2008
Study: 000257
Acronym: HPW004_Q95
Study Description:
This is a "large" raster scan for JPEG95 detailed analysis
Warning: none.
desc000257.txt
8338013
1
0
Quiet Sun
Scanning
60856189
0
0
0
246
1
128
HPW004_Q90
HPW004_Q90
000258 HPW004_Q90
Harry Warren
10-Mar-2008
Study: 000258
Acronym: HPW004_Q95
Study Description:
This is a "large" raster scan for JPEG90 detailed analysis
Warning: none.
desc000258.txt
8338013
1
0
Quiet Sun
Scanning
92004082
0
0
0
247
1
128
HPW004_Q92
HPW004_Q92
000259 HPW004_Q92
Harry Warren
Science
10-Mar-2008
Study: 000259
Acronym: HPW004_Q92
Study Description:
This is a "large" raster scan for JPEG92 detailed analysis
Warning: none.
desc000259.txt
8338013
1
0
Quiet Sun
Scanning
55778228
0
0
0
248
1
128
HPW004_Q85
HPW004_Q85
000260 HPW004_Q85
Harry Warren
Science
10-Mar-2008
Study: 000260
Acronym: HPW004_Q85
Study Description:
This is a "large" raster scan for JPEG85 detailed analysis
Warning: none.
desc000260.txt
8338013
1
0
Quiet Sun
Scanning
36042041
0
0
0
249
1
128
Modified CAM_AR_LIMB_V1 for polar region scan (70 s Exposure time)
dhb_polar_scan
000261 dhb_polar_scan
David Brooks
Science
13-Mar-2008
Study 000261:
ACRONYM: dhb_polar_scan
***************************************************************
Modified AR_LIMB_V1 (45 s exposure time) to 70 s expsoure time,
as requested by David Brooks
***************************************************************
The objective of this study is to determine the thermal structure
of an active region as a function of height above the AR. In addition,
the electron density distribution will be derived.
A new line list has been devised to cover coronal emission over an
extensive range of temperatures. The 2" slit is used with a 45sec
exposure, using the full FoV of EIS, full length of slit and 6' wide
raster. Total time is about 2.5 hours.
TARGET: AR
An AR just as it approaches the limb, with the FoV such that the
AR core (still just on the disk) is included, but most of the FoV
is above the limb. An AR close to the equator would be best.
Other Hinode Observations:
If possible, it would be good to co-ordinate with XRT
(Temp diagnostics from filter ratios).
Other Observations:
It would also be useful (but not essential) to have co-ordinated
observations with CDS and TRACE.
WARNING:
None
desc000261.txt
13606190
1
0
Quiet Sun
Scanning
515057584
0
2
2
250
1
360
Modified qs-dynamics-small for Polar CH (60s Exposure time)
pch_plume_dynamics
000262 pch_plume_dynamics
David Williams
Science
17-Mar-2008
Study 000262:
ACRONYM: pch_plume_dynamics
*************************************************
Modified QS-dynamics_small for Polar CH (60 seconds exposure time),
as requested by David Williams
************************************************
This study should be run in areas of quiet Sun, plage and
moderately active regions (e.g. a decaying AR).
Well developed ARs and coronal holes should be avoided.
We are looking for small-scale, short-term variation of
quiet sun structures primarily in the cooler EIS lines.
TARGET: Quiet Sun, CH, plage, small AR
EXPOSURE TIME: 60s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 10"x464"
2) Pointing
QS, PCH
3) WARNING
None
desc000262.txt
347325
1
0
Coronal Hole
Scanning
5960112
0
2
2
251
1
10
Small CH raster for diagnostics, 60"x120",slit 2,exp.t 100s
EL_WHI_CH_small
000263 EL_WHI_CH_small
Enrico Landi
Science
26-Mar-2008
Study 000263:
ACRONYM: EL_WHI_CH_SMALL
This study is aimed at investigating the density, temperature and
abundance composition of equatorial coronal holes on the disk
by capitalizing on the number of ions included in the full EIS
range. This study is developed in response to the Whole Heliospheric
Interval campaign. The availability of many lines for accurate plasma
diagnostics is privileged at the expense of a wide field of view.
Target: equatorial coronal hole
Exposure time: 100s
Raster: scanning
Slit: 2"
Step size: 30
FOV: 60"x120"
Duration: 55 min.
POINTING:
equatorial coronal hole, with slit center more or less at the center of
the coronal hole. If coronal hole is small, it is OK to include surrounding
quiet Sun areas in the slit.
INSTRUCTIONS TO PLANNERS:
Run this study once a day as long as the equatorial hole is on the disk.
If possible, observe the same area in the hole each time.
WARNINGS
Avoid SAA.
desc000263.txt
3338413
1
0
Coronal Hole
Scanning
11112469
0
2
2
252
1
62
Sit'n'stare at limb,2"x512",3 reps at 600s exp.t each
EL_WHI_CH_limb
000264 EL_WHI_CH_limb
Enrico Landi
Science
26-Mar-2008
Study 000264:
ACRONYM: EL_WHI_CH_LIMB
This study is aimed at investigating the density, temperature and
abundance composition of equatorial coronal holes at the solar limb
as a function of latitude by capitalizing on the full length of the EIS
slit (512") and of the number of ions included inthe full EIS range.
Deep exposures are taken in order to 1) maximize the signal-to-noise
ratio and observe faint lines from a multitude of elements, and
2) reduce the data volume. This study is developed in response
to the Whole Heliospheric Interval and is meant to be run together
with a similar study for SOHO/UVCS.
Target: equatorial coronal hole
Exposure time: 600s
Raster: sit'n'stare
Slit: 2"
Step size: N/A
FOV: 2"x512"
Duration: 33 min.
POINTING:
equatorial coronal hole, with slit center more or less at
the equator, unless the coronal hole is located at v. high or v.low
latitudes, in which case the center of the slit should be more or
less at the latitude of the center of the coronal hole. Both west and east
limb are OK. the raster should be run close to the limb, say at around
1000" (20-40" above the limb).
INSTRUCTIONS TO PLANNERS:
Run this study once a day as long as the equatorial hole is at the limb.
WARNINGS
Avoid SAA.
desc000264.txt
2014769
1
0
Coronal Hole
Scanning
13124289
0
2
2
253
1
2
SYNOP005_A
SYNOP005_A
000265 SYNOP005_A
John Mariska
Science
27-Mar-2008
Study 000265:
ACRONYM: SYNOP005_A (SYNOP001/SYNOP005 low data volume replacement)
** DO NOT run more than once a day **
Study Description:
Low data volume version of SYNOP001. Take one 90 s slot exposure
and one 90 s slit exposure while XRT is making its synoptic
exposures. Only the CCD windows that are analyzed for SYNOP001
and SYNOP002 are included. Slot/slit placement should be over
quiet Sun near Sun-center.
Duration: 3 min 26 s.
Target: Quiet Sun near Sun-center. Please do not use elsewhere.
Instruction to planner:
1) Run if a second XRT available for a specific day
2) The FIRST SYNOP of the day is SYNOP001
Warning:
DO NOT run more than once a day
desc000265.txt
216930
2
0
Quiet Sun
Scanning
1749477
1
3
0
244
1
40
254
1
1
SYNOP006
SYNOP006
000266 SYNOP006
John Mariska
Science
27-Mar-2008
Study 000266:
ACRONYM: SYNOP006
*** This is a low data rate replacement for SYNOP002 ***
This is a 90 second exposure time, 128 exposures, 1" raster scan. Uses only
lines that analyzed for SYNOP002.
DURATION: 3h 26m 10s
TARGET: Sun center or near Sun center. Do not use anywhere else
WARNING:
None
desc000266.txt
12370013
1
0
Quiet Sun
Scanning
53650658
0
0
0
255
1
128
Coronal Hole study: JS_CH 140x256 45sec, adpoted from SK_CH1_70x512 (study 220)
JS_CH_140x256p
000267 JS_CH_140x256p
Louise Harra
Science
8-Apr-2008
Study 000267:
Acronym: JS_CH_140x256p
TARGET: Coronal Hole
Title: Coronal Hole study: JS_CH 140x256 45sec, adpoted from SK_CH1_70x512
Study description:
The target of this study is a polar coronal hole. EIS should be pointed to
include the boundary of the coronal hole and the limb. The purpose is to
obtain velocity maps of million degree plasma.
1"slit scan, FOV 140"x256", 45sec exp time. DCPM compression is used to
get good line profile.
Instructions to planners:
1. The regcal 071 & regcal 072 should be run before running this study.
2. Ideally this raster should run repeatedly (e.g. 2 or 3 times).
WARNING:
None
desc000267.txt
6912592
1
0
Coronal Hole
Scanning
79150874
0
0
0
256
1
140
Small raster for measuring density in coronal holes
PRY_CH_density
000268 PRY_CH_density
Peter Young
Science
8-Apr-2008
Study 000268:
ACRONYM: PRY_CH_density
A small raster covering 70"x200" intended for measuring densities in
coronal holes. It should be run in the darkest regions visible in EIT
171 or 195 images.
Since the raster field-of-view is small it is important to run a
context raster beforehand. PRY_slot_context_v2 is recommended.
PRY_CH_density should be repeated to fill the available time slot
Duration: 1hr 2min
Compression: DPCM
Data volume: 17 Mbits
Exposure time: 100s
Slit: 2"
WARNING:
None
desc000268.txt
3766273
1
0
Quiet Sun
Scanning
20122034
0
2
2
257
1
70
FOCUS_STUDY_COOL_LINES_FOR_MEASURING_CCD_OFFSET_AT_LIMB
FOCUS_STUDY
000269 FOCUS_STUDY
Harry Warren
Test
9-Apr-2008
Study 000269:
ACRONYM: FOCUS_STUDY
This study is used for EIS slit focus test
Duration: 1h 37m
Compression: DPCM
Data volume: 53 Mbits
Slit: 1"
Ratser scan: 60"
Step size: 1"
Exposure time: 90s
***************************************************************************
* This study is used in conjunctin with comcal077, comcal080 & comcal081 *
***************************************************************************
Pointing: Equatorial limb
******** should follow the pointing of the regcals******:
MIP = 1080
YIP = 256
Instructions to user:
1) Run FOCUS_STUDY (slit nominal position)
2) Run comcal077 (slit nominal position - 2 steps)
3) Run comcal080 (slit nominal position - 4 steps)
4) Run comcal081 (slit nominal position - 6 steps)
It would be (nice) to be able to run steps 1 to 4 twice, if possible.
WARNING:
None
desc000269.txt
5810397
1
0
Quiet Sun
Scanning
54983594
0
0
0
258
1
60
Focussing (nomianl slit position + 2)
comcal076
000270 comcal076
Khalid al Janabi
Engineering
Study 000270:
ACRONYM: comcal076
This study is used for EIS slit focus test
Duration: 1h 37s
Compression: DPCM
Data volume: 53 Mbits
Ratser scan: 60"
Exposure time: 90s
Slit: 1"
** This study is used with the FOCUS_STUDY **
Pointing:
MIP = 1080
YIP = 256
Instructions to user:
******** SEE study ID 269 ************
WARNING:
None
desc000270.txt
5820000
0
0
Engineering
SnS
54982656
0
0
0
Focussing (nomial slit position - 2)
comcal077
000271 comcal077
Matthew Whillock
Engineering
Study 000271:
ACRONYM: comcal077
This study is used for EIS slit focus test (nominal slit position -2 steps)
Duration: 1h 37s
Compression: DPCM
Data volume: 53 Mbits
Ratser scan: 60"
Exposure time: 90s
Slit: 1"
** This study is used with the FOCUS_STUDY **
Pointing:
MIP = 1080
YIP = 256
Instructions to user:
******** SEE study ID 269 ************
WARNING:
None
desc000271.txt
5820000
0
0
Engineering
SnS
54982656
0
0
0
FELDMAN_QSCH_ATLASv1
FELDMAN_QSCH_ATLASv1
000272 FELDMAN_QSCH_ATLASv1
Harry Warren
Science
22-Apr-2008
Study 000272:
ACRONYM: FELDMAN_QSCH_ATLASv1
This is a full CCD raster designed for lower data volumes. The 2" slit is
used to cut the number of exposures. Note that long exposures are used
(120s) so there may be some saturation of Fe XII 195. Also note that JPEG92
compression is used. An extended region along the slit is used so that the
raster may be positioned across a coronal/quiet Sun boundary.
TARGET: Quiet Sun/Coronal Hole
EXPOSURE TIME: 120s
FOV: 60"x304"
WINDOWS: FULL CCD
SLIT: 2"
COMPRESSION: JPEG92
DATA VOLUME: 140 Mbits
WARNING:
None
desc000272.txt
3861448
1
0
Quiet Sun
Scanning
141632308
0
2
2
259
1
60
HH_QS_EW_SCAN_01
HH_QS_EW_SCAN_01
000273 HH_QS_EW_SCAN_01
Hiro Hara
Science
22-Apr-2008
Study 000273:
Acronym: HH_QS_EW_SCAN_01
This study is intended to be run on the quiet sun in the equatorial region
for measurements of the average Doppler velocity relative to the limb.
Five spacecraft pointings are required to achieve the goal.
TARGET: Quiet Sun (equatorial)
EXPOSURE TIME: 120 sec
RASTER: Scanning
SLIT: 1"
STEP SIZE: 30"
FOV: EWxNS = 540" x 512"
RASTER DURATION: 40m54s
COMPRESSION: JPEG (Q=95)
2) ****** Five fixed pointings are required *******
No tracking of differential rotation by spacecraft.
(X,Y) = (800",0"), (400", 0"), (0",0"), (-400",0"), (-800",0")
Spacecraft pointing: west is first, east is last.
3) Use/Instruction to planners
Observation at one pointing in a single spacecraft orbit.
If possible, 2 raster scans at a single spacecraft pointing is
requested to see the details of orbital variation of the line
center positions. One raster is possible also for eclipse phase
(Apr 22 - Aug 21) because it takes 41 min for a single raster.
Observations of 2 rasters at a single spacecraft pointing are
requested for non-eclipse phase (82 min/2 rasters).
Coordination with other telescopes is not required.
4) WARNING
None
desc000273.txt
2453834
1
0
Quiet Sun
Scanning
9688751
0
0
0
260
1
541
HH_QS_EW_SCAN_02
HH_QS_EW_SCAN_02
000274 HH_QS_EW_SCAN_02
Hiro Hara
Science
22-Apr-2008
Study 000274:
Acronym: HH_QS_EW_SCAN_02
This study is intended to be run on the quiet sun in the equatorial region
for measurements of the average Doppler velocity relative to the limb.
Five spacecraft pointings are required to achieve the goal.
TARGET: Quiet Sun (equatorial)
EXPOSURE TIME: 120 sec
RASTER: Scanning
SLIT: 2"
STEP SIZE: 30"
FOV: EWxNS = 540" x 512"
RASTER DURATION: 40m54s
COMPRESSION: JPEG (Q=95)
2) ****** Five fixed pointings are required ******
No tracking of differential rotation by spacecraft.
(X,Y) = (800",0"), (400", 0"), (0",0"), (-400",0"), (-800",0")
Spacecraft pointing: west is first, east is last.
3) Use/Instruction to planners
Observation at one pointing in a single spacecraft orbit.
If possible, 2 raster scans at a single spacecraft pointing is
requested to see the details of orbital variation of the line
center positions. One raster is possible also for eclipse phase
(Apr 22 - Aug 21) because it takes 41 min for a single raster.
Observations of 2 rasters at a single spacecraft pointing are
requested for non-eclipse phase (82 min/2 rasters).
Coordination with other telescopes is not required.
4) WARNING
None
desc000274.txt
2453834
1
0
Quiet Sun
Scanning
9688751
0
2
2
261
1
542
kpd02_qs_rast_55
kpd02_qs
000275 kpd02_qs
Ken Dere
Science
22-Apr-2008
Study 000275:
Acronym: kpd02_qs
This study consists of a single raster that uses the 1" slit and
60s exposures times. The slit is rastered in 1 arc-sec increments over
an area of 55 arc-sec with the profiles read out over a length of 512
pixels. The study is intended primarily for the quiet Sun. It contains
a reduced but comprehensive set of spectral lines that should be
practical for operations during reduced telemetry but still provides a
large temperature coverage as well as density diagnostics. The width of
the raster is designed to fit between SAA traversals. Similar studies
have been run in the past so that the best use of this program would be
to implement an extended time sequence of rasters that are manually
placed between the SAAs.
TARGET: Anywhere on QS
WARNING:
None
desc000275.txt
3660537
1
0
Quiet Sun
Scanning
118186958
0
0
0
262
1
56
Focussing (nominal slit position -4 steps)
comcal080
000276 comcal080
Khalid al Janabi
Engineering
Study 000276:
ACRONYM: comcal080
This study is used for EIS slit focus test (nominal slit position -4 steps)
Duration: 1h 37s
Compression: DPCM
Data volume: 53 Mbits
Ratser scan: 60"
Exposure time: 90s
Slit: 1"
** This study is used with the FOCUS_STUDY **
Pointing:
MIP = 1080
YIP = 256
Instructions to user:
******** SEE study ID 269 ************
WARNING:
None
desc000276.txt
5820000
0
0
Engineering
SnS
54982656
0
0
0
Focussing (nominal slit position -6 steps)
comcal081
000277 comcal081
Matthew Whillock
Engineering
Study 000277:
ACRONYM: comcal081
This study is used for EIS slit focus test (nominal slit position -6 steps)
Duration: 1h 37s
Compression: DPCM
Data volume: 53 Mbits
Ratser scan: 60"
Exposure time: 90s
Slit: 1"
** This study is used with the FOCUS_STUDY **
Pointing:
MIP = 1080
YIP = 256
Instructions to user:
******** SEE study ID 269 ************
WARNING:
None
desc000277.txt
5820000
0
0
Engineering
SnS
54982656
0
0
0
St Andrews loop oscillations - context raster - lo telemetry rate
sta_loop_context_lo
000278 sta_loop_context_lo
Danielle Bewsher
Science
28-Apr-2008
Study 000278:
Acronym: sta_loop_context_lo
Context raster to be used in conjunction with sta_loop_slot_lo
Objective: to investigate the morphology of coronal loops which support
longitudinal intensity perturbations, the nature of the (quasi-) periodic
driver and the evolution of the perturbation as they travel through the
different temperature regions of the solar atmosphere.
Study summary:
Slit/slot: 2" slit
No of pointing positions: 59
Total spatial width: 120"
Pixels in solar-y: 248
Exposure time: 30 seconds
Cadence: 33 minutes 50 seconds
Compression: DPCM
Data rate: 11.7755 kbits/s
Data volume: 23644.07 kbits
Condition necessary to run and POINTING:
Occurence of a relatively quiescent
(non-flaring) coronal loop system either of the disk or limb. Involvement of,
at a minimum, Hindoe/EIS, SOHO/CDS and TRACE. Additional support from
Hinode/XRT and Hinode/SOT/FPP would be nice.
WARNING:
None
desc000278.txt
2030397
1
0
Active Region
Scanning
24211526
0
2
2
263
1
120
CME Onset - slit study - lo telemetry rate
cmeo_slit_lo
000279 cmeo_slit_lo
Danielle Bewsher
Science
28-Apr-2008
Study 000279:
Acronym: cmeo_slit_lo
Objective: To observe coronal dimming associated with the eruptions of CMEs
Study summary
Slit/slot: 2" slit
No of pointing positions: 89
Total spatial width: 180"
Pixels in solar-y: 320
Exposure time: 30 seconds
Cadence 50 minutes 12 seconds
Compression DPCM
Data rate: 9.1165 kbits/s
Data volume: 26771.19 kbits
POINTING:
The raster should be pointed to limb of Sun - above AR or
QS. Part of the raster should contain the limb.
WARNING:
None
desc000279.txt
3034345
1
0
Active Region
Scanning
28116610
0
2
2
264
1
180
CME Onset - slot study - lo telemetry rate
cmeo_slot_lo
000280 cmeo_slot_lo
Danielle Bewsher
Science
28-Apr-2008
Study 000280:
Acronym: cmeo_slot_lo
Objective: To observe coronal dimming associated with the eruptions of CMEs
Pointing:
The raster should be pointed to limb of Sun - above AR or
QS. Part of the raster should contain the limb.
Study summary
Slit/slot: 40" slot
No of pointing positions: 4
Total spatial width: 200"
Pixels in solar-y: 320
Exposure time: 30 seconds
Cadence 3 minutes 21 seconds
Compression JPEG (Q=85)
Data rate: 5.2059 kbits/s
Data volume: 1045.30 kbits
WARNING:
None
desc000280.txt
223290
1
0
Active Region
Scanning
1070383
0
3
3
265
1
240
Dark exposures, 0s, 2 exposures, bottom ccd half
regcal078
000281 regcal078
Louisa Bradley
Engineering
Study 000281:
Acronym: regcal078
2 dark exposures, 0 seconds, bottom half of ccd.
Data volume: 33 Mbit
WARNING:
Do not run in the SAA
desc000281.txt
120000
0
0
Engineering
SnS
33554432
0
0
0
Dark exposures, 0s, 2 exposures, top ccd half
regcal079
000282 regcal079
Louisa Bradley
Engineering
Study 000282:
Acronym: regcal079
2 dark exposures, 0 seconds, top half of ccd.
Data Volume: 33 Mbit
WARNING:
Do not run in the SAA
desc000282.txt
120000
0
0
Engineering
SnS
33554432
0
0
0
Alignment slot 266 short
Alignment_266_01
000283 Alignment_266_01
K. Watanabe
Science
16-May-2008
Study 000283:
ACRONYM: Alignment_266_01
This study is a light data volume replacement of Alignment_266.
1) Study outline
TARGET: Quiet Sun
EXPOSURE TIME: 20 sec
RASTER: Sit' n' stare
SLIT: 266"
FOV: EWxNS = 266" x 512"
STUDY DURATION: 45s
COMPRESSION: JPEG (Q=50)
DATA RATE: 43.4284 kBits/s
DATA VOLUME: 1 Mbits
2) Pointing
This Study should be pointed to limb of the Sun.
3) Use/Instruction to planners
None
4) WARNING
*** Short raster duration *** Add 5 seconds by putting the next study
5 seconds after this study end time on the timeline. Alternatively if used
with raster repeat, add 5 seconds per repeat.
desc000283.txt
45465
1
0
Quiet Sun
Scanning
1021269
0
1
1
266
1
266
Bright point slot raster
dob_bp_slot_raster
000284 dob_bp_slot_raster
Danielle Bewsher
Science
3-Jun-2008
Study 000284:
ACRONYM: dob_bp_slot_raster
Objective: To capture the dynamics and evolution of an x-ray bright point
Study summary:
Slit/slot: 40"
No of pointing positions: 3
Total spatial width: 160"
Pixels in solar-y: 160
Exposure time: 30 seconds
Cadence: 2m 13s
Compression: JPEG 92
Data rate: 3.6158 kbits/s
Data volume: 7830 kbits
Emission Lines: Fe XII (186.75), O V (192.90), Fe XII (195.12), He II
(256.32), Fe X (257.26), Si VII (275.35)
POINTING:
Point at region of QS - at location of a bright point if it can be predicted.
If not, point at QS and keep fingers crossed!
If possible, overlap with SOT field of view.
WARNING:
None
desc000284.txt
156360
1
0
Quiet Sun
Scanning
582369
0
3
3
267
1
160
Bright point slit raster
dob_bp_slit_raster
000285 dob_bp_slit_raster
Danielle Bewsher
Science
3-Jun-2008
Study 000285:
ACRONYM: dob_bp_slit_raster
Objective: To capture the dynamics and evolution of an x-ray bright point
Study summary:
Slit/slot: 2"
No of pointing positions: 59
Total spatial width: 120"
Pixels in solar-y: 160
Exposure time: 30 seconds
Cadence: 33m 50s
Compression: JPEG 95
Data rate: 3.5768 kbits/s
Data volume: 7262.25
Emission Lines: Fe XII (186.75), O V (192.90), Fe XII (195.12), He II
(256.32), Fe X (257.26), Si VII (275.35)
POINTING:
Point at region of QS - at location of a bright point if it can be predicted.
If not, point at QS and keep fingers crossed!
If possible, overlap with SOT field of view.
WARNING:
None
desc000285.txt
2030397
1
0
Quiet Sun
Scanning
7436541
0
2
2
268
1
120
Flare trigger AJW
FlareO_slit_AJW
000286 FlareO_slit_AJW
Alison Wallace
Science
9-Jun-2008
Study 000286:
ACRONYM: FlareO_slit_AJW
Objective: To capture activities in an active region leading to a flare.
Study summary:
Slit/slot: 2"
No of pointing positions: 89
Total spatial width: 180"
Pixels in solar-y: 320
Exposure time: 30 seconds
Cadence: 50m 34s
Compression: JPEG 95
Data rate: 9.5 kbits/s
Data volume: 29048 Kbits
POINTING:
Point at a flaring active region.
WARNING:
None
desc000286.txt
3034345
1
0
Active Region
Scanning
29746166
0
2
2
269
1
180
LT_CH_1_510x256
LT_CH_1_510x256
000287 LT_CH_1_510x256
Giulio del Zanna
Science
13-Jun-2008
Study 000287:
ACRONYM: LT_CH_1_510x256_1
Intended to study the morphology and flows in the boundary region between
coronal holes and quiet Sun.
The study is a sparse-raster of a large area with the 2" slit and step size
4" (128 pointing positions), for 6 spectral windows.
Spectral windows are selected to include
He II (blend) 256.2, O V 192.9, Fe VIII 186.6, Fe X 184.5, Fe XI (blend) 192.8,
Fe XII 186.8, 195.1, Fe XIV 264.7, i.e. with a good temperature coverage
for coronal holes/quiet Sun.
TARGET : Coronal Hole/Quiet Sun boundary
EXPOSURE TIME : 40s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 4"
FOV : 512"x256"
SPECTRAL WIND.: 6
DATA COMP. : DCPM
VOLUME : 32.5 Mbits
RASTER DURATON: 1h 34m
POINTING:
On-disc coronal hole boundary. If possible repeat with 2-3 different
pointings.
INSTRUCTION TO PLANNERS:
There should be ample coverage in each exposure of at least a
part of Quiet Sun. This is to ensure proper wavelength calibration
using the Quiet Sun as a reference.
WARNING:
This study is not suitable for active regions since some of the strong
lines might saturate.
desc000287.txt
5650013
1
0
Coronal Hole
Scanning
32491087
0
2
2
270
1
510
HPW_QS_MAP_v2_DPCM
HPW_QS_MAP_v2_DPCM
000288 HPW_QS_MAP_v2_DPCM
Harry Warren
Science
18-Jun-2008
Study 000288:
ACRONYM: HPW_QS_MAP_V2_DPCM
This raster is designed for observations of the quiet Sun at
relatively low data rates. Note that there are DPCM, JPEG 90, 85,
and 75 versions of this study.
The standard strong Fe lines are included. The only strong cool lines
are He II 256.32 and O VI 184.12. The following density sensitive line
pairs are included: Fe XII 186.880/195.119, Fe XIII 203.826/202.044,
and Fe XIV 264.787/274.230 (which is only sensitive above 10^9).
TARGET: Quiet Sun
EXPOSURE TIME: 60s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 30"x304"
RASTER DURATION: 32m29s
VOLUME: 21737 kbits
RATE: 11 kbits/s
Pointing:
---------
Anywhere on the quiet sun
Use/Instructions to planners:
-----------------------------
This is a narrow raster that can be expanded using ASRC.
If used with ASRC, use the following ASRC parameters:
* Set the raster repeat parameter and enable ASRC.
Direction: Leave in FORWARD position (ASRC specific)
SKIP: Don't change -> 1 (ASRC specific)
Compensation steps: Set to 120
Warning:
--------
None.
desc000288.txt
1971448
1
0
Quiet Sun
Scanning
22258983
0
0
0
271
1
30
HPW_QS_MAP_v2_Q90
HPW_QS_MAP_v2_Q90
000289 HPW_QS_MAP_v2_Q90
Harry Warren
Science
18-Jun-2008
Study 000289:
ACRONYM: HPW_QS_MAP_V2_Q90
This raster is designed for observations of the quiet Sun at
relatively low data rates. Note that there are DPCM, JPEG 90, 85,
and 75 versions of this study.
The standard strong Fe lines are included. The only strong cool lines
are He II 256.32 and O VI 184.12. The following density sensitive line
pairs are included: Fe XII 186.880/195.119, Fe XIII 203.826/202.044,
and Fe XIV 264.787/274.230 (which is only sensitive above 10^9).
TARGET: Quiet Sun
EXPOSURE TIME: 60s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 30"x304"
RASTER DURATION: 32m29s
VOLUME: 11079 kbits
RATE: 5.6 kbits/s
Pointing:
---------
Anywhere on the quiet sun
Use/Instructions to planners:
-----------------------------
This is a narrow raster that can be expanded using ASRC.
If used with ASRC, use the following ASRC parameters:
* Set the raster repeat parameter and enable ASRC.
Direction: Leave in FORWARD position (ASRC specific)
SKIP: Don't change -> 1 (ASRC specific)
Compensation steps: Set to 120
Warning:
--------
None.
desc000289.txt
1971448
1
0
Quiet Sun
Scanning
11345831
0
0
0
272
1
30
HPW_QS_MAP_v2_Q85
HPW_QS_MAP_v2_Q85
000290 HPW_QS_MAP_v2_Q85
Harry Warren
Science
18-Jun-2008
Study 000290:
ACRONYM: HPW_QS_MAP_V2_Q85
This raster is designed for observations of the quiet Sun at
relatively low data rates. Note that there are DPCM, JPEG 90, 85,
and 75 versions of this study.
The standard strong Fe lines are included. The only strong cool lines
are He II 256.32 and O VI 184.12. The following density sensitive line
pairs are included: Fe XII 186.880/195.119, Fe XIII 203.826/202.044,
and Fe XIV 264.787/274.230 (which is only sensitive above 10^9).
TARGET: Quiet Sun
EXPOSURE TIME: 60s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 30"x304"
RASTER DURATION: 32m29s
VOLUME: 8937 kbits
RATE: 4.5 kbits/s
Pointing:
---------
Anywhere on the quiet sun
Use/Instructions to planners:
-----------------------------
This is a narrow raster that can be expanded using ASRC.
If used with ASRC, use the following ASRC parameters:
* Set the raster repeat parameter and enable ASRC.
Direction: Leave in FORWARD position (ASRC specific)
SKIP: Don't change -> 1 (ASRC specific)
Compensation steps: Set to 120
Warning:
--------
None.
desc000290.txt
1971448
1
0
Quiet Sun
Scanning
9151777
0
0
0
273
1
30
HPW_QS_MAP_v2_Q75
HPW_QS_MAP_v2_Q75
000291 HPW_QS_MAP_v2_Q75
Harry Warren
Science
18-Jun-2008
Study 000291:
ACRONYM: HPW_QS_MAP_V2_Q75
This raster is designed for observations of the quiet Sun at
relatively low data rates. Note that there are DPCM, JPEG 90, 85,
and 75 versions of this study.
The standard strong Fe lines are included. The only strong cool lines
are He II 256.32 and O VI 184.12. The following density sensitive line
pairs are included: Fe XII 186.880/195.119, Fe XIII 203.826/202.044,
and Fe XIV 264.787/274.230 (which is only sensitive above 10^9).
TARGET: Quiet Sun
EXPOSURE TIME: 60s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 30"x304"
RASTER DURATION: 32m29s
VOLUME: 6723 kbits
RATE: 3.4 kbits/s
Pointing:
---------
Anywhere on the quiet sun
Use/Instructions to planners:
-----------------------------
This is a narrow raster that can be expanded using ASRC.
If used with ASRC, use the following ASRC parameters:
* Set the raster repeat parameter and enable ASRC.
Direction: Leave in FORWARD position (ASRC specific)
SKIP: Don't change -> 1 (ASRC specific)
Compensation steps: Set to 120
Warning:
--------
None.
desc000291.txt
1971448
1
0
Quiet Sun
Scanning
6884823
0
0
0
274
1
30
AR slot image/movie. 136x400 FOV. JPEG65. Low data rate.
IUU_SLOT_136x400_Q65
000292 IUU_SLOT_136x400_Q65
Ignacio Ugarte
Science
24-Jun-2008
Study 000292:
ACRONYM: IUU_SLOT_136x400_Q65
Slot imaging. Low data rate. Four 15s exposures at adjacent pointing
positions sampling a 136"x400" FOV in around 90s (there's a 5 second
delay after each exposure). 8" overlapping scan (40" Slot, 32" FMIR step size).
Spectral windows are selected for their spectral purity, diagnosed from
previous 40" observations. JPEG65 compression.
TARGET : Active Region (AR)
EXPOSURE TIME : 15s (+5s exposure delay)
SLIT : 40"
FOV : 136"x400"
SPECTRAL WIND. : 9
COMPRESSION : JPEG65
ESTIMATED CADENCE : ~90s
ESTIMATED DURATION : ~15m 41s (10 repeats)
Data rate : 10.39 kBits/s
Data Volume (per hour) : 37.4 MBits/h
WARNING:
None
desc000292.txt
941100
1
0
Active Region
Scanning
9773060
0
3
3
275
10
136
Chromospheric_Evaporation_During_Solar_Flares_V3
CHROMO_EVAP_RM_V3
000293 CHROMO_EVAP_RM_V3
Ryan Milligan
Science
24-Jun-2008
Study 000293:
ACRONYM: CHROMO_EVAP_RM_V3
This study is designed to detect Doppler shifts in several high temperature
emission lines as signatures of chromospheric evaporation.
TARGET: Flare
EXPOSURE TIME: 1s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 152"x152"
RASTER DURATION: 4m 00s
COMPRESSION: DPCM
DATA RATE: 50 kbits/s
DATA VOLUME/HOUR: 180 Mbits/h
Pointing:
Any flaring active region within approximately +/- 600" of disk center
for accurate line-of-sight velocity measurements.
Use/Instructions to planners:
The CHROMO_EVAP_RM_V3 study is one hour in duration (15 repeats of a 4 minute
raster). It should be run in large blocks of repeats to increase the
probability of jointly observing a flare with RHESSI.
WARNING:
High data volume
desc000293.txt
3623205
1
0
Flare
Scanning
187964745
0
2
2
276
15
152
Modified CAM_AR_LIMB_V1 for polar region scan (70 s Exposure time), remodified, 224H, JPEG90
dhb_polar_scan_Q90
000294 dhb_polar_scan_Q90
David Brooks
Science
3-Jul-2008
Study 000294:
ACRONYM: dhb_polar_scan_Q90
***************************************************************
Modified AR_LIMB_V1 (45 s exposure time) to 70 s expsoure time,
as requested by David Brooks
Remodified to reduce Y-height to 224" and increase
compression to JPEG90.
***************************************************************
The objective of this study is to measure line intensities to
allow derivation of the temperature and density structure of
the target. Since intensities are more important than velocities,
JPEG90 compression is used.
The line list covers coronal emission over an extensive range of
temperatures. The 2" slit is used with 70 sec exposures using
a FoV of 360x224 arcsecs. Total time is about 3 hours 50 mins.
TARGET: pretty much anything, except a very active region.
WARNING:
None
desc000294.txt
13606190
1
0
Quiet Sun
Scanning
156087574
0
2
2
277
1
360
SK_QS_34x168c_210sec
SK_QS_34x168c
000295 SK_QS_34x168c
Suguru Kamio
Science
10-Jul-2008
Study 000295:
ACRONYM: sk_qs_34x168c
This study is a rapid raster intended to capture temporal evolution
of X-ray bright point in a quiet region or microflare.
Spectral windows are selected to cover a wide rage of temperature.
T < 6.0 : He II 256.32, O V 192.90, Fe VIII 186.60
T = 6.2 : Fe XII 195.12/186.88, Fe XV 284.16
T > 6.4 : Ca XVII 192.82, Fe XXIII 263.76
TARGET: Quiet Sun
EXPOSURE TIME: 20s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 4"
FOV: 34"x168"
RASTER DURATION: 3m27s
Volume per raster: 2 Mbits
Volume/hour: 37 Mbits/h
2) POINTING
Enhanced magnetic field network or plage in a quiet region.
Align EIS FOV with SOT FOV (spacecraft center pointing).
3) INSTRUCTIONS TO PLANNERS
a) Run Study ID 292 IUU_SLOT_136x400_Q65 as a context raster
b) Run sk_qs_34x168c for 3 hours or longer (desired).
c) Run Study ID 292 IUU_SLOT_136x400_Q65 as a context raster
It is recommended to run this study in conjunction with
SOT magnetogram and Ca II H filtergram. The slit height is
selected to fit the height of SOT narrow-band filter and
spectropolarimeter.
4) WARNING
None
desc000295.txt
229185
1
0
Quiet Sun
Scanning
2105412
0
2
2
278
1
34
Range of Fe lines for density and temp. diagnostic of prom and prom. cavities
cavity_dem_1
000296 cavity_dem_1
Donald Schmit
Science
15-Jul-2008
Study 000296:
ACRONYM: cavity_dem
The study is designed to be used in examining
the density and temperature characteristics of prominence
and prominence cavities through the fitting of DEM curves
at every pixel in a set of spectroscopic images.
Previous observing runs have been done on cavities using
dhb_polar_scan, pry_ch_density, and gad_raster_2.
Analysis on these data sets have provided quality data for
preliminary analysis and have been helpful in realizing the
design of a cavity specific study. This study makes
use of 10 Fe lines (in 9 windows). By focusing solely on iron lines,
it is possible to neglect relative elemental abundance errors in the
DEM analysis. Two sets of density sensitive lines are chosen,
for Fe VIII and Fe XII, with complimentary ranges spanning densities
from 10^7-10^10 cm^-3. By using the 2” slit and long exposures,
a signal can be obtained well into the corona.
A wide FOV is necessary to capture the contrast between the cavity
and the surrounding coronal plasma. These features of the study
will allow us to better probe the temperature structure of
prominence cavities with regard to radial height and in relation to
the prominence.
TARGET: Prominence and surrounding corona (off limb)
EXPOSURE TIME: 100s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 302"x352"
RASTER DURATION: 4h30m
TOTAL VOLUME: 105 Mbits
WARNING:
None
desc000296.txt
16174207
1
0
Filament
Scanning
108172101
0
2
2
279
1
302
QS study designed to allow consecutive rasters over a full day
kpd02_QS_RAST_55
000297 kpd02_QS_RAST_55
Ken Dere
Science
23-Jul-2008
Study 000297:
Acronym: kpd02_qs_rast_55
This study consists of a single raster that uses the 1" slit and
60s exposures times. The slit is rastered in 1 arc-sec increments over
an area of 56 arc-sec with the profiles read out over a length of 256
pixels. The study is intended primarily for the quiet Sun. It contains
a reduced but comprehensive set of spectral lines that should be
practical for operations during reduced telemetry but still provides a
large temperature coverage as well as density diagnostics. The width of
the raster is designed to fit between SAA traversals. Similar studies
have been run in the past so that the best use of this program would be
to implement an extended time sequence of rasters that are manually
placed between the SAAs.
TARGET : Anywhere on QS
EXPOSURE TIME : 60s
RASTER : Scanning
SLIT : 1"
STEP_SIZE : 1"
FOV : 56"x256"
DATA COMP. : DPCM
RASTER DURATON: 1h 0s
DATA VOLUME/H : 31 Mbits/h
WARNING:
None
desc000297.txt
3660537
1
0
Quiet Sun
Scanning
32247001
0
0
0
280
1
56
GDZ_LT_FAST_340x300
GDZ_LT_FAST_340x300
000298 GDZ_LT_FAST_340x300
Giulio del Zanna
Science
23-Jul-2008
Study 000298:
ACRONYM: GDZ_LT_FAST_340x300
OBJECTIVE:
Monitor an active region evolution with a large field of view and
low-telemetry.
TARGET : Active region near disc centre
EXPOSURE TIME : 10s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 4"
FOV : 338"x304"
SPECTRAL WIND.: 5
DATA COMP. : JPEG90
RASTER DURATON: 18m
DATA VOLUME : 12.6 Mbits
DATA VOLUME/H : 44 Mbits/h
LINES : Si VII, Fe VII, Fe XII, Fe XIV, Fe XVI
POINTING: a reasonably small active region which would fit in the
340x300" field of view and is observed near meridian, say within
+/- 200".
INSTRUCTION TO PLANNERS:
Study must be repeated following the active region for at least 6 hours.
It is important to coordinate with TRACE planners so TRACE 171 band
is observed during the same period of observation.
WARNING:
none.
desc000298.txt
1082020
1
0
Active Region
Scanning
12907395
0
2
2
281
1
338
YK_AR_50x384
YK_AR_50x384
000299 YK_AR_50x384
Suguru Kamio
Science
12-Aug-2008
Study 000299:
ACRONYM: YK_AR_50x384
This active region study is intended to capture penumbral micro-jets
and their counterparts in the transition region and the corona.
Spectral windows cover cool lines as well as hot lines.
T < 6.0 : He II 256.32, O V 248.46, Mg VI 268.99, Fe VIII 186.60
T = 6.2 : Fe XII 195.12/186.88, Fe XV 284.16
T > 6.4 : Fe XVII 254.87, Fe XXIV 255.11
TARGET: Active region
EXPOSURE TIME: 20s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 51"x384"
RASTER DURATION: 19m31s
Compression: JPEG90
Volume per raster: 17 Mbits
Volume/hour: 52 Mbits/hour
2) POINTING
Penumbra of active region sunspots.
Align EIS FOV with SOT.
3) INSTRUCTIONS TO PLANNERS
Repeat this raster for two hours or more.
It is essential to get SOT Ca II H filtergram
to study penumbral micro-jets.
4) WARNING
None
desc000299.txt
1193712
1
0
Active Region
Scanning
17730685
0
0
0
282
1
51
GDZ_LT_XRBP_100x200
GDZ_LT_XRBP_100x200
000300 GDZ_LT_XRBP_100x200
Giulio del Zanna
Science
20-Aug-2008
Study 000300:
ACRONYM: GDZ_LT_XRBP_100x200
OBJECTIVE:
Monitor a quiet Sun X-ray bright point evolution with a
large selection of lines and low-telemetry.
TARGET : Quiet Sun region near disc centre
EXPOSURE TIME : 25s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 2"
FOV : 100"x200"
SPECTRAL WIND.: 15
DATA COMP. : JPEG90
RASTER DURATON: 24m
DATA volume : 16.16 Mbits
DATA VOLUME/H : 41.5 Mbits/h
LINES : He II, O V, Si VII, SiX, Ca XVII
Fe VIII X,XI,XII,XIII,XIV,XV,XVI,XVII, XXIII
POINTING: a quiet Sun region near disc centre
INSTRUCTION TO PLANNERS:
Ensure that the EIS FOV is aligned with SOT FOV
Study must be repeated following the region for at least 6 hours.
It is important to coordinate with TRACE planners so TRACE 171 band
is observed during the same period of observation.
WARNING:
The 25s exposure will produce low signal in most lines in the
quiet Sun, so this study is not well suited for quiet Sun studies.
desc000300.txt
1433247
1
0
Quiet Sun
Scanning
16546341
0
2
2
283
1
100
GDZ_LT_JET_SLOT1
GDZ_LT_JET_SLOT1
000301 GDZ_LT_JET_SLOT1
Giulio del Zanna
Science
20-Aug-2008
Study 000301:
ACRONYM: GDZ_LT_JET_SLOT1
OBJECTIVE:
Monitor with a 1.5m cadence an area of 110x200, to measure flows and
electron densities in X-ray jets located inside coronal holes.
TARGET : Coronal hole region
EXPOSURE TIME : 25s
RASTER : Scanning
SLIT : 40"
STEP_SIZE : 35"
FOV : 110"x240"
SPECTRAL WIND.: 10
DATA COMP. : JPEG75
RASTER DURATON: 1m 25s
DATA volume : 0.945 Mbits
Data Volume/H : 40 Mbits/h
LINES : He II, O V, Si VII, SiX
Fe XII,XIII, XV,XVI, XXIII
POINTING: a bright point inside a coronal hole region.
INSTRUCTION TO PLANNERS:
Ensure that the EIS FOV is aligned with SOT FOV
Study must be repeated following the region for at least 6 hours.
It is important to coordinate with TRACE planners so TRACE 195 A band
is observed during the same period of observation.
WARNING:
None
desc000301.txt
107145
1
0
Coronal Hole
Scanning
967680
0
3
3
284
1
110
GDZ_LT_JET_60x160
GDZ_LT_JET_60x160
000302 GDZ_LT_JET_60x160
Giulio del Zanna
Science
20-Aug-2008
Study 000302:
ACRONYM: GDZ_LT_JET_60x160
OBJECTIVE:
Monitor with a 12m cadence an area of 60x120, to measure flows and
electron densities in X-ray jets located inside coronal holes.
TARGET : Coronal hole region
EXPOSURE TIME : 20s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 2"
FOV : 60"x160"
SPECTRAL WIND.: 16
DATA COMP. : JPEG90
RASTER DURATON: 11m 30s
DATA volume : 9.66 Mbits
DATA volume/H : 48 Mbits/h
LINES : He II, O V, Si VII, SiX, Ca XVII
Fe VIII X,XI,XII,XIII,XIV,XV,XVI,XVII, XXIII
POINTING: a bright point inside a coronal hole region.
INSTRUCTION TO PLANNERS:
Ensure that the EIS FOV is aligned with SOT FOV
Study must be repeated following the region for at least 6 hours.
It is important to coordinate with TRACE planners so TRACE 195 A band
is observed during the same period of observation.
WARNING:
The 20s exposure will produce low signal in most lines in the
coronal hole, so this study is not well suited for coronal hole studies.
desc000302.txt
711448
1
0
Coronal Hole
Scanning
9890341
0
2
2
285
1
60
30s cadence slot raster movie with two positions
DHB_prom_slot_movie
000303 DHB_prom_slot_movie
David Brooks
Science
2-Sep-2008
Study 000303:
ACRONYM: DHB_prom_slot_movie
This study was designed to make a high cadence slot movie with a
FOV matched to SOT (typically smaller than EIS usually uses) and
a duration close to the maximum length of time SOT can run in "burst"
mode. It was originally intended for HOP73 (prominences/filaments)
but the exposure time is such that it would be suitable for a variety
of active targets.
The He II 256.32 line is the main target, but a series of coronal
lines from Fe XI - Fe XV are also included.
EXPOSURE TIME: 15s
RASTER: Scanning
SLIT: 40"
STEP SIZE: 36"
FOV: 76"x200"
STUDY DURATION: 6m17s
VOLUME: 3750 kbits
VOLUME/HOUR: 36 Mbits/h
RATE: 9.95 kbits/s
Use/Instructions to planners:
Align with SOT. Adjust repeats to fill the available time slot.
Warning:
None.
desc000303.txt
376800
1
0
Filament
Scanning
3840000
0
3
3
286
10
76
Coronal hole study for polar monitoring campaign
SK_CH_DIAG_320x384
000304 SK_CH_DIAG_320x384
Suguru Kamio
Science
2-Sep-2008
Study 000304:
ACRONYM: SK_CH_DIAG_320x384
This study performes a large scan for coronal holes
with low temperature lines (log T < 6.2).
It is designed for polar monitoring campaign with
SOT/SP measurement of magnetic fields.
TARGET : Coronal hole
EXPOSURE TIME : 50s
RASTER : Scanning
SLIT : 1"
STEP_SIZE : 1"
FOV : 320"x384"
SPECTRAL WIND.: 12
DATA COMP. : JPEG90
RASTER DURATON: 4h50m
DATA VOLUME : 150 Mbits
LINES : Fe VIII, Fe X, Fe XI, Fe XII, Fe XIII,
He II, O V, Mg VI, Mg VII, Si VII, Si X
POINTING:
Polar coronal hole with fixed pointing.
Make sure to cover SOT FOV and the solar limb.
INSTRUCTION TO PLANNERS:
Start this study at the beginning of SAA free period (roughly 10-15UT)
The later part may coincide with a short SAA.
WARNING:
Large data volume (150 Mbits), duration 4h 50m. Avoid SAAs as much
as possible (SAA degrade data compression factors and mutilate the data)
desc000304.txt
17451282
1
0
Coronal Hole
Scanning
153450150
0
0
0
287
1
320
SLOT imaging, large FOV. Quiet Sun.
IUU_SLOT_616X512_Q85
000305 IUU_SLOT_616X512_Q85
Ignacio Ugarte
Science
10-Sep-2008
Study 000305:
ACRONYM: IUU_SLOT_616x512_Q85
***************************************************
* OBSOLETE: Replaced by IUU_SLOT_488X512 (ID#378) *
***************************************************
Slot imaging, large FOV. Eighteen 28s exposures at adjacent pointing
positions sampling a 616"x512" area. 8" overlapping scan (40" Slot, 32"
FMIR step size). JPEG85 compression.
TARGET : Coronal hole / Quiet Sun
EXPOSURE TIME : 28s
SLIT : 40"
RASTER POINTINGS : 18
FOV : 616"x512"
SPECTRAL WIND. : 9
COMPRESSION : JPEG85
ESTIMATED DURATION : ~10m 18s
Data Volume : 11.4 MBits
Data Volume (per hour) : 66 MBits/h
WARNING:
None
desc000305.txt
618434
1
0
Quiet Sun
Scanning
11625161
0
3
3
288
1
616
NRL_QSCH_30x400_60s
NRL_QSCH_30x400_60s
000306 NRL_QSCH_30x400_60s
Harry Warren
Science
10-Sep-2008
Study 000306:
ACRONYM: NRL_QSCH_30x400_60s
This raster is designed for context observations of the quiet Sun and
coronal holes at relatively low data rate.
To conserve telemetry some standard strong lines, such as Fe XIII
202.04 and Fe XVI 262.98, have been omitted. S XIII 256.69, which is
in the He II 256.32 window, is included to cover any hot emission. The
Fe XII 186.880/195.119 density sensitive line pair is included.
The raster is sized so that ASRC can be used to make a larger raster.
TARGET: Quiet Sun/Coronal Hole
EXPOSURE TIME: 60s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 30"x400"
RASTER DURATION: 32m51s
VOLUME: 9.5 Mbits
VOLUME/HOUR: 17.4 Mbits/h
RATE: 4.8 kbits/s
COMPRESSION: JPEG90
Pointing:
---------
Anywhere in the quiet sun or a coronal hole
Use/Instructions to planners:
-----------------------------
This is a narrow raster that can be expanded using ASRC.
If used with ASRC, use the following ASRC parameters:
* Set the raster repeat parameter and enable ASRC.
Direction: Leave in FORWARD position (ASRC specific)
SKIP: Don't change -> 1 (ASRC specific)
Compensation steps: Set to 120
Warning:
--------
None.
desc000306.txt
1971448
1
0
Quiet Sun
Scanning
9740488
0
0
0
289
1
30
YKK_EqCH_01_50x400_300s_1arcsec
YKK_EqCH_01
000307 YKK_EqCH_01
Harry Warren
Science
10-Sep-2008
Study 000307:
***********************************************************
Do not use. YKK_EqCH_02W and YKK_EqCH_02N are preferred
IDs 329 and 330.
***********************************************************
ACRONYM: YKK_EqCH_01
This raster is designed for measuring temperatures, densities,
velocities, and abundances in coronal holes. To improve the signal in
weak lines, 2 long exposures are taken at each position in the raster.
TARGET: Coronal Hole
EXPOSURE TIME: 150s x 2 (2 exposures per raster position)
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 50"x400"
RASTER DURATION: 4h32m25s
COMPRESSION: DPCM
VOLUME: 115 Mbits
Pointing:
---------
Anywhere in the quiet sun or a coronal hole
Use/Instructions to planners:
-----------------------------
Chose the pointing so that part of raster lies in the quiet Sun. Since
this raster has a narrow width a context raster should be taken before
or after this is run.
Warning:
--------
None.
desc000307.txt
16367657
1
0
Coronal Hole
Scanning
119322036
0
0
0
290
1
50
GDZ_LT_PLUME_160x340
GDZ_LT_PLUME_160x340
000308 GDZ_LT_PLUME_160x340
Giulio del Zanna
Science
18-Sep-2008
Study 000308:
ACRONYM: GDZ_LT_PLUME_160x340
OBJECTIVE:
Measure Te, Ne on-disc and off-limb in a plume-interplume
area in a polar coronal hole. The EIS raster covers
160"x340" with low telemetry and is designed to have transition
region lines, with a few hotter ones aswell.
TARGET : Coronal hole region
EXPOSURE TIME : 40s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 2"
FOV : 160"x344"
SPECTRAL WIND.: 16
DATA COMP. : JPEG90
RASTER DURATON: 58m 37s
DATA volume : 51 Mbits
LINES : He II, O V, O VI, Si VII, S VIII, Si X, Ca XVII
Fe VIII X,XI,XII,XIV,XVI, XXIII
POINTING:
The pointing should be such as the base of a plume inside
a coronal hole region is observed, as well as its extension off-limb.
Make sure that the base of the plume is observed by SOT.
INSTRUCTION TO PLANNERS:
Shift the EIS CCD window (Y-direction) if needed to adjust the pointing.
It is important to coordinate with TRACE planners so TRACE 171 A band
is observed during the same period of observation.
WARNING:
None
desc000308.txt
3539696
1
0
Coronal Hole
Scanning
52408820
0
2
2
291
1
160
GDZ_LT_PLUME_10x180
GDZ_LT_PLUME_10x180
000309 GDZ_LT_PLUME_10x180
Giulio del Zanna
Science
18-Sep-2008
Study 000309:
ACRONYM: GDZ_LT_PLUME_10x180
Monitor with a 3m cadence and low telemetry an area of 10'x184", to measure
flows and electron densities in a plume located inside coronal holes.
TARGET : Coronal hole region
EXPOSURE TIME : 25s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 2"
FOV : 10"x184"
SPECTRAL WIND.: 15
DATA COMP. : JPEG90
RASTER DURATON: 2m 21s
DATA volume : 1.49 Mbits
LINES : He II, O V, Si VII, SiX, Ca XVII
Fe VIII X,XI,XII,XIV,XVI, XXIII
POINTING: the base of a plume inside a coronal hole region.
INSTRUCTION TO PLANNERS:
1 - Shift the EIS CCD window (Y-direction) if needed, so as to have
SOT and EIS to observe the same on-disc region.
2 - The study (duration 2m 44s) must be repeated 10 times
following the region (27m - 14.9 Mbits). Then the sequence should be repeated
5 times changing everytime the pointing by 10" (total of 2h 16m, 75 MBits)
in order to scan across the base of a plume.
It is essential to coordinate with TRACE planners so TRACE 171 A band
is observed during the same period of observation.
WARNING:
None
desc000309.txt
163575
1
0
Coronal Hole
Scanning
1522263
0
2
2
292
1
10
Prominence_raster_Slit1_x80y128_JPEG98_25Lines
prom_rast_v1
000310 prom_rast_v1
Nicolas Labrosse
Science
18-Sep-2008
Study 000310:
ACRONYM: prom_rast_v1
prom_rast_v1 consists in one raster taking spectra at 80 positions with 1"
steps, using the 1" slit, with 50s exposures at each position.
It runs in 1h14min, therefore it can be easily inserted in the EIS observing
plans. The window height in the Y direction is taken to be 128 pixels,
which is sufficient to cover the area occupied by our type of target.
JPEG98 compression is used to lower the telemetry requirements. The choice
of the 1" slit allows us to aim for maximal spatial and spectral resolution,
especially within the frame of HOP0082 where we will combine EIS and SUMER
observations (SUMER will use the 0.3"x120" or 1"x120" slit depending on line
and location).
We observe in 25 spectral windows to have a wide range of lines formed at
different temperatures, and allowing several density-sensitive line ratios
to be used for plasma diagnostics.
ACRONYM: prom_rast_v1
TARGET: active or quiescent filament / prominence
EXPOSURE TIME: 50 s
RASTER: scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 81"x128"
RASTER DURATION: 1h14m
2) Pointing
Any limb prominence or disk filament, with a preference for active / eruptive
structures
3) Running
Coordinated with SUMER
4) Warning
None
desc000310.txt
4434161
1
0
Eruptive Filament
Scanning
54432000
0
0
0
293
1
81
Prominence_small_rasters_slit2_x4y128_JPEG98_25Lines
prom_rast_small_v2
000311 prom_rast_small_v2
Nicolas Labrosse
Science
18-Sep-2008
Study 000311:
ACRONYM: prom_rast_small_v2
prom_rast_small_v2 consists in one small raster taking spectra at 2 positions
with 2" steps, using the 2" slit, with 25s exposures at each position. The
raster is repeated 30 times. The study runs in 28m35s, and is dedicated to
the study of prominence oscillations and their
variations with temperature. The window height in the Y direction is taken to
be 128 pixels, which is sufficient to cover the area occupied by our type of
target. The choice of the 2" slit allows us to cover more quickly a small
region with enough spatial and spectral resolution.
Ideally this would be a sit-n-stare study, but instead a narrow spatial scan
is made to co-align the two CCD images.
This study should be repeated as many times as possible over a continuous
period for increasing the range of oscillations periods to be detected.
We observe in 25 spectral windows to have a wide range of lines formed at
different temperatures, and allowing several density-sensitive line ratios
to be used for plasma diagnostics.
ACRONYM: prom_rast_small_v2
TARGET: filament / prominence
EXPOSURE TIME: 25 s
RASTER: scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 4"x128"
RASTER REPEATS: 30
RASTER DURATION: 28m35s
2) Pointing
Any limp prominence or disk filament
3) Running
Coordinated with SUMER if SUMER is observing.
The study should be run as many times as possible over a continuous period of
time to detect a range of oscillation periods.
4) Warning
None
desc000311.txt
1715400
1
0
Filament
Scanning
41856000
0
2
2
294
30
4
Solar microflares and network dynamic fibrils: context study
dot+eis:mic_fib_con
000312 dot+eis:mic_fib_con
Jan Rybak
Science
3-Oct-2008
Study 000312:
ACRONYM: dot+eis:mic_fib_con (HOP88)
Context raster for HOP88 (see study ID #313) for details
desc000312.txt
309194
1
0
Quiet Sun
Scanning
1723317
0
2
2
295
1
46
Solar microflares and network dynamic fibrils: sit-and-stare study
dot+eis:mic_fib_sit
000313 dot+eis:mic_fib_sit
Jan Rybak
Science
3-Oct-2008
Study 000313:
ACRONYM: dot+eis:mic_fib_sit (HOP 88)
Key Note:
---------
Because of a concern about a possible artifacts (possible introducing of noise)
associated with using JPEGs on low count rate data
(short exposures) (e.g. 10s), the following is recommended:
1) If more TM is available, try to switch the DC on the timeline to DPCM
(requires just over 200 Mbits)
2) else try JPEG95
3) Otherwise keep the default DC (JPEG90)
This applies to both context and SNS studies.
STUDY TITLE:
------------
Solar microflares and network dynamic fibrils - relevance for coronal
heating and mass supply
TARGET/POINTING:
----------------
QS at the disk center (or)
AR (or its remnants) near the disk center
Raster specific:
----------------
EXPOSURE TIME: 10s
SLIT: 2"
COMPRESSION: JPEG90 (default, see key note above)
USE/INSTRUCTIONS TO PLANNERS:
-----------------------------
The following sequence (1 to 3) should be repeated **TWICE**
1. Run dot+eis:mic_fib_con (context raster), number of raster repeats: 3
total time: 14m30s
2. Run dot+eis:mic_fib_sit (SNS), number of raster repeats: 11
total time: 1h50m
**** slit placed at the X-center of the context raster ****
3. Run dot+eis:mic_fib_con (context raster), number of raster repeats: 3
total time: 14m30s
**** raster positioned as in the previous context (step 1) ****
Steps 1 to 3 total time: 2h19m
*********** Total HOP time **********
2 x 2h19m (Data volume: 2 x 51.23 MBits - Using JPEG95)
There could be an interruption between the previous and following study
allowing any instrument specific upload of tables, etc. Adjust the number
of repeats so as to finish before the OBS table uplink. For example,
if it is only possible to do 3 of the 11 SNS, schedule the remaining 8
following the OBS table uplink.
SCHEDULING OF THE PROGRAM:
--------------------------
PREFERRED OBSERVING TIME SLOT (~DOT/LaPalma): ~09 - ~13 UT
Warning:
--------
As usual, avoid SAAs if possible (DC degradation)
desc000313.txt
620817
1
0
Quiet Sun
Scanning
3596487
0
2
2
296
1
2
HH_QS_EW_SCAN_01s (45arcsec step raster, 13 scanning positions, 30s exp. for velocity calibration)
HH_QS_EW_SCAN_01s
000314 HH_QS_EW_SCAN_01s
Hiro Hara
Calibration
13-Oct-2008
Study 000314:
Acronym: HH_QS_EW_SCAN_01s
This study is intended to be run on the quiet sun in the equatorial
region for measurements of the average Doppler velocity relative to
the limb. Five spacecraft pointings are required to achieve the goal.
TARGET: Quiet Sun (equatorial)
EXPOSURE TIME: 30 sec
RASTER: Scanning
SLIT: 1"
STEP SIZE: 45"
FOV: 540" x 512"
RASTER DURATION: 7m38s
COMPRESSION: JPEG (Q=90)
2) ****** Five fixed pointings are required *******
No tracking of differential rotation by spacecraft.
(X,Y) = (850",0"), (450", 0"), (0",0"), (-450",0"), (-850",0")
Spacecraft pointing: west is first, east is last.
3) Use/Instruction to planners
Run this study 10 times at a single spacecraft pointing.
The total raster duration covers about 75 min. Each scanning
point has 10 data points in the temporal direction and the
line centroid position changing with time due to orbital
variation is obtained at each scanning point.
Each coarse raster overlaps the neighbouring rasters in the
east-west direction, so that the line centroid position will
be calibrated to that measured at the limb.
4) WARNING
None
desc000314.txt
457544
1
0
Quiet Sun
Scanning
5520310
0
0
0
297
1
541
small quiet sun rasters
KM-qs-study-low
000315 KM-qs-study-low
Karin Muglach
Science
13-Oct-2008
Study 000315:
*** Replacement for qs-dynamics-small ***
ACRONYM: KM-qs-study-low
This study should be run in areas of quiet Sun, plage and
moderately active regions (e.g. a decaying AR).
Well developed ARs and coronal holes should be avoided.
We are looking for small-scale, short-term variation of
quiet sun structures primarily in the cooler EIS lines.
TARGET: Quiet Sun, plage, small AR
EXPOSURE TIME: 17s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 10"x256"
DURATION: 2m 2s
VOLUME: 2.27 Mbits
VOLUME/HOUR: 64 Mbits/h
COMP: DPCM
2) Pointing
anywhere on disk
3) Instruction to planners
* Run context raster study ID #210 "quiet_sun_raster" (3 times)
* Run KM-qs-study-low. Repeat raster to fill the available TM slot
* Run context raster study ID #210 "quiet_sun_raster" (3 times)
4) WARNING
None
desc000315.txt
121575
1
0
Quiet Sun
Scanning
2360406
0
2
2
298
1
10
Transient Horizontal Magnetic Field variability response in the TR and lower corona
DRW_QS_THMF
000316 DRW_QS_THMF
David Williams
Science
4-Nov-2008
Study 000316:
ACRONYM: DRW_QS_THMF
Description:
40” slot raster with two slightly overlapping positions, each position
having 30-second exposures giving ~1 minute net cadence.
The original target of this study, to investigate the coronal counterpart
to transient horizontal magnetic fields, is the quiet Sun at or near disc
centre. However, if we cannot obtain any chromospheric Stokes Q/U signals
corresponding to horizontal fields in the quiet Sun, we may go to the limb,
where Stokes V signal more sensitive to weaker line-of-sight magnetic field
gives us the information of horizontal fields.
4) WARNING
None
desc000316.txt
89430
1
0
Quiet Sun
Scanning
844800
0
3
3
299
1
76
Coronal Search for Alfven Waves
DRW_Alf_01
000317 DRW_Alf_01
David Williams
Science
4-Nov-2008
Study 000317:
ACRONYM: RW_Alf_01
Description:
Narrow continuous scan with six positions of the 2” slit (10 second
exposures), giving FOV of 12”x152”, at relatively high cadence
(60 seconds)
** N.B. For the original intended programme of THMFs with SOT,
align the centre of the EIS raster to the SOT pointing (beware the
offset between SOT centre and spacecraft centre, so please co-ordinate
with the SOT CO on this).
For all other uses of this study, use CO discretion as normal **
Original Programme: We prefer active regions to the quiet Sun for the
Alfven wave study. We would like to contain pore in target region,
because magnetic structure with life time longer than an hour is
preferable for the study. The target region should be far away from
THE disk center (We would like µ-angle about 60°), because we use the
Stokes V to detect transverse fluctuation of magnetic field and velocity.
4) WARNING
None
desc000317.txt
3762000
1
0
Active Region
Scanning
49226000
0
2
2
300
50
12
GRATING_RASTER_1_LARGE_WINDOWS_LARGE_FOV_FEW_LINES_v2
GRATING_RASTER_V2
000318 GRATING_RASTER_V2
Harry Warren
Science
11-Nov-2008
Study 000318:
ACRONYM: GRATING_RASTER_V2
This study was designed for studying the effects of moving the grating
position. The windows are large (48 pixels) to accomodate any shifts of
the lines on the detector as the grating is moved. The field of view is
also large (200x512). To conserve telemetry only a few lines are taken.
TARGET: Quiet Sun
EXPOSURE TIME: 50s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 200"x512"
RASTER DURATION: 3h1m32s
VOLUME: 193 Mbits
COMPRESSION: DPCM
Line List:
----------
184.20 48 # O VI 183.937, O VI 184.117, Fe X 184.536
186.60 48 # Fe VIII 186.601, Ca XIV 186.610, Fe XII 186.880
193.51 48 # Fe XII 193.509, Ca XIV 193.874
197.86 48 # Fe VIII 197.362, Fe XIII 197.434, Fe IX 197.862
256.32 48 # He II 256.317, Si X 256.366, S XIII 256.686
275.35 48 # Si VII 275.352, Fe XVII 275.54, Si VII 275.665
Pointing:
--------
Anywhere in the quiet sun.
Use/Instructions to planners:
-----------------------------
None.
desc000318.txt
10915489
1
0
Quiet Sun
Scanning
197430623
0
0
0
301
1
200
GDZ QUIET SUN 2" SLIT 60s 60X512 QS LINES ONLY
GDZ_QS1_60x512_60s
000319 GDZ_QS1_60x512_60s
Giulio del Zanna
Science
11-Nov-2008
Study 000319:
CRONYM: GDZ_QS1_60x512_60s
OBJECTIVE:
TARGET : Quiet Sun
EXPOSURE TIME : 60s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 2"
POINTING POS. : 30
FOV : 60"x512"
RASTER DURATON: 32m 29s
DATA volume : 69 Mbits
DATA COMP. : DPCM
SPECTRAL WIND.: 20
LINES : O IV,V,VI, Si VII, SiX, Ca XVII
Fe VIII X,XI,XII,XIII,XIV,XV,XVI
POINTING:
It is essential that Quiet Sun is observed, from the North
to the South limb, with some off-limb spectra.
1) Solar X=0", Solar Y=+500" top 512" of the slit
2) Solar X=0", Solar Y=+500" bottom 512" of the slit
3) Solar X=0", Solar Y=0" top 512" of the slit
4) Solar X=0", Solar Y=+0" bottom 512" of the slit
5) Solar X=0", Solar Y=-500" top 512" of the slit
6) Solar X=0", Solar Y=-500" bottom 512" of the slit
INSTRUCTION TO PLANNERS:
*** shift the EIS CCD extraction window *** (Top and Bottom of the CCDs)
WARNING:
Stronger lines would saturate if the study is run on an
active region.
desc000319.txt
1971448
1
0
Quiet Sun
Scanning
69100718
0
2
2
302
1
60
NRL_QSCH_30x400_60s2
NRL_QSCH_30x400_60s2
000320 NRL_QSCH_30x400_60s2
Harry Warren
Science
20-Nov-2008
Study 000320:
ACRONYM: NRL_QSCH_30x400_60s2
This is a revised version of NRL_QSCH_30x400_60s. A new window at
Fe IX 197.862 has been added.
This raster is designed for context observations of the quiet Sun and
coronal holes at relatively low data rate.
To conserve telemetry some standard strong lines, such as Fe XIII
202.04 and Fe XVI 262.98, have been omitted. S XIII 256.69, which is
in the He II 256.32 window, is included to cover any hot emission. The
Fe XII 186.880/195.119 density sensitive line pair is included.
The raster is sized so that ASRC can be used to make a larger raster.
TARGET: Quiet Sun/Coronal Hole
EXPOSURE TIME: 60s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 30"x400"
RASTER DURATION: 32m51s
VOLUME: 10.6 Mbits
VOLUME/HOUR: 19.4 Mbits/h
RATE: 5.4 kbits/s
COMPRESSION: JPEG90
Line List:
----------
256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
186.75 32 # Fe VIII 186.601, Ca XIV 186.610, Fe XII 186.880
275.40 24 # Si VII 275.352
197.86 24 # Fe IX 197.862
184.54 24 # Fe X 184.536
188.32 24 # Fe XI 188.216, Fe XI 188.299
195.12 24 # Fe XII 195.119
270.52 24 # Mg VI 270.394, Fe XIV 270.519
284.16 24 # Al IX 284.015, Fe XV 284.160
Pointing:
---------
Anywhere in the quiet sun or a coronal hole
Use/Instructions to planners:
-----------------------------
This is a narrow raster that can be expanded using ASRC.
If used with ASRC, use the following ASRC parameters:
* Set the raster repeat parameter and enable ASRC.
Direction: Leave in FORWARD position (ASRC specific)
SKIP: Don't change -> 1 (ASRC specific)
Compensation steps: Set to 120
Warning:
--------
None.
desc000320.txt
1971448
1
0
Quiet Sun
Scanning
10864390
0
0
0
303
1
30
NRL_QSCH_30x400_90s
NRL_QSCH_30x400_90s
000321 NRL_QSCH_30x400_90s
Harry Warren
Science
20-Nov-2008
Study 000321:
ACRONYM: NRL_QSCH_30x400_90s
****** Do not use -- OBSOLETE *****
Modified version imported by a mistake
desc000321.txt
2916448
1
0
Quiet Sun
Scanning
24421756
0
0
0
304
1
5
NRL_QSCH_30x400_90s_2
NRL_QSCH_30x400_90s2
000322 NRL_QSCH_30x400_90s2
Harry Warren
Science
20-Nov-2008
Study 000322:
ACRONYM: NRL_QSCH_30x400_90s
This raster is designed for more detailed observations of the quiet Sun
and coronal holes at relatively low data rate. This study is intendend to
complement nrl_qsch_30x400_60s2 by including more lines, deeper exposures,
and lower compression. The Fe XII 186.880/195.119 density sensitive line
pair is included. S X 264.233 is also included for abundance studies.
The raster is sized so that ASRC can be used to make a larger raster.
TARGET: Quiet Sun/Coronal Hole
EXPOSURE TIME: 90s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 30"x400"
RASTER DURATION: 48m36s
VOLUME: 23.8 Mbits
VOLUME/HOUR: 29.4 Mbits/h
RATE: 8.2 kbits/s
COMPRESSION: DPCM
Line List:
----------
256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
186.75 32 # Fe VIII 186.601, Ca XIV 186.610, Fe XII 186.880
275.40 24 # Si VII 275.352
197.86 24 # Fe IX 197.862
184.54 24 # Fe X 184.536
188.32 24 # Fe XI 188.216, Fe XI 188.299
193.60 24 # Fe XII 193.509
195.12 24 # Fe XII 195.119
264.23 24 # S X 264.233
202.04 24 # Fe XIII 202.044
270.52 24 # Mg VI 270.394, Fe XIV 270.519
284.16 24 # Al IX 284.015, Fe XV 284.160
262.98 24 # Fe XVI 262.984
Pointing:
---------
Anywhere in the quiet sun or a coronal hole
Use/Instructions to planners:
-----------------------------
This is a narrow raster that can be expanded using ASRC.
If used with ASRC, use the following ASRC parameters:
* Set the raster repeat parameter and enable ASRC.
Direction: Leave in FORWARD position (ASRC specific)
SKIP: Don't change -> 1 (ASRC specific)
Compensation steps: Set to 120
Warning:
--------
None.
desc000322.txt
2916448
1
0
Quiet Sun
Scanning
24421756
0
0
0
305
1
30
Study for measuring temperature with Fe IX in coronal holes
Fe9_offlimb
000323 Fe9_offlimb
Peter Young
Science
20-Nov-2008
Study 000323:
ACRONYM: Fe9_Offlimb
This is a long exposure, large raster intended for measuring the
temperature in coronal holes off-limb using the Fe IX 197.86/171.07
ratio. Other diagnostic lines are also obtained (Si VIII, Fe X).
TARGET: Off-limb coronal holes
EXPOSURE TIME: 100s
RASTER: scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 200"x400"
DURATION: 3 hours
VOLUME: 100 Mbits
Pointing:
---------
Large, polar coronal hole, off-limb, the slit should be placed from 30”
inside the limb to 370” outside the limb
Instruction to planners:
-----------------------
run following studies:
PRY_slot_context_v2 (3min, 4Mbit)
Fe9_Offlimb (3 hrs, 100Mbit)
PRY_slot_context_v2 (3min, 4Mbit)
* No specific support is requested for SOT
* XRT should run deep exposures in a wide range of filters to provide
temperature measurements.
Warning:
-------
None
desc000323.txt
10718994
1
0
Coronal Hole
Scanning
102828449
0
2
2
306
1
200
QS study
madj_qs
000324 madj_qs
Maria Madjarska
Science
20-Nov-2008
Study 000324:
ACRONYM: madj_qs
The study will run in the quiet Sun context raster. To be run with
madj_qs_small (Study ID: #325)
Target: quiet Sun
Expsore time: 50 sec
slit: 2"
Step size: 2"
FOV: 70"x248"
Duration: 32m 9s
Data Volume: 15.8 Mbits
S/C Solar rotational compensation i.e., tracking the same region on the Sun
enabled (default)
Warning:
Do not start the context raster within SAA
The study madj_qs_small should follow immediately after
desc000324.txt
1928773
1
0
Quiet Sun
Scanning
16259122
0
2
2
307
1
70
QS study with small rasters
madj_qs_small
000325 madj_qs_small
Maria Madjarska
Science
20-Nov-2008
Study 000325:
ACRONYM: madj_qs_small
The study will run in the quiet Sun.
Target: quiet Sun
Expsore time: 50 sec
slit: 2"
Step size: 2"
FOV: 24"x248"
Duration: 11m 16s
Data Volume: 5.5 Mbits
Data Volume/H: 30 Mbits/h
Pointing:
---------
Day 1: Y ~ 0" and X ~ -400"
Day 2: Y ~ 0" and X ~ 0"
Day 3: Y ~ 0" and X ~ 400"
Day 4: Y ~ 0" and X very close to the limb
S/C Solar rotational compensation i.e., tracking the same region on the Sun
should be enabled (default)
Instruction to planners:
------------------------
Run the following studies:
1) Run madj_qs (context raster)
To be followed by (preferably chained to)
2) Run madj_qs_small, 24 raster repeat, minimum.
Warning:
-------
Do not start within SAA
desc000325.txt
676079
1
0
Quiet Sun
Scanning
5574556
0
2
2
308
1
24
St Andrews Plume Context Study
sta_plume_context
000326 sta_plume_context
Danielle Bewsher
Science
12-Dec-2008
Study 000326:
ACRONYM: sta_plume_context
Context raster to be used in conjunction with sta_plume_slot
Objective: to observe fast magnetoacoustic waves and Alfven waves in plumes.
Condition necessary to run and pointing:
---------------------------------------
Occurrence of a plume on the limb. Slot should cover the plume footpoint
and as much of the plume length as possible.
Study summary:
Slit/slot: 2" slit
No of pointing positions: 59
Total spatial width: 120"
Pixels in solar-y: 512
Exposure time: 60 seconds
Cadence: 1 hour 5 minutes 20 seconds
Compression: DPCM
Data rate: 12.2949 kbits/s
Data volume: 48200.84 kbits
Emission lines:
186.75 Fe XII
188.23 Fe XI
192.90 O V
195.12 Fe XII
202.04 Fe XIII
203.83 Fe XIII
256.32 He II
274.20 Fe XIV
284.16 Fe XV
Warning:
-------
None
desc000326.txt
3920397
1
0
Coronal Hole
Scanning
49357655
0
2
2
309
1
120
St Andrews Plume Slot Study
sta_plume_slot
000327 sta_plume_slot
Danielle Bewsher
Science
12-Dec-2008
Study 000327:
ACRONYM: sta_plume_slot
Objective: to observe fast magnetoacoustic waves and Alfven waves in plumes.
Condition necessary to run and pointing:
----------------------------------------
Occurrence of a plume on the limb. Slot should cover the plume footpoint
and as much of the plume length as possible.
Study summary:
Slit/slot: 40" slot
No of pointing positions: 0 (sit 'n' stare)
Total spatial width: 40"
Pixels in solar-y: 512
Exposure time: 30 seconds
Number of repeats: 50
Cadence: 28 minutes 16 seconds
Compression: JPEG (Q=75)
Data rate: 17.2982 kbits/s
Data volume: 29333.33 kBits
Emission lines
188.23 Fe XI
192.82 Ca XVII
195.12 Fe XII
202.04 Fe XIII
203.83 Fe XIII
256.32 He II
262.98 Fe XVI
269.00 Mg VI
274.20 Fe XIV
275.35 Si VII
284.16 Fe XV
Instruction to planners:
------------------------
1) Run sta_plume_context
2) Run sta_plume_slot. Repeat N number of times to fill available time slot
3) Run sta_plume_context
Warning:
-------
None
desc000327.txt
1695747
1
0
Coronal Hole
Scanning
30037334
0
3
3
310
1
40
High data volume study for active region loop footpoints
PRY_footpoints_HI2
000328 PRY_footpoints_HI2
Peter Young
Science
12-Dec-2008
Study 000328:
ACRONYM: PRY_footpoints_HI2
This study is designed for a HOP where EIS receives 50% of the DR
allocation. The HOP is for measuring active region outflows, and EIS
should be pointed towards loop footpoints.
Care should be taken to ensure some quiet Sun is observed somewhere
along the slit in order to get a reliable wavelength calibration.
TARGET: Active region loop footpoints
EXPOSURE TIME: 25s
RASTER: scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 180"x512"
DURATION: 42 mins
VOLUME: 120 Mbits
Warning:
None
desc000328.txt
2561845
1
0
Active Region
Scanning
122583896
0
2
2
311
1
180
Equatorial coronal hole study, wide raster
YKK_EqCH_02W
000329 YKK_EqCH_02W
Harry Warren
Science
12-Dec-2008
Study 000329:
ACRONYM: YKK_EqCH_02w
This study is one of the two studies designed for measuring temperatures,
densities, velocities, and abundances in and at the boundary of equatorial
and low-latitude coronal holes. To improve the signal in weak lines,
2 long exposures are taken at each position in the raster.
TARGET: Coronal Hole
EXPOSURE TIME: 150s x 2 (2 exposures per raster position)
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 50"x400"
RASTER DURATION: 4h 32 m25s
COMPRESSION: DPCM
VOLUME: 121 Mbits
Pointing:
---------
An equatorial or low-latitude coronal hole (within 40 degrees to the
solar equator) during its passage across the central meridian.
Polar coronal hole extensions can also be a candidate of study if
it extends to below 40 degrees in latitude.
The slit field-of-view should at least cover the solar equator or,
if the coronal hole does not reach latitude zero, the lowest latitude
that the coronal hole covers.
Use/Instructions to planners:
-----------------------------
The objective of this study is the variation in physical properties
(temperature, density, velocity, abundances) along the longitudinal
extent of an equatorial or low-latitude coronal hole that may correspond
to different footpoints of the fast to slow solar wind. Therefore the
longitudinal coverage is essential.
This raster is used in combination with another study YKK_EqCH_02n
to complete a set of observations on
the coronal hole and its EAST boundary. A default set of study is as follows.
1) run twice the study YKK_EqCH_02n, one near the center of the coronal hole,
the other in between the center and the EAST coronal hole boundary.
2) run one time this study YKK_EqCH_02w at the EAST boundary of the
coronal hole, partly covering the 'visible' coronal hole,
partly covering the neighboring active region or quiet Sun at its east.
3) followed by one context raster (400"x400") covering the FOV of the
above raster runs.
Alternatively, two `slot shots' before and after the above raster runs
are OK too as long as it covers the FOV of the above raster runs.
The two studies (YKK_EqCH_02n and YKK_EqCH_02w) can be used in various
combinations depending on coronal size or planning restrictions. At least
three raster runs like the above default set on the same day are requested
in order to meet the objectives of the study. If not possible, the priority
is:
1) east coronal hole boundary,
2) in between the center and the EAST coronal hole boundary,
3) center of the coronal hole.
The pointing of multi raster runs should be made in a sequence that is
toward the east.
Warning:
--------
None.
desc000329.txt
16367657
1
0
Coronal Hole
Scanning
124251043
0
0
0
312
1
50
Equatorial coronal hole study, narrow raster
YKK_EqCH_02N
000330 YKK_EqCH_02N
Harry Warren
Science
12-Dec-2008
Study 000330:
ACRONYM:YKK_EqCH_02n
This study is one of the two studies designed for measuring temperatures,
densities, velocities, and abundances in and at the boundary of equatorial
and low-latitude coronal holes. To improve the signal in weak lines,
2 long exposures are taken at each position in the raster.
TARGET: Coronal Hole
EXPOSURE TIME: 150s x 2 (2 exposures per raster position)
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 25"x400"
RASTER DURATION: 2h 16 m 13s
COMPRESSION: DPCM
VOLUME: 61 Mbits
Pointing:
---------
An equatorial or low-latitude coronal hole (within 40 degrees to the solar
equator) during its passage across the central meridian. Polar coronal hole
extensions can also be a candidate of study if it extends to below 40
degrees in latitude.
The slit field-of-view should at least cover the solar equator or,
if the coronal hole does not reach latitude zero, the lowest latitude
that the coronal hole covers.
Use/Instructions to planners:
-----------------------------
The objective of this study is the variation in physical properties
(temperature, density, velocity, abundances) along the longitudinal extent
of an equatorial or low-latitude coronal hole that may correspond to different
footpoints of the fast to slow solar wind. Therefore the longitudinal coverage
is essential.
This raster is used in combination with another study YKK_EqCH_02w to complete
a set of observations on the coronal hole and its EAST boundary. A default set
of study is as follows.
1) run twice this study YKK_EqCH_02n, one near the center of the coronal hole,
the other in between the center and the EAST coronal hole boundary.
2) run one time the study YKK_EqCH_02w at the EAST boundary of the coronal hole,
partly covering the 'visible' coronal hole, partly covering the neighboring active
region or quiet Sun at its east.
3) followed by one context raster (400"x400") covering the FOV of the above raster
runs.
Alternatively, two `slot shots' before and after the above raster runs are OK too as
long as they cover the FOV of the above raster runs.
The two studies (YKK_EqCH_02n and YKK_EqCH_02w) can be used in various combinations
depending on coronal size or planning restrictions. At least three raster runs like
the above default set on the same day are requested in order to meet the objectives
of the study. If not possible, the priority is
1) east coronal hole boundary,
2) in between the center and the EAST coronal hole boundary,
3) center of the coronal hole.
The pointing of multi raster runs should be made in a sequence that is toward the east.
Warning:
--------
None.
desc000330.txt
8195078
1
0
Coronal Hole
Scanning
62125521
0
0
0
313
1
25
QS long duration slot movie. 104x216 FOV. JPEG65. Low data rate.
IUU_SLOT_104x216_Q65
000331 IUU_SLOT_104x216_Q65
Ignacio Ugarte
Science
23-Dec-2008
Study 000331:
ACRONYM: IUU_SLOT_104x216_Q65
Slot imaging. Low data rate. High compression. Three 28s exposures at
adjacent pointing positions sampling a 104"x216" FOV in around 90s. 8"
spatial overlap. 13 repeats totaling around 20min. Designed to run for
several hours (full day even) at low telemetry.
TARGET : Quiet Sun (QS)
EXPOSURE TIME : 28s
SLIT : 40"
FOV : 104"x216"
SPECTRAL WIND. : 8
COMPRESSION : JPEG65
Data rate : 4.58 kBits/s
Data Volume (per hour) : 16.5 MBits/h
ESTIMATED CADENCE : ~94 s per raster.
ESTIMATED DURATION : ~21 m (13 raster repeat)
WARNING:
None
desc000331.txt
1245735
1
0
Quiet Sun
Scanning
5844280
0
3
3
314
13
104
QS long duration slot movie. 104x280 FOV. JPEG65. Low data rate.
IUU_SLOT_104x280_Q65
000332 IUU_SLOT_104x280_Q65
Ignacio Ugarte
Science
23-Dec-2008
Study 000332:
ACRONYM: IUU_SLOT_104x280_Q65
Identical to (IUU_SLOT_104x216_Q65 - 216 pixel slit height)
BUT with 280 pixel slit height, i.e. slightely bigger data volume.
Slot imaging. Low data rate. High compression. Three 28s exposures at
adjacent pointing positions sampling a 104"x280" FOV in around 90s. 8"
spatial overlap. 13 repeats totaling around 20min. Designed to run for
several hours (full day even) at low telemetry.
TARGET : Quiet Sun (QS)
EXPOSURE TIME : 28s
SLIT : 40"
FOV : 104"x280"
SPECTRAL WIND. : 8
COMPRESSION : JPEG65
Data rate : 5.94 kBits/s
Data Volume (per hour) : 21.4 MBits/h
ESTIMATED CADENCE : ~94 s per raster.
ESTIMATED DURATION : ~21 m (13 raster repeat)
WARNING:
None
desc000332.txt
1245735
1
0
Quiet Sun
Scanning
7575932
0
3
3
315
13
104
coronal responses of QS transient brightenings
blinker_cr
000333 blinker_cr
Gerry Doyle
Science
8-Jan-2009
Study 000333:
ACRONYM: blinker_cr
Study description:
The purpose of this study is to understand the driving mechanism(s) of quiet
Sun brightenings in the solar atmosphere and their coronal responses.
Acronym : blinker_cr
Target : Quiet Sun
Raster : scanning
Slit : 2”
FOV : 70”x248”
Raster duration : 26m1s
Raster Data Volume : 17.5 Mbits
Pointing:
--------
quiet Sun at the disk center
Instruction to planners :
-------------------------
*** Requires raster repeat ****
To be run minimum 2 days, around 3 hours per day of continuous observations
i.e., around ** 7 raster repeat ** .
Solar rotational compensation is needed i.e., tracking the same region on
the Sun.
As it is a coordinated observation with SoHO, it is essential to have the
same FOV observed. If there is an offset between CDS/SoHO and EIS/Hinode,
it has to be taken into account.
It is essential to have simultaneous H-alpha and FGIV magnetograms / SOT
and Al Poly / XRT observations.
If/when the HOP run, please contact:
Maria Madjarska at
madjarska@mps.mpg.de
tel. +49 2406 303 5295
Warning:
None
desc000333.txt
1561273
1
0
Quiet Sun
Scanning
17885034
0
2
2
316
1
70
HPW017AR_30x400_30s_HOT_CA_LINES
HPW017AR_30x400_30s
000334 HPW017AR_30x400_30s
Harry Warren
Science
19-Jan-2009
Study 000334:
** Obsoleted by author, replace by V2 **
ACRONYM: HPW017AR_30x400_30s
* This is a narrow raster that can be expanded using ASRC (see below) *
This raster is designed for active region observations and includes
Ca XIV, XV, XVI, and XVII lines in addition to all of standard Fe lines.
Fe XXIII and XXIV are present. Cooler Mg lines are also included.
A complete line list is given below.
The extensive line list leads to a lot of telemetry being generated.
Using DPCM compression 47.7 Mbits will be generated for each run of this
raster. It may be possible to use higher compression levels, but many of the
interesting lines are weak and this may complicate the analysis. Lower
telemetry studies with fewer lines exist and may be a better choice when
a limited data volume is available.
181.90 16 # Ca XV 181.900
184.54 24 # Fe X 184.536
186.75 32 # Fe VIII 186.601, (Ca XIV 186.610), Fe XII 186.880
188.40 32 # Fe XI 188.216, Fe XI 188.299, Fe IX 188.497, S XI 188.675
192.20 32 # Fe XXIV 192.04, Fe XII 192.394
192.82 24 # Fe XI 192.813, Ca XVII 192.858
193.87 24 # Ca XIV 193.874
195.12 24 # Fe XII 195.119, Fe XII 195.180
201.05 24 # Ca XV 200.972, Fe XIII 201.121
202.04 24 # Fe XIII 202.044
203.83 24 # Fe XII 203.720, Fe XIII 203.826
208.50 32 # Ca XV 208.324, Ca XVI 208.604, (Fe XIII 208.679, Ca XV 208.722)
255.00 32 # Fe XVII 254.87, Fe XXIV 255.10
256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
262.98 24 # Fe XVI 262.984
263.98 40 # Fe XXIII 263.76, S X 264.233
270.52 24 # Mg VI 270.394, Fe XIV 270.519
275.40 24 # Si VII 275.352, Fe XVII 275.54
276.30 40 # Mg VII 276.153, Mg V 276.579
278.40 32 # Mg VII 278.402, Si VII 278.445
280.74 24 # Mg VII 280.737
284.16 24 # (Al IX 284.015), Fe XV 284.160
TARGET: Active Region
EXPOSURE TIME: 30s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 30"x400"
RASTER DURATION: 16m44s
VOLUME: 47.7 Mbits
RATE: 46.5 kbits/s
COMPRESSION: DPCM
Pointing:
---------
Any interesting place within the active region.
Use/Instructions to planners:
-----------------------------
This is a narrow raster that can be expanded using ASRC.
If used with ASRC, use the following ASRC parameters:
* Set the raster repeat parameter and enable ASRC.
Direction: Leave in FORWARD position (ASRC specific)
SKIP: Don't change -> 1 (ASRC specific)
Compensation steps: Set to 120
Warning:
--------
None.
desc000334.txt
1026448
1
0
Active Region
Scanning
48843513
0
0
0
317
1
30
HPW018AR300x400_30s_HOT_CA_LINES
HPW018AR300x400_30s
000335 HPW018AR300x400_30s
Harry Warren
Science
19-Jan-2009
Study 000335:
ACRONYM: HPW018AR300x400_30s
** Obsoleted by Author, replaced by V2 **
This raster is designed for active region observations and includes Ca XIV,
XV, XVI, and XVII lines in addition to all of standard Fe lines. Fe XXIII
and XXIV are present. Cooler Mg lines are also included. A complete line
list is given below.
The extensive line list leads to a lot of telemetry being generated. Using DPCM
compression 477 Mbits will be generated for each run of this raster. It may
be possible to use higher compression levels, but many of the interesting
lines are weak and this may complicate the analysis. Lower telemetry studies
with fewer lines exist and may be a better choice when a limited data
volume is available.
181.90 16 # Ca XV 181.900
184.54 24 # Fe X 184.536
186.75 32 # Fe VIII 186.601, (Ca XIV 186.610), Fe XII 186.880
188.40 32 # Fe XI 188.216, Fe XI 188.299, Fe IX 188.497, S XI 188.675
192.20 32 # Fe XXIV 192.04, Fe XII 192.394
192.82 24 # Fe XI 192.813, Ca XVII 192.858
193.87 24 # Ca XIV 193.874
195.12 24 # Fe XII 195.119, Fe XII 195.180
201.05 24 # Ca XV 200.972, Fe XIII 201.121
202.04 24 # Fe XIII 202.044
203.83 24 # Fe XII 203.720, Fe XIII 203.826
208.50 32 # Ca XV 208.324, Ca XVI 208.604, (Fe XIII 208.679, Ca XV 208.722)
255.00 32 # Fe XVII 254.87, Fe XXIV 255.10
256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
262.98 24 # Fe XVI 262.984
263.98 40 # Fe XXIII 263.76, S X 264.233
270.52 24 # Mg VI 270.394, Fe XIV 270.519
275.40 24 # Si VII 275.352, Fe XVII 275.54
276.30 40 # Mg VII 276.153, Mg V 276.579
278.40 32 # Mg VII 278.402, Si VII 278.445
280.74 24 # Mg VII 280.737
284.16 24 # (Al IX 284.015), Fe XV 284.160
TARGET: Active Region
EXPOSURE TIME: 30s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 300"x400"
RASTER DURATION: 2h47m42s
VOLUME: 477 Mbits
RATE: 47.4 kbits/s
COMPRESSION: DPCM
Pointing:
---------
The center of the active region.
Warning:
--------
None.
desc000335.txt
10061983
1
0
Active Region
Scanning
488435136
0
0
0
318
1
300
HPW019AR__1x400_45s_HOT_CA_LINES
HPW019AR__1x400_45s
000336 HPW019AR__1x400_45s
Harry Warren
Science
19-Jan-2009
Study 000336:
ACRONYM: HPW019AR__1x400_45s
** Obsoleted by Autor, replaced by V2 **
**** This is a sit-and-stare raster, don't forget some context! ****
This raster is designed for active region observations and includes Ca XIV,
XV, XVI, and XVII lines in addition to all of standard Fe lines. Fe XXIII
and XXIV are present. Cooler Mg lines are also included. A complete line
list is given below.
The extensive line list leads to a lot of telemetry being generated. Using DPCM
compression 116 Mbits will be generated every hour that this raster is run.
It may be possible to use higher compression levels, but many of the
interesting lines are weak and this may complicate the analysis. Lower
telemetry studies with fewer lines exist and may be a better choice when
a limited data volume is available.
181.90 16 # Ca XV 181.900
184.54 24 # Fe X 184.536
186.75 32 # Fe VIII 186.601, (Ca XIV 186.610), Fe XII 186.880
188.40 32 # Fe XI 188.216, Fe XI 188.299, Fe IX 188.497, S XI 188.675
192.20 32 # Fe XXIV 192.04, Fe XII 192.394
192.82 24 # Fe XI 192.813, Ca XVII 192.858
193.87 24 # Ca XIV 193.874
195.12 24 # Fe XII 195.119, Fe XII 195.180
201.05 24 # Ca XV 200.972, Fe XIII 201.121
202.04 24 # Fe XIII 202.044
203.83 24 # Fe XII 203.720, Fe XIII 203.826
208.50 32 # Ca XV 208.324, Ca XVI 208.604, (Fe XIII 208.679, Ca XV 208.722)
255.00 32 # Fe XVII 254.87, Fe XXIV 255.10
256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
262.98 24 # Fe XVI 262.984
263.98 40 # Fe XXIII 263.76, S X 264.233
270.52 24 # Mg VI 270.394, Fe XIV 270.519
275.40 24 # Si VII 275.352, Fe XVII 275.54
276.30 40 # Mg VII 276.153, Mg V 276.579
278.40 32 # Mg VII 278.402, Si VII 278.445
280.74 24 # Mg VII 280.737
284.16 24 # (Al IX 284.015), Fe XV 284.160
TARGET: Active Region
EXPOSURE TIME: 45s
RASTER: Sit-and-Stare
SLIT: 1"
STEP SIZE: 1"
FOV: 1"x400"
RASTER DURATION: 1h0m15s
VOLUME: 116 Mbits
RATE: 32.1 kbits/s
COMPRESSION: DPCM
Instruction to planners:
-----------------------
* Run context raster
* Run study
* Run context raster
Consult Harry Warren.
Pointing:
---------
An part of an active region
Warning:
--------
None.
desc000336.txt
3615191
1
0
Active Region
Scanning
118852549
0
0
0
319
1
1
RAH Line Narrowing
rah_line_narrow
000337 rah_line_narrow
Danielle Bewsher
Science
28-Jan-2009
Study 000337:
ACRONYM: rah_line_narrow
Objective:
---------
Observe line narrowing above the solar limb
Study summary:
-------------
Slit/slot: 2" slit
No of pointing positions: 59 (scanning)
Step size: 4"
Total spatial width: 238"
Pixels in solar-y: 256
Exposure time: 60 seconds
Cadence: 1 hour 5 minutes 20 seconds
Compression: DPCM
Data rate: 6.3524 kbits/s
Data volume: 25 Mbits
Emission lines
184.54 Fe X (32 pixel window)
192.90 O V (56 pixel window, wavelength range 192.65 - 193.88, also
includes Fe XI 192.83 and Fe XII 193.51)
195.12 Fe XII (32 pixel window)
202.04 Fe XIII (32 pixel window, density sensitive with Fe XIII 203.83)
203.83 Fe XIII (32 pixel window, density sensitive with Fe XIII 202.04)
256.32 He II (32 pixel window)
275.55 Si VII (32 pixel window)
Condition necessary to run and pointing:
----------------------------------------
On the limb above the equator (solar_y = 0). The limb should be seen in
the fov, but maximise the altitude above the limb that can be observed.
Instruction to planners:
-----------------------
Minimum of 6 hours observations requested. Fill time available with
as many repeats as possible. Avoid SAA
Either:
1) run using raster repeat in the golden period (light skirmishes with one SAA)
Or
2) Space as individual studies in betwenn SAAs
Warning:
--------
Do not run in SAA
desc000337.txt
2030397
1
0
Quiet Sun
Scanning
23033572
0
2
2
320
1
238
RAH Line Narrowing - 2" slit
rah_line_narrow_v2
000338 rah_line_narrow_v2
Danielle Bewsher
Science
29-Jan-2009
Study 000338:
ACRONYM: rah_line_narrow_v2
Objective:
---------
Observe line narrowing above the solar limb
Study summary:
-------------
Slit/slot: 2" slit
No of pointing positions: 59 (scanning)
Step size: 4"
Total spatial width: 238"
Pixels in solar-y: 256
Exposure time: 60 seconds
Cadence: 1 hour 5 minutes 20 seconds
Compression: DPCM
Data rate: 6.3524 kbits/s
Data volume: 25 Mbits
Emission lines
184.54 Fe X (32 pixel window)
192.90 O V (56 pixel window, wavelength range 192.65 - 193.88, also
includes Fe XI 192.83 and Fe XII 193.51)
195.12 Fe XII (32 pixel window)
202.04 Fe XIII (32 pixel window, density sensitive with Fe XIII 203.83)
203.83 Fe XIII (32 pixel window, density sensitive with Fe XIII 202.04)
256.32 He II (32 pixel window)
275.55 Si VII (32 pixel window)
Condition necessary to run and pointing:
----------------------------------------
On the limb above the equator (solar_y = 0). The limb should be seen in
the fov, but maximise the altitude above the limb that can be observed.
Instruction to planners:
-----------------------
Minimum of 6 hours observations requested. Fill time available with
as many repeats as possible. Avoid SAA
Either:
1) run using raster repeat in the golden period (light skirmishes with one SAA)
Or
2) Space as individual studies in betwenn SAAs
Warning:
--------
Do not run in SAA
desc000338.txt
3920397
1
0
Quiet Sun
Scanning
25501455
0
2
2
321
1
238
Coronal Hole, off limb, context study: 2" slit spatial raster
ab_CH_offlimb_cntxt
000339 ab_CH_offlimb_cntxt
Science
Alessandro Bemporad
18-Feb-2009
Study 000339:
ACRONYM: ab_ch_offlimb_cntxt
******* OBSOLETED due to an error in category vs author *****
Re-import if needed again
Objective:
---------
Context raster for Coronal Hole Observations
Study summary:
-------------
slot: 2"
S/C pointing: X=0", Y=-945" (off limb)
window height: 512"
exposure time: 100s
# of pointing: 39
step size: 2"
duration: 1h 11m 18s
Data Volume: 24 Mbits
Spectral lines:
- density study: Fe XII 195.12/186.85, Fe XIV 264.8/274.2
- kinetic temperature study: Si VII 275.35, Ca XIV 193.87,
Fe XV 284.16, Fe XIII 202.04
- comparison with previous UVCS data: O VI 184.00
- core lines: Ca XVII 192.82, He II 256.32
Instruction to planner:
----------------------
This is a context raster to be run with study ID #340 ( ab_ch_offlimb_sands)
Warning:
--------
None
desc000339.txt
4301098
1
0
Coronal Hole
Scanning
43873471
0
2
2
322
1
80
Coronal Hole, off limb, sit & stare study: 1" slit, 500s exposure time
ab_CH_offlimb_sands
000340 ab_CH_offlimb_sands
Science
Alessandro Bemporad
18-Feb-2009
Study 000340:
ACRONYM: ab_ch_offlimb_sands
******* OBSOLETED due to an error in category vs author *****
Re-import if needed again
Objective:
---------
Long duration sit and stare Coronal Hole Observation for HOP103.
Study summary:
-------------
slit: 1"
S/C pointing: X=0", Y=-945" (off limb)
window height: 512"
exposure time: 500s
# of exposures: 155
duration: 22h 41m 19s
Data Volume: 166 Mbits
Spectral lines:
- density study: Fe XII 195.12/186.85, Fe XIV 264.8/274.2
- kinetic temperature study: Si VII 275.35, Ca XIV 193.87,
Fe XV 284.16, Fe XIII 202.04
- comparison with previous UVCS data: O VI 184.00
- core lines: Ca XVII 192.82, He II 256.32
Pointing:
---------
South coronal hole (off limb observations).
Spacecraft pointing: X=0", Y=-945"
EIS Ystart = 1 (cannot use Ystart = 0) (bottom of the CCD).
This implies 16 pixels inside the limb and (512-16) pixels off the limb
Instruction to planners:
-----------------------
Run the folllowing sequence (preferably chained)
1) Run context study (ab_ch_offlimb_cntxt)
2) Run SNS study (ab_ch_offlimb_sands_2)
3) Run context study (ab_ch_offlimb_cntxt)
Run the study CONTINUOUSLY even through the SAAs.
Warning:
--------
Must run through SAA
***********
POC:
name: Dr. Alessandro Bemporad
email: bemporad@oato.inaf.it
phone: +39 011 8101 954
**********
desc000340.txt
81702067
1
0
Coronal Hole
Scanning
170009703
0
0
0
323
1
1
Coronal Hole study: JS_CH_280x256_2arc with 90s, modified version of study 267 to increase DN/pixel
JS_CH_280x256_2arc
000341 JS_CH_280x256_2arc
Unknown
Science
5-Mar-2009
Study 000341:
Acronym: JS_CH_280x256_2arc
TARGET: Coronal Hole
Coronal Hole study: JS_CH_280x256_2arc with 90s, modified version
of study 267 to increase DN/pixel
Study description:
The target of this study is a polar coronal hole. EIS should be pointed
to include the boundary of the coronal hole and the limb. The purpose
is to obtain velocity maps of million degree plasma.
2"slit scan, FOV 280"x256", 90sec exp time. DCPM compression is used to
get good line profile.
Duration: 3h 45m
Volume: 97 Mbits
Instruction to planners:
1. It would be better to run REGCAL 071 & 072 studies prior to run this study.
2. Ideally this study should run repeatedly (e.g. 4 or 5 times consecutively).
WARNING:
None
desc000341.txt
13527592
1
0
Coronal Hole
Scanning
99812148
0
2
2
324
1
280
Quiet_Sun_alternating_slots_for_Dopplershifts
dei_qs_80_slot40_lo
000342 dei_qs_80_slot40_lo
Davina Innes
Science
5-Mar-2009
Study 000342:
ACRONYM: dei_qs_80_slot40_low
Takes two neighbouring slot positions, separated by 38".
The aim is to put the left and right window edges repetitively at
the same position on the Sun, so that both wings of high Doppler shift
events at the window edge appear beyond the main line window. A small
sample of clean slot windows have been chosen. Windows are wide, not less
than 64 pixels
TARGET: Quiet Region of Sun
EXPOSURE TIME: 60 s
SLIT: 40"
FOV: 78"x384"
SPECTRAL WIND: 6
DATA COMP.: JPEG(Q=90)
Duration: 2m 32s
Volume: 1.3 Mbits
Target:
Filaments, Prominences, Quiet Sun.
Warning:
None
desc000342.txt
152430
1
0
Quiet Sun
Scanning
1351680
0
3
3
325
1
78
RAL Helium Intensities - 2" slit
ral_he_int_2slit
000343 ral_he_int_2slit
Danielle Bewsher
Science
5-Mar-2009
Study 000343:
ACRONYM: ral_he_int_2slit
Objective: Predict Helium intensities in the solar atmosphere
Study summary:
Slit/slot: 2" slit
No of pointing positions: 29 (scanning)
Total spatial width: 60"
Pixels in solar-y: 256
Exposure time: 20 seconds
Cadence: 11m 51s
Compression: DPCM
Data rate: 23.1480 kbits/s
Data volume: 16.5 MBits
Emission lines
184.29 O VI (72 pixel window, wavelength range 183.49 - 185.07,
includes Fe X 184.54)
186.88 Fe XII (40 pixel window, wavelength range 186.43 - 187.30,
includes Fe VIII 186.6)
193.28 O V (56 pixel window, wavelength range 192.65 - 193.88,
includes Fe XI 192.83 and Fe XII 193.51)
256.32 He II (32 pixel window)
262.98 Fe XVI (32 pixel window)
275.55 Si VII (48 pixel window, wavelength range 275.02 - 276.06,
includes Si VII 275.35)
280.02 O IV (48 pixel window, wavelength range 279.49 - 280.35,
including O IV 279.63 and O IV 279.93)
Target:
Target 1: Active Region on disk
Traget 2: Quiet Sun preferably near disk centre
Warning:
None
desc000343.txt
711448
1
0
Quiet Sun
Scanning
16863865
0
2
2
326
1
60
RAL Helium Intensities - 1" slit
ral_he_int_1slit
000344 ral_he_int_1slit
Danielle Bewsher
Science
5-Mar-2009
Study 000344:
ACRONYM: ral_he_int_1slit
Objective: Predict Helium intensities in the solar atmosphere
Study summary:
Slit/slot: 1" slit
No of pointing positions: 59 (scanning)
Total spatial width: 60"
Pixels in solar-y: 256
Exposure time: 40 seconds
Cadence: 44m 20s
Compression: DPCM
Data rate: 12.3806 kbits/s
Data volume: 33 Mbits
Emission lines
184.29 O VI (72 pixel window, wavelength range 183.49 - 185.07,
includes Fe X 184.54)
186.88 Fe XII (40 pixel window, wavelength range 186.43 - 187.30,
includes Fe VIII 186.6)
193.28 O V (56 pixel window, wavelength range 192.65 - 193.88,
includes Fe XI 192.83 and Fe XII 193.51)
256.32 He II (32 pixel window)
262.98 Fe XVI (32 pixel window)
275.55 Si VII (48 pixel window, wavelength range 275.02 - 276.06,
includes Si VII 275.35)
280.02 O IV (48 pixel window, wavelength range 279.49 - 280.35,
including O IV 279.63 and O IV 279.93)
Target:
Target 1: Active Region on disk
Traget 2: Quiet Sun preferably near disk centre
Warning:
None
desc000344.txt
2660397
1
0
Quiet Sun
Scanning
33727731
0
0
0
327
1
60
HOP : Study of Coronal Hole Dynamics from EIS/Hinode and SUMER/SOHO (scan)
aks_slit_raster_pch
000345 aks_slit_raster_pch
A.K. Srivastava
Science
23-Mar-2009
Study 000345:
ACRONYM: aks_slit_raster_pch
This is a context raster to be used with aks_slit_sas_pch.(#ID 346)
Exposure time: 300 s
Slit : 1" slit
Window width: 56 pixels
Window Height : 512 pixels
***** Rotation compensation: off ******
No.of pointing positions: 50, Step size : 1", Total spatial width : 51"
(No. of exposures = 51)
Compression: lossless
Duration : 4h 29m 25s
Data Rate : 5.9138 KB/s
Data Volume : 95 Mbits
desc000345.txt
16187712
1
0
Coronal Hole
Scanning
97892684
0
0
0
328
1
51
HOP : Study of Coronal Hole Dynamics from EIS/Hinode and SUMER/SOHO (SAS)
aks_slit_sas_pch
000346 aks_slit_sas_pch
A.K. Srivastava
Science
23-Mar-2009
Study 000346:
ACRONYM: aks_slit_sas_pch
Objective:
The scan and Sit&Statr observations by the 1" slit will
provide the spatial and temporal variation of plasma parameters respectively
in the polar coronal holes. The study of these crucial parameters will
enable us to investigate coronal hole dynamics, linking it with possible
MHD waves.
Target: CH
Exposure time: 300 s
Slit: 1" slit
Window width: 56 pixels
Window Height : 512 pixels
***** Rotation compensation: On ********
Total duration of study: 4 h 24 min 08 s
Data Rate: 5.9138 KB/s DCPM (Lossless)
Data Volume : 93 Mbits
Pointings (Target):
------------------
On-disk and Off-limb regions at the solar poles. Slit is positioned so
that 2/3 pixels of the total slit height (512 pixels) must be off-limb,
while the rest of the pixels must be on-disk. The field of view should also
capture the plume and interplume structures at the poles.
Instruction to planners:
------------------------
1) Run (aks_slit_sas_pch). Rotation compensation: ON
2) Run context study (aks_slit_raster_pch). Rotation compensation: OFF
Total DV: 95+93 = 188 Mbits
Warning:
None
desc000346.txt
15870747
1
0
Coronal Hole
Scanning
95973219
0
0
0
329
1
1
Interleaved rasters 50x320 for QS/CH
SK_QS_50x320i
000347 SK_QS_50x320i
Suguru Kamio
Science
26-Mar-2009
Study 000347:
ACRONYM: SK_QS_50x320i
The study consists of two identical rasters
which have 4" step size with 2" slit to
perform interleaved rasters.
The second raster must be shifted by 2" with respect
to the first raster (see instructions below).
It is designed to trace the variations of low
tempearture corona as well as microflares.
The study uses the following emission lines:
He II 256.3
O V 192.9
Fe VIII 186.6
Si X 261.0
Fe XI 192.8
Fe XII 186.9/195.2
Fe XV 284.2
Fe XVII 254.9
TARGET: Quiet region and coronal hole
EXPOSURE TIME: 25 sec
RASTER: scanning
SLIT: 2"
STEP SIZE: 4"
FOV: 50"x320"
DURATION: 12 min (6 min x 2 rasters)
COMPRESSION: JPEG90
VOLUME: 6.1 Mbits
DATA RATE: 31Mbits / hour
Instruction to planners:
1. Put an entry in the timeline.
2. Point the first raster at the target.
3. The second raster must be shifted to the West
by 2" (+2" in X coordinate) with respect to
the first raster so that the two consecutive
rasters make a complete scan.
4. Append a new enrty by copying it using the planning tool
(Study -> Selected (single) entry -> Copy to cursor time)
5. Continue copying until it reaches the end of the observing
period, avoiding SAAs.
Warning:
None
desc000347.txt
757588
2
0
Quiet Sun
Scanning
6233912
0
2
2
330
1
50
330
1
50
Active region raster
madj_ar
000348 madj_ar
Mike Marsh
Science
26-Mar-2009
Study 000348:
ACRONYM: madj_ar
This is a context raster to be used with study ID #349
Target: active region
Expsore time: 15 sec
slit: 2"
Step size: 2"
FOV: 70"x248"
Duration: 10m 43s
Volume: 18 Mbits
Pointing:
---------
Active region
Solar rotational compensation On, i.e. tracking the same region on the Sun
Warning:
Do not start the context raster within SAA
desc000348.txt
642523
1
0
Active Region
Scanning
18156019
0
2
2
331
1
70
Active region small raster
madj_ar_small
000349 madj_ar_small
Mike Marsh
Science
26-Mar-2009
Study 000349:
ACRONYM: madj_ar_small
The study will run in active region.
Target: active region
Expsore time: 15 sec
slit: 2"
Step size: 2"
FOV: 24"x248"
Duration: 3m 55s
Volume: 6 Mbits
Pointing:
---------
Active region
Solar rotational compensation on, i.e. tracking the same region on the Sun
Intruction to planners:
-----------------------
1) Run context raster (madj_ar, ID #348) (do not run in SAA)
2) Run madj_ar_small (preferably chained to the context in 1, i.e.
append to highlighted entry). Repeat raster to fill the available time
slot. Study madj_ar_small should continue through SAAs.
Warning:
--------
Do not start the *context* raster within SAA.
desc000349.txt
235079
1
0
Active Region
Scanning
6224921
0
2
2
332
1
24
vel_ch_sumer_SI005
CHvel_240x400_sumer
000350 CHvel_240x400_sumer
Shin Imada
Science
3-Apr-2009
Study 000350:
ACRONYM: CHvel_240x400_sumer
Study summary:
--------------
slit: 2"
S/C pointing: polar coronal hole
window height: 400"
exposure time: 30s
# of pointing: 119
step size: 2"
duration: 1h 6m 55s
Data Volume: 80 Mbits
Data Rate: 20 kBits/s
Lines: He II 256, O V 193, Si VII 275.35, Fe X 184.5, Fe XI 188.23,
Fe XII 195.12, Fe XIII 202.4, Fe XV 284.
Instruction to planner and pointing:
------------------------------------
Raster scan of a 240"x400" centered over the north limb
with the 2" slit, 30 s exposure and 2" steps (120 spectra),
to cover the required region in 1 h.
This study is design for the observation of velocity fields at the base
of polar coronal holes.
This study is for April 2009 Hinode/SUMER campaign.
Target will be the limb of a polar coronal hole.
Because of technical requirements in implementing the SUMER
observing program, the target need to be the North polar coronal hole.
Please repeat *FIVE* times at SUMER campaign.
Warning:
--------
None
desc000350.txt
4038293
1
0
Coronal Hole
Scanning
82262759
0
2
2
333
1
240
Coronal hole, 60"x512" raster, 240s exp.time
LANDI_SCAN_CH
000351 LANDI_SCAN_CH
Enrico Landi
Science
3-Apr-2009
Study 000351:
ACRONYM: LANDI_SCAN_CH
Purpose:
-------
The aim of this sequence (and of HOP 107) is to measure the dependence
of the ion temperature on the charge-over-mass ratio (Q/A) in polar coronal
holes as a function of distance from the limb. The Q/A ratio will be used to
test/validate theoretical models of fast solar wind acceleration that rely on
ion-cyclotron waves, along the guidelines of Landi & Cranmer 2009. This
investigation requires the observation of lines from a very large number
of different ions, and to maximize the number of ions
available it needs to be run in the same place and at the same time with a
full spectral scan from SOHO/SUMER.
Line intensities will be used to measure the electron density, the plasma
temperature distribution, and the element abundances of the plasma as a
function of distance from the limb.
Repeating the study in plumes and in interplume lanes is desired, the
60" E-W raster will allow us to observe both plasma structures within
the same scan.
The need to observe the line profiles and intensities for as many ions as
possible and for as many distances from the limb as possible in polar
coronal holes justifies the use of the full length of the
EIS slit. The wide 2" slit is selected as compromis between high-resolution
and large signal-to-noise ratio.
Target: CH
Expsore time: 240 Second
slit: 2"
Step size: 2"
FOV: 60"x512"
Duration: 2h 7m 21s
Volume: 164 Mbits
Instruction to planners:
------------------------
Repeat the raster, when possible, to fill the available time slot.
Pointing:
--------
The ideal pointing for this study is off-disk in polar coronal holes,
at the central meridian, to maximize the distance from the limb covered by
the slit. Pointing will be adjusted to include plume and interplume lanes.
Warning:
-------
None
desc000351.txt
7641448
1
0
Coronal Hole
Scanning
168315633
0
2
2
334
1
60
Study for comparing slit and slot data calibration
CALIB_slit_slot_v1
000352 CALIB_slit_slot_v1
Peter Young
Calibration
17-Apr-2009
Study 000352:
******* Replaced by Study ID #389 **********
ACRONYM: CALIB_slit_slot_v1
**** CALIBRATION study ****
This study takes 3 small rasters using the 40", 1" and 2" slits (in
this order) to allow the intensity calibration for each to be
compared, and also to check the instrumental width of the 2" slit.
DURATION: 18.5 mins
VOLUME: 26.6 Mbits
Pointing:
--------
The study should be run on a variety of targets, including quiet Sun,
active regions and off-limb.
Instruction to planners:
-----------------------
The CO should ensure that, when setting the pointing, the same
heliocentric coordinates are used for all three rasters
Warning:
-------
1 - Do not use within SAA
2 - Do not use within Eclipse passes
desc000352.txt
1098343
3
0
Quiet Sun
Scanning
27221774
2
3
2
335
1
104
336
1
15
337
1
30
Heavily compressed (Q=50) slot context raster; 488"x488"; 3.5mins
PRY_slot_context_v3
000353 PRY_slot_context_v3
Peter Young
Science
17-Apr-2009
Study 000353:
ACRONYM: PRY_slot_context_v3
This version of PRY_slot_context has a smaller spatial step between
exposures which improves the final images. Fe XI 180.4 replaces Fe X
184.5 and Fe XXIII 263.76 has been added.
This study is useful both as a context study and also for generating
high cadence movies for active regions.
TARGET: Active regions
EXPOSURE TIME: 10s
RASTER: scanning
SLIT: 40"
STEP SIZE: 32"
FOV: 488"x488"
DURATION: 3.5 mins
VOLUME: 4.9 Mbits
Warning:
None
desc000353.txt
209474
1
0
Active Region
Scanning
4989137
0
3
3
338
1
488
Heavily compressed slot context raster; 488"x488"; 3.5mins; reduced line list
PRY_slot_contextLITE
000354 PRY_slot_contextLITE
Peter Young
Science
17-Apr-2009
Study 000354:
ACRONYM: PRY_slot_contextLITE
This version of PRY_slot_context is the same as PRY_slot_context_v3
except that the line list has been reduced to enable the study to be
run for longer periods.
For obtaining single context images, PRY_slot_context_v3 is
preferred.
TARGET: Active regions
EXPOSURE TIME: 10s
RASTER: scanning
SLIT: 40"
STEP SIZE: 32"
FOV: 488"x488"
DURATION: 3.5 mins
VOLUME: 2.4 Mbits
Warning:
None
desc000354.txt
209474
1
0
Active Region
Scanning
2494568
0
3
3
339
1
488
HPW017AR_30x400_30s_HOT_CA_LINES_v2
HPW017AR_30x400_30s2
000355 HPW017AR_30x400_30s2
Harry Warren
Science
20-Apr-2009
Study 000355:
ACRONYM: HPW017AR_30x400_30s2
* Version 2 of HPW017, modified line list added O VI 184.117 and
Ar XIV 194.396, fixed error in Fe XXIII/S X window.
* This is a narrow raster that can be expanded using ASRC (see below) *
This raster is designed for active region observations and includes
Ca XIV, XV, XVI, and XVII lines in addition to all of standard Fe lines.
Fe XXIII and XXIV are present. Cooler Mg lines are also included. A complete
line list is given below.
The extensive line list leads to a lot of telemetry being generated. Using DPCM
compression 49.4 Mbits will be generated for each run of this raster. It
may be possible to use higher compression levels, but many of the interesting
lines are weak and this may complicate the analysis. Lower telemetry studies
with fewer lines exist and may be a better choice when a limited data volume
is available.
181.90 16 # Ca XV 181.900
184.33 32 # O VI 184.117, Fe X 184.536
186.75 32 # Fe VIII 186.601, (Ca XIV 186.610), Fe XII 186.880
188.40 32 # Fe XI 188.216, Fe XI 188.299, Fe IX 188.497, S XI 188.675
192.20 32 # Fe XXIV 192.04, Fe XII 192.394
192.82 24 # Fe XI 192.813, Ca XVII 192.858
194.10 40 # Ca XIV 193.874, Ar XIV 194.396
195.12 24 # Fe XII 195.119, Fe XII 195.180
201.05 24 # Ca XV 200.972, Fe XIII 201.121
202.04 24 # Fe XIII 202.044
203.83 24 # Fe XII 203.720, Fe XIII 203.826
208.50 32 # Ca XV 208.324, Ca XVI 208.604, (Fe XIII 208.679,
Ca XV 208.722)
255.00 32 # Fe XVII 254.87, Fe XXIV 255.10
256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
262.98 24 # Fe XVI 262.984
263.98 40 # Fe XXIII 263.76, S X 264.233
270.52 24 # Mg VI 270.394, Fe XIV 270.519
275.40 24 # Si VII 275.352, Fe XVII 275.54
276.30 40 # Mg VII 276.153, Mg V 276.579
278.40 32 # Mg VII 278.402, Si VII 278.445
280.74 24 # Mg VII 280.737
284.16 24 # (Al IX 284.015), Fe XV 284.160
TARGET: Active Region
EXPOSURE TIME: 30s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 30"x400"
RASTER DURATION: 16m44s
VOLUME: 49.6 Mbits
VOLUME/h: 150 Mbits/h
RATE: 49.4 kbits/s
COMPRESSION: DPCM
Pointing:
---------
Any interesting place within the active region.
Use/Instructions to planners:
-----------------------------
This is a narrow raster that can be expanded using ASRC.
If used with ASRC, use the following ASRC parameters:
* Set the raster repeat parameter and enable ASRC.
Direction: Leave in FORWARD position (ASRC specific)
SKIP: Don't change -> 1 (ASRC specific)
Compensation steps: Set to 120
Warning:
--------
None.
desc000355.txt
1026448
1
0
Active Region
Scanning
50771547
0
0
0
340
1
30
HPW018AR300x400_30s_HOT_CA_LINES_v2
HPW018AR300x400_30s2
000356 HPW018AR300x400_30s2
Harry Warren
Science
20-Apr-2009
Study 000356:
ACRONYM: HPW018AR300x400_30s
* Version 2 of HPW018, modified line list added O VI 184.117 and
Ar XIV 194.396, fixed error in Fe XXIII/S X window.
This raster is designed for active region observations and includes Ca XIV,
XV, XVI, and XVII lines in addition to all of standard Fe lines. Fe XXIII
and XXIV are present. Cooler Mg lines are also included. A complete line list
is given below.
The extensive line list leads to a lot of telemetry being generated. Using DPCM
compression 496 Mbits will be generated for each run of this raster. It
may be possible to use higher compression levels, but many of the interesting
lines are weak and this may complicate the analysis. Lower telemetry studies
with fewer lines exist and may be a better choice when a limited data volume
is available.
181.90 16 # Ca XV 181.900
184.33 32 # O VI 184.117, Fe X 184.536
186.75 32 # Fe VIII 186.601, (Ca XIV 186.610), Fe XII 186.880
188.40 32 # Fe XI 188.216, Fe XI 188.299, Fe IX 188.497, S XI 188.675
192.20 32 # Fe XXIV 192.04, Fe XII 192.394
192.82 24 # Fe XI 192.813, Ca XVII 192.858
194.10 40 # Ca XIV 193.874, Ar XIV 194.396
195.12 24 # Fe XII 195.119, Fe XII 195.180
201.05 24 # Ca XV 200.972, Fe XIII 201.121
202.04 24 # Fe XIII 202.044
203.83 24 # Fe XII 203.720, Fe XIII 203.826
208.50 32 # Ca XV 208.324, Ca XVI 208.604, (Fe XIII 208.679,
Ca XV 208.722)
255.00 32 # Fe XVII 254.87, Fe XXIV 255.10
256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
262.98 24 # Fe XVI 262.984
263.98 40 # Fe XXIII 263.76, S X 264.233
270.52 24 # Mg VI 270.394, Fe XIV 270.519
275.40 24 # Si VII 275.352, Fe XVII 275.54
276.30 40 # Mg VII 276.153, Mg V 276.579
278.40 32 # Mg VII 278.402, Si VII 278.445
280.74 24 # Mg VII 280.737
284.16 24 # (Al IX 284.015), Fe XV 284.160
TARGET: Active Region
EXPOSURE TIME: 30s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 1"
FOV: 300"x400"
RASTER DURATION: 2h47m19s
VOLUME: 496 Mbits
RATE: 49.4 kbits/s
COMPRESSION: DPCM
Pointing:
---------
The center of the active region.
Warning:
-------
High data volume (496 Mbits)
desc000356.txt
10061983
1
0
Active Region
Scanning
507715470
0
0
0
341
1
300
HPW019AR__1x400_45s_HOT_CA_LINES_v2
HPW019AR__1x400_45s2
000357 HPW019AR__1x400_45s2
Harry Warren
Science
20-Apr-2009
Study 000357:
ACRONYM: HPW019AR__1x400_45s
* Version 2 of HPW018, modified line list added O VI 184.117 and
Ar XIV 194.396, fixed error in Fe XXIII/S X window.
*** This is a sit-and-stare raster, don't forget some context! ***
This raster is designed for active region observations and includes Ca XIV,
XV, XVI, and XVII lines in addition to all of standard Fe lines. Fe XXIII and
XXIV are present. Cooler Mg lines are also included. A complete line list is
given below.
The extensive line list leads to a lot of telemetry being generated. Using DPCM
compression 121 Mbits will be generated every hour that this raster is run.
It may be possible to use higher compression levels, but many of the
interesting lines are weak and this may complicate the analysis. Lower
telemetry studies with fewer lines exist and may be a better choice when a
limited data volume is available.
181.90 16 # Ca XV 181.900
184.33 32 # O VI 184.117, Fe X 184.536
186.75 32 # Fe VIII 186.601, (Ca XIV 186.610), Fe XII 186.880
188.40 32 # Fe XI 188.216, Fe XI 188.299, Fe IX 188.497, S XI 188.675
192.20 32 # Fe XXIV 192.04, Fe XII 192.394
192.82 24 # Fe XI 192.813, Ca XVII 192.858
194.10 40 # Ca XIV 193.874, Ar XIV 194.396
195.12 24 # Fe XII 195.119, Fe XII 195.180
201.05 24 # Ca XV 200.972, Fe XIII 201.121
202.04 24 # Fe XIII 202.044
203.83 24 # Fe XII 203.720, Fe XIII 203.826
208.50 32 # Ca XV 208.324, Ca XVI 208.604, (Fe XIII 208.679,
Ca XV 208.722)
255.00 32 # Fe XVII 254.87, Fe XXIV 255.10
256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
262.98 24 # Fe XVI 262.984
263.98 40 # Fe XXIII 263.76, S X 264.233
270.52 24 # Mg VI 270.394, Fe XIV 270.519
275.40 24 # Si VII 275.352, Fe XVII 275.54
276.30 40 # Mg VII 276.153, Mg V 276.579
278.40 32 # Mg VII 278.402, Si VII 278.445
280.74 24 # Mg VII 280.737
284.16 24 # (Al IX 284.015), Fe XV 284.160
TARGET: Active Region
EXPOSURE TIME: 45s
RASTER: Sit-and-Stare
SLIT: 1"
STEP SIZE: 1"
FOV: 1"x400"
RASTER DURATION: 59m53s
VOLUME: 121 Mbits
RATE: 33.6 kbits/s
COMPRESSION: DPCM
Instruction to planners:
-----------------------
1) Run context HPW017AR_30X400_30s2 (ID #355)
2) Run this study
Pointing:
---------
Any part of an active region
Warning:
--------
None.
desc000357.txt
3615191
1
0
Active Region
Scanning
123544097
0
0
0
342
1
1
Fast scan, 58x368, 2" slit, 4" steps. AR line list.
IUU_SCAN_STEPS_002
000358 IUU_SCAN_STEPS_002
Ignacio Ugarte
Science
20-Apr-2009
Study 000358:
ACRONYM: IUU_SCAN_STEPS_002
This is a fast raster designed to do diagnostics of active region
dynamics. The 2" slit scans 58" in fourteen 4" steps at a cadence of 6
minutes, i.e. it samples 2" in every 4".
It includes Ca XIV, XV and XVII lines in addition to all of standard Fe
lines. Fe XXIII and XXIV are present. A complete line list is given
below.
Using JPEG90 compression 9 Mbits will be generated for each run of this
raster. Higher compression is not recommended.
184.33 32 # O VI 184.117, Fe X 184.536
186.75 32 # Fe VIII 186.601, (Ca XIV 186.610), Fe XII 186.880
188.40 32 # Fe XI 188.216, Fe XI 188.299, Fe IX 188.497,
S XI 188.675
192.20 32 # Fe XXIV 192.04, Fe XII 192.394
192.82 24 # Fe XI 192.813, Ca XVII 192.858
193.87 24 # Ca XIV 193.874
195.12 24 # Fe XII 195.119, Fe XII 195.180
201.05 24 # Ca XV 200.972, Fe XIII 201.121
202.04 24 # Fe XIII 202.044
203.83 24 # Fe XII 203.720, Fe XIII 203.826
256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
262.98 24 # Fe XVI 262.984
263.98 40 # Fe XXIII 263.76, S X 264.233
275.40 24 # Si VII 275.352, Fe XVII 275.54
284.16 24 # (Al IX 284.015), Fe XV 284.160
TARGET: Active Region
EXPOSURE TIME: 20s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 4"
FOV: 58"x368"
RASTER DURATION: 6m7s
VOLUME: 8.8 Mbits
RATE: 23.9 kbits/s
COMPRESSION: JPEG90
Pointing:
---------
The center of the active region.
Warning:
--------
None.
desc000358.txt
366974
1
0
Active Region
Scanning
8961248
0
2
2
343
1
58
Active Region Temperature Diagnostic - Lite Version
cam_ar_temp_lite
000359 cam_ar_temp_lite
Helen Mason
Science
29-Apr-2009
Study 000359:
Acronym: cam_ar_temp_lite
*******************************************************
* DEFUNCT : Replaced by cam_ar_temp_lite_v2 (ID #377) *
*******************************************************
This study is intended to be run on active regions on limb to study the
temperature structure of active regions.
Target: On Limb Active Region
Exposure time: 30s
Raster: scanning
Slit: 2"
Step Size: 2"
FOV: 360"X400"
Duration: 1h40m46s
Data Volume: 197 Mbits
Pointing:
--------
An active region on the limb. The raster should be centered at the
active region core.
Warning:
--------
None.
desc000359.txt
6046190
1
0
Active Region
Scanning
202302443
0
2
2
344
1
360
High cadence observations of active region transient brightenings and microflares
cam_artb_lite_v2
000360 cam_artb_lite_v2
Durgesh Tripathi
Science
29-Apr-2009
Study 000360:
Acronym: cam_artb_lite_v2
This study is intended to be run on active region to study transient
brightenings and microflares at a very high cadence. This would help us
measure the physical parameters of transient brightenings and microflares
during its evolution at a very high cadence.
Raster: Scanning
Slit: 2"
Step size: 2"
FOV: 40"X120"
Raster Duration: 4m 31s
Data Volume: 7 Mbits
Data Volume/h: ~100 Mbits/h
Pointing:
--------
The center of raster should be at the polarity inversion line.
Instruction to planners:
-----------------------
* Run PRY_slot_context_V3 (ID #353) BEFORE and AFTER this study
* This study should be run continuously for 3-4 hours (or longer if possible)
to get a good evolution time for a micoroflare, flare or transient
brightening.
Warning:
-------
None
desc000360.txt
271799
1
0
Active Region
Scanning
7492683
0
2
2
345
1
40
Active Region Transietn Brightening -- Lite
cam_artb_cds_a_lite
000361 cam_artb_cds_a_lite
Durgesh Tripathi
Science
29-Apr-2009
Study 000361:
Acronym: cam_artb_cds_a_lite
The study is intended to be run on on-disk active regions to study active
region transient brightening as well as density structure of active regions.
This would be combined with Magnetogram observations. Therefore its would be
useful to run this study when the active regions are closer to disk center.
Target: On Disk Active region
Exposure time: 10s
Raster: scanning
Slit: 2"
Step Size: 2"
FOV: 200"X400"
Raster Duration: 21m9s
Data Volume: 108 Mbits
Data Volume/h: 300 Mbits/h
Data Rate: 90 Kbits/s
Pointing:
--------
An active region on the disk. The raster should be centered at the active
region core or the polarity inversion line.
Instruction to planners:
-----------------------
* Run PRY_slot_context_V3 (ID #353) BEFORE and AFTER this study
Warning:
--------
Not very lite. Data volume = 300 Mbits/h, data rate = 90 Kbits/s
desc000361.txt
1268994
1
0
Active Region
Scanning
111141466
0
2
2
346
1
200
Eclipse raster which takes 60 % of spectrum; 3x3 arcmin
Eclipse_raster_v2
000362 Eclipse_raster_v2
Peter Young
Science
7-May-2009
Study 000362:
ACRONYM: Eclipse_raster_v2
This study is intended for taking reference spectra during the eclipse
season. It covers an area of 3x3 arcminute with the 2" slit, and takes
about 60% of the EIS spectrum. The spectral coverage is designed to
take mostly those parts of the CCD where the effective area is high,
ignoring low sensitivity areas.
The study can be run on any target, including high temperature active
regions.
TARGET: Any, including high temperature active regions.
EXPOSURE TIME: 30s
RASTER: scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 180"x176"
DURATION: 50 mins
VOLUME: 100 Mbits
Instructions to planners:
-------------------------
1) Run context study (PRY_slot_context_v3). Should be started
about 10 mins after the end of Hinode orbital night
2) Run Eclipse_raster_v2
Total duration = 54 minutes
Total data volume = 104 Mbits
The sequence above (items 1 and 2) should be repeated for consecutive
day-time periods, depending on the available data volume.
Warning:
--------
None
desc000362.txt
3034345
1
0
Quiet Sun
Scanning
101375993
0
2
2
347
1
180
FLR001_5s-exp_5m-rast_80"x120"_2"slit_fe14_den
FLR001_flare_study
000363 FLR001_flare_study
Ryan Milligan
Science
27-May-2009
Study 000363:
ACRONYM: FLR001_flare_study
This study is the default flare study for EIS and a test bed for future flare studies.
It is fast raster study designed to diagnose flaring plasma through the measurement
of line intensities, shifts, and widths over a range of high temperatures, as well as
electron densities using the Fe XIV ratio.
TARGET: Flare
EXPOSURE TIME: 5s
RASTER: Scanning
SLIT: 2":
STEP SIZE: 2"
FOV: 80"x120"
DURATION: 5m
VOLUME: 3 Mbits
VOLUME/HOUR: 36 Mbits
TARGET/POINTING:
----------------
The target should be a flare-producing active region, preferably aimed along the
magnetic neutral line if the target will not fit inside the FOV.
INTRUCTION TO PLANNERS:
-----------------------
1) Run the study for 16h/day or fill the TM allocation available,
by adjusting the raster repeat parameter.
2) Continuous run is required (run through SAAs).
3) Track the active region for the duration required,
using Hinode tracking mode
WARNING:
-------
None.
desc000363.txt
3485676
1
0
Flare
Scanning
37018236
0
2
2
348
12
80
Flush CCDs (10 flushes)
flush_ccds
000364 flush_ccds
Khalid al Janabi
Engineering
Study 000364:
ACRONYM: flush_ccds
This engineering sequence perform 10 CCDs flushes (dark current removals).
Warning:
None
desc000364.txt
1000
0
0
Engineering
SnS
0
0
0
0
XBP_CONTEXT_SI007
XBP_CONTEXT_SI007
000365 XBP_CONTEXT_SI007
Shin Imada
Science
6-Aug-2009
Study 000365:
ACRONYM: xbp_context_si007
This study is context raster for the observation of xbp transient phenomena
Raster scan of a 264"x256" with the 40" slot,
28 s exposure and 32" steps, to cover the required region in 4min.
Lines: Fe XII 195.12, He II 256, Fe XV 284.
Study summary:
-------------
slit: 40"
S/C pointing: xbp near disk center
window height: 256"
exposure time: 28s
# of pointing: 7
step size: 32"
duration: 4m
Voulume: 0.5 Mbits
TARGET:
------
X-ray Bright Point (HOP 0124, 2009 August)
Instruction to planner:
----------------------
THis study is a context raster for study (xbp_obs_si006).
This study is for HOP0124 which is planned end of August 2009.
Target will be the X-ray Bright Point near the disc center.
Warning:
--------
None
desc000365.txt
273420
1
0
Quiet Sun
Scanning
532813
0
3
3
349
1
264
XBP_OBS_SI006
XBP_OBS_SI006
000366 XBP_OBS_SI006
Shin Imada
Science
6-Aug-2009
Study 000366:
ACRONYM: xbp_obs_si006
This study is design for the observation of xbp transient phenomena.
Raster scan of a 40"x256" with the 2" slit,
30 s exposure and 2" steps (20 spectra),
to cover the required region in 11min.
Lines: Fe X 184.5, Fe XII 186.9, O V 192.9, Fe XII 195.12,
He II 256, Si VII 275.35, Fe XV 284.
Study summary:
-------------
slit: 2"
S/C pointing: xbp near disk center
window height: 256"
exposure time: 30s
# of pointing: 19
step size: 2"
duration: 11m
Volume: 2 Mbits
TARGET:
------
X-ray Bright Point (HOP 0124, 2009 August)
Instruction to planner:
----------------------
* Key note: This is a low data study. Switch to DPCM if possible
(default JPEG95)
1) Run context study (XBP_CONTEXT_SI007, ID #365). Repeat raster 3 times
for safety, unless otherwise requested.
2) Run this study. Repeat to fill the allocated time slot
3) Run context study (XBP_CONTEXT_SI007, ID #365). Repeat raster 3 times
for safety, unless otherwise requested.
Warning:
-------
None
desc000366.txt
691799
1
0
Quiet Sun
Scanning
1276915
0
2
2
350
1
40
488x512 Slot Scan. Basic unit to Full Sun Slot Scan.
full_sun_slot_scan_1
000367 full_sun_slot_scan_1
Ignacio Ugarte
Science
6-Aug-2009
Study 000367:
ACRONYM: FULL_SUN_SLOT_SCAN_1
This is the basic unit of the full solar disk slot scan. See HOP130
for details: "Multi-temperature Full Disk Slot Scan"
Fifteen, 20s exposures at adjacent pointings with a 8" overlap, resulting
in a 488"x512" FOV every 6 minutes.
TARGET: Quiet Sun and Active Region
EXPOSURE TIME: 20s
RASTER: Scanning
SLIT: 40"
STEP SIZE: 32"
FOV: 488"x512"
RASTER DURATION: 6m7s
VOLUME: 8 Mbits
RATE: 21.7 kbits/s
COMPRESSION: JPEG85
Pointing:
---------
Pointing (when run as HOP130)
15 spacecraft pointings covering full disk.
Two EIS pointings per spacecraft pointing, i.e.
**** TOP and BOTTOM portions of the CCDs with possible rows overlapping****
to maximize the area and minimize spacecraft pointings
Exact pointing positions and times will be provided by the points of contact:
Ignacio Ugarte-Urra (iugarte@ssd5.nrl.navy.mil) or
David Brooks (dhbrooks@ssd5.nrl.navy.mil)
Warning:
--------
If run for HOP130, (keep) compression at Q85 to avoid compression artifacts.
desc000367.txt
366974
1
0
Quiet Sun
Scanning
8158007
0
3
3
351
1
488
Coronal Hole study: JS_CH_280x256_2arc, modified version of study #341 (exp. time 90s -> 120s)
JS_CH_280x256_V3
000368 JS_CH_280x256_V3
Jian Sun
Science
6-Aug-2009
Study 000368:
Acronym: JS_CH_280x256_V3
Coronal Hole study: 120s exposure time version.
Modified version of study #341 (90S exposure time) to increase DN/pixel
2"slit scan, FOV 280"x256", 120S exp. time. DCPM compression is used to
get good line profile.
Duration: 4h 58m
Volume: 97 Mbits
TARGET: Coronal Hole
Pointing:
The target of this study is a polar coronal hole. EIS should be pointed
to include the boundary of the coronal hole and the limb. The purpose
is to obtain velocity maps of million degree plasma.
Instruction to planners:
1. It would be better to run REGCAL 071 & 072 studies prior to run this study.
*** Run REGCAL 071 & 072 only ONCE prior to multiple JS_CH run(s), per
day. I.e do not run the regcals more than once per 24h ***
2. Ideally this study should run repeatedly (e.g. 4 or 5 times consecutively).
WARNING:
None
desc000368.txt
17937592
1
0
Coronal Hole
Scanning
99812148
0
2
2
352
1
280
MicroType3_fullscan
MicroType3_fullscan
000369 MicroType3_fullscan
Shin Imada
Science
25-Aug-2009
Study 000369:
ACRONYM: MicroType3_fullscan
This study is designed to observe the evolution of active regions associated
with micro-type III radio bursts.
Study summary:
--------------
Raster scan of a 128"x256" centered Equatorial Coronal Hole Boundaries
with the 1" slit, 20 s exposure and 1" steps (128 spectra),
to cover the required region in 40 min.
S/C pointing: Equatorial Coronal Hole Boundaries
slit: 1"
# of pointing: 127
step size: 1"
window height: 256"
exposure time: 20s
duration: 42m 54s
Volume: 34 Mbits
Lines: FeXII(195.12, 196.65), FeXV(284.16), FeXVI(262.98), SiVII(275.35).
TARGET:
-------
Equatorial Coronal Hole Boundaries (HOP 129)
Instruction to planner:
-----------------------
DPCM is required for this study, However, JPEG 95 is acceptable.
This study is for HOP 129. Target will be the Equatorial Coronal Hole
Boundaries.
1) Run this study "Full scan mode".
2) This study should be followed by "Fast scan mode", study ID #370,
repeatedly.
Warning:
--------
None
desc000369.txt
2962013
1
0
Coronal Hole
Scanning
35098777
0
0
0
353
1
128
MicroType3_fastscan
MicroType3_fastscan
000370 MicroType3_fastscan
Shin Imada
Science
25-Aug-2009
Study 000370:
ACRONYM: MicroType3_fastscan
This study is designed to observe the evolution of active regions
associated with micro-type III radio bursts.
This study is for HOP 129.
Study summary:
--------------
Raster scan of a 128"x256" centered Equatorial Coronal Hole Boundaries
with the 1" slit, 20 s exposure and 4" steps (33 spectra),
to cover the required region in 40 min.
slit: 1"
S/C pointing: Equatorial Coronal Hole Boundaries
window height: 256"
exposure time: 20s
# of pointing: 32
step size: 4"
duration: 11m 0s
Volume: 9 Mbits
Lines: FeXII(195.12, 196.65), FeXV(284.16), FeXVI(262.98), SiVII(275.35).
TARGET:
------
Equatorial Coronal Hole Boundaries (HOP 129)
Instruction to planner:
----------------------
Keep DPCM data compression if possible. However, JPEG 95 is acceptable.
1) Run "FULL scan mode" study (ID #369), first
2) Run this study "FAST scan mode". Use the raster repeat function to
to fill the available time slot
Both studies are 128"X256" and should be pointed using the same X&Y
coordinates.
Warning:
--------
None
desc000370.txt
780343
1
0
Coronal Hole
Scanning
9048903
0
0
0
354
1
129
VHH_SlowAR_slow_scan_of_AR_to_search_for_line_assymetries_V2
VHH_SlowAR_5m_V2
000371 VHH_SlowAR_5m_V2
Viggo Hansteen
Science
1-Sep-2009
Study 000371:
ACRONYM: VHH_SlowAR_5m_DCPM
Fast sparse raster covering 256x240 arcsec with 30s exposures,
step size of 32 arcsec. Mainly constructed to give good S/N of line profiles
in an active region - line list is fairly unblended. Lossless compression.
Pointing can be anywhere, but meant to be run in conjunction with
VHH_SlowAR_2h20_DCPM to give time evolution or also VHH_SlowAR_1h12m to check
for JPEG compression artifacts in the line profiles. In the latter case the
pointings should be identical.
Study summary:
--------------
slit: 1"
step size: 32"
window height: 240"
exposure time: 30s
# of pointing: 8
duration: 5m 24s
Volume: 4 Mbits
Line list: CaXVII 192.82, FeXII 195.12, FeXIII 202.04, HeII 256.32,
SiX 258.37, SiX 261.04, FeXIV 264.78, FeXIV 274.20
SiVII 275.35
TARGET:
------
Anywhere on Sun Disc
Instruction to planner:
----------------------
This is a sparse raster to be used with study IDs #372 & #373.
***** Keep DPCM data compression*****
Warning:
--------
None
desc000371.txt
323685
1
0
Active Region
Scanning
4164552
0
0
0
355
1
257
VHH_SlowAR_slow_scan_of_AR_to_search_for_line_assymetries_V2M
VHH_SlowAR_1h12_V2
000372 VHH_SlowAR_1h12_V2
Viggo Hansteen
Science
1-Sep-2009
Study 000372:
ACRONYM: VHH_SlowAR_1h12m
Slow raster covering 256x240 arcsec with 30s exposures, step size of 2 arcsec.
Mainly constructed to give good S/N of line profiles in an active region - line
list is fairly unblended. JPEG compression. Pointing can be anywhere.
Study summary:
--------------
slit: 1"
step size: 2"
window height: 240"
exposure time: 30s
# of pointing: 128
duration: 1h 12m
Volume: 33 Mbits
Line list: CaXVII 192.82, FeXII 195.12, FeXIII 202.04, HeII 256.32,
SiX 258.37, SiX 261.04, FeXIV 264.78, FeXIV 274.20
SiVII 275.35
TARGET:
------
Anywhere on Sun Disc
Instruction to planner:
----------------------
1) Run study ID #370 (VHH_SlowAR_5m_DPCM), first. Keep DPCM data compression
2) Run this study. Repeat raster to fill the available time slot
Warning:
--------
None
desc000372.txt
4339478
1
0
Active Region
Scanning
34796020
0
0
0
356
1
257
VHH_SlowAR_2h20_DPCM
VHH_SlowAR_2h20_DPCM
000373 VHH_SlowAR_2h20_DPCM
Viggo Hansteen
Science
1-Sep-2009
Study 000373:
ACRONYM: VHH_SlowAR_2h20_DCPM
Slow raster covering 240x256 arcsec with 60s exposures, step size of 2 arcsec.
Mainly constructed to give good S/N of line profiles in an active region - line
list is fairly unblended. Lossless compression. Pointing can be anywhere.
Study summary:
--------------
slit: 1"
step size: 2"
window height: 256"
exposure time: 60s
# of pointing: 128
duration: 2h 20m
Volume: 60 Mbits
Line list: CaXVII 192.82, FeXII 195.12, FeXIII 202.04, HeII 256.32,
SiX 258.37, SiX 261.04, FeXIV 264.78, FeXIV 274.20
SiVII 275.35
TARGET:
------
Anywhere on Sun Disc
Instruction to planner:
----------------------
1) Run study ID #370 (VHH_SlowAR_5m_DPCM), first. Keep DPCM data compression
2) Run this study. Repeat raster to fill the available time slot
Warning:
--------
None
desc000373.txt
8402978
1
0
Active Region
Scanning
63671376
0
0
0
357
1
257
Multi-temperature observations of sigmoids
cam_sigmoid_study_v1
000374 cam_sigmoid_study_v1
Durgesh Tripathi
Science
22-Oct-2009
Study 000374:
ACRONYM: cam_sigmoid_study_v1
Using EIS data has shown the existence of sigmoidal structures at
lower coronal temperatures and interpreted as cooling plasma on newly
reconnected field lines within a flux rope. However, more specific
observations simultaneously at different temperatures are needed to
comprehend this result.
TARGET: Active Region
EXPOSURE TIME: 10s
RASTER: Scanning
SLIT: 2"
FOV: 400"x400"
RASTER DURATION: 41m 33s
Data Volume: 125 Mbits
Data rate: 50 Kbits/s
Line list:
----------
FeX,184.54; FeXII,186.88; FeXI,188.23; FeXII,195.12; FeIX,196.81;
FeXIII,202.04; FeXIII,203.83; FeXVII,254.87; FeXVI,262.98; FeXXIII,263.76;
FeXIV,274.20; SiVII,275.35; FeXV,284.16
Pointing:
---------
Small to medium size active regions. The pointing should be such that
the active region is located in the middle of the raster, Preferably at
the centre.
Instructions to planner:
------------------------
Adjust the raster repeat to fill the available time slot. However,
it would be very helpful scientifically if at least **4** repeats
can be supported
WARNING:
--------
Total data volume for the desired 4 repeats is ~500 Mbits
desc000374.txt
2515489
1
0
Active Region
Scanning
129873173
0
2
2
358
1
400
Deep exposures with 1 arcsec slit for measuring precise velocity
SK_DEEP_5x512_SLIT1
000375 SK_DEEP_5x512_SLIT1
Suguru Kamio
Science
22-Oct-2009
Study 000375:
ACRONYM: SK_DEEP_5x512_SLIT1
Deep exposure scan covering 5x512 arcsec with step size
of 1 arcsec. Spectral lines are selected to achieve precise
velocity measurement in a wide temperature range.
Study summary:
--------------
slit: 1"
step size: 1"
window height: 512"
exposure time: 120 sec
# of pointing: 4
duration: 10 min 40 sec
Volume: 7 Mbits
Line list:
Fe VIII 186.60
Fe X 184.54/257.26
Fe XI 180.40/188.30
Fe XII 192.39/195.12
Fe XIII 202.04
Fe XIV 264.79
Fe XV 284.16
He II 256.32
O IV 279.93
O V 192.75/192.91/248.46
Mg VI 268.99
Si VII 275.35
Si X 261.04
TARGET:
------
Quiet region at disk center or off-limb region
Instruction to planner:
----------------------
If you obtain full height spectrum (Y range:1-1023),
three consecutive scans must be performed with following
Y initial positions (YIP) in the EIS planning tool;
YIP = 1 (Y range:1-512)
YIP = 256 (Y range:256-767)
YIP = 512 (Y range:512-1023)
The first and the last ones record the bottom and the top halves.
The middle one is needed to bridge the top and the bottom spectra.
Mirror initial position (MIP) must be an identical number in all scans.
Spacecraft pointing should not be changed during the consecutive scans
(tracking is fine), i.e. all three pointings must be to the same region.
XRT support:
------------
It would be useful to ask XRT planner for a context image.
Warning:
--------
Some intense lines might be saturated in active regions.
desc000375.txt
662325
1
0
Quiet Sun
Scanning
7129439
0
0
0
359
1
5
Deep exposure with 2 arcsec slit for measuring precise velocity
SK_DEEP_10x512_SLIT2
000376 SK_DEEP_10x512_SLIT2
Suguru Kamio
Science
22-Oct-2009
Study 000376:
ACRONYM: SK_DEEP_10x512_SLIT2
This is a 2" slit version of SK_DEEP_5x512_SLIT1
Exposure time is reduced to 60 sec.
Study summary:
--------------
slit: 2"
step size: 2"
window height: 512"
exposure time: 60 sec
# of pointing: 4
duration: 5 min 25 sec
Volume: 7 Mbits
Line list:
Fe VIII 186.60
Fe X 184.54/257.26
Fe XI 180.40/188.30
Fe XII 192.39/195.12
Fe XIII 202.04
Fe XIV 264.79
Fe XV 284.16
He II 256.32
O IV 279.93
O V 192.75/192.91/248.46
Mg VI 268.99
Si VII 275.35
Si X 261.04
TARGET:
------
Quiet region at disk center or off-limb region
Instruction to planner:
----------------------
If you obtain full height spectrum (Y range:1-1023),
three consecutive scans must be performed with following
Y initial positions (YIP) in the EIS planning tool;
YIP = 1 (Y range:1-512)
YIP = 256 (Y range:256-767)
YIP = 512 (Y range:512-1023)
The first and the last ones record the bottom and the top halves.
The middle one is needed to bridge the top and the bottom spectra.
Mirror initial position (MIP) must be an identical number in all scans.
Spacecraft pointing should not be changed during the consecutive scans
(tracking is fine), i.e. all three pointings must be to the same region.
XRT support:
------------
It would be useful to ask XRT planner for a context image.
Warning:
--------
Some intense lines might be saturated in active regions.
desc000376.txt
347325
1
0
Quiet Sun
Scanning
7129439
0
2
2
360
1
10
large AR diagnostic raster, 320 x 380, 2'' slit, 45 sec
cam_ar_limb_lite_v2
000377 cam_ar_limb_lite_v2
Helen Mason
Science
4-Nov-2009
Study 000377:
Acronym: cam_ar_temp_lite_v2
This study is intended to be run on active regions on limb to study the
temperature structure of active regions.
Target: On Limb Active Region
Exposure time: 45s
Raster: scanning
Slit: 2"
Step Size: 2"
FOV: 322"X376"
Duration: 2h13m15s
Data Volume: 186 Mbits
Pointing:
--------
An active region on the limb. The raster should be centered at the
active region core.
Warning:
--------
None.
desc000377.txt
7995321
1
0
Active Region
Scanning
190164297
0
2
2
361
1
324
SLOT_imaging,_large_FOV._Quiet_Sun_(V2)
IUU_SLOT_488x512
000378 IUU_SLOT_488x512
Ignacio Ugarte
Science
4-Nov-2009
Study 000378:
ACRONYM: IUU_SLOT_488x512
Slot imaging, large FOV. Fourteen 30s exposures at adjacent pointing
positions sampling a 488"x512" area. 8" overlapping scan (40" Slot, 32"
FMIR step size). JPEG85 compression.
TARGET : Coronal hole / Quiet Sun
EXPOSURE TIME : 30s
RASTER : Scanning
SLIT : 40"
STEP SIZE : 32"
FOV : 418"x512"
SPECTRAL WIND. : 8
RASTER DURATION : ~8m 44s
COMPRESSION : JPEG85
Data Volume : 8.0 MBits
Data Volume (per hour) : 55 MBits/h
Line list:
Fe XI 180.4
Fe XII 195.1
Fe XIII 202.0
Fe XIII 203.8
He II 256.3
Fe XVI 263.0
Si VII 275.4
Fe XV 284.2
WARNING:
None
desc000378.txt
524474
1
0
Quiet Sun
Scanning
8158007
0
3
3
362
1
488
Equatorial/low-latitude coronal holes and associated solar wind, narrow raster
YKK_EqCHab_01N
000379 YKK_EqCHab_01N
Yuan-Kuen Ko
Science
16-Nov-2009
Study 000379:
ACRONYM: YKK_EqCHab_01N
This study is one of the two studies designed for measuring temperatures,
densities, and abundances in and at the boundary of equatorial, low-latitude
and polar coronal holes that may correspond to different footpoints of the
fast to slow solar wind.
To improve the signal in weak lines, 2 long exposures are taken at each
position in the raster.
TARGET: Coronal Hole
EXPOSURE TIME: 150s x 2 (2 exposures per raster position)
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 50"x400"
RASTER DURATION: 2h16m13s
COMPRESSION: DPCM
VOLUME: 65 Mbits
Pointing:
---------
Targets:
1) An equatorial or low-latitude coronal hole (within 40 degrees to the
solar equator)
2) Polar coronal hole can also be a candidate of study especially if it
extends to below 40 degrees in latitude.
Detailed pointing:
The raster field-of-view should at least cover the solar equator or
if the coronal hole does not reach latitude zero, the lowest latitude
that the coronal hole covers. The best time for observing is around its
passage across the central meridian. For a polar coronal hole without
low-latitude extension, point at the central meridian with
raster FOV covering partly the coronal hole, partly the quiet Sun.
Use/Instructions to planners:
-----------------------------
The objective of this study is the variation in physical
properties (temperature, density, abundances) along the LONGITUDINAL extent
of an equatorial, low-latitude or polar coronal hole that may correspond
to different footpoints of the fast to slow solar wind. Therefore the
longitudinal coverage is essential.
This raster is used in combination with another study YKK_EqCHab_01W to
complete a set of observations on the coronal hole and its EAST boundary. A
default set of study is as follows.
a) Run this study YKK_EqCHab_01N (twice), one near the center of the coronal
hole, the other in between the center and the EAST coronal hole boundary.
b) Run the study YKK_EqCHab_01W (once) at the EAST boundary of the
coronal hole, partly covering the 'visible' coronal hole, partly covering
the neighboring active region or quiet Sun at its east.
c) Follow step b) by one context raster study (PRY_slot_context_v3,
or PRY_slot_contextLITE if the available telemetry is tight) covering
the FOV of the above raster runs.
The two studies (YKK_EqCHab_01N and YKK_EqCHab_01W) can be used in
various combinations depending on the coronal hole size or planning
restrictions. At least three raster runs like the above default set on one
given coronal hole are requested in order to meet the objectives of the study.
If not possible, the priority is
1) East coronal hole boundary
2) In between the center and the EAST coronal hole boundary,
3) Center of the coronal hole.
The pointing of multi-raster runs should be made in a sequence toward the EAST
(i.e. from the center of the coronal hole toward its east boundary).
The FOV (relative to the CH) of the series of raster scans should not overlap.
Warning:
--------
None.
desc000379.txt
8195078
1
0
Coronal Hole
Scanning
66410040
0
2
2
363
1
50
Equatorial/low-latitude coronal holes and associated solar wind, wide raster
YKK_EqCHab_01W
000380 YKK_EqCHab_01W
Yuan-Kuen Ko
Science
16-Nov-2009
Study 000380:
ACRONYM: YKK_EqCHab_01W
This study is one of the two studies designed for measuring temperatures,
densities, and abundances in and at the boundary of equatorial,
low-latitude and polar coronal holes that may correspond to different
footpoints of the fast to slow solar wind.
To improve the signal in weak lines, 2 long exposures are taken at each
position in the raster.
TARGET: Coronal Hole
EXPOSURE TIME: 150s x 2 (2 exposures per raster position)
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 100"x400"
RASTER DURATION: 4h32m25s
COMPRESSION: DPCM
VOLUME: 130 Mbits
Pointing:
---------
Targets:
1) An equatorial or low-latitude coronal hole (within 40 degrees to the
solar equator)
2) Polar coronal hole can also be a candidate of study especially if
it extends to below 40 degrees in latitude.
Detailed pointing:
The raster field-of-view should at least cover the solar equator or,
if the coronal hole does not reach latitude zero, the lowest latitude
that the coronal hole covers. The best time for observing is around its
passage across the central meridian. For a polar coronal hole without
low-latitude extension, point at the central meridian with raster FOV
covering partly the coronal hole, partly the quiet Sun.
Use/Instructions to planners:
-----------------------------
The objective of this study is the variation in physical properties
(temperature, density, abundances) along the LONGITUDINAL extent of an
equatorial, low-latitude or polar coronal hole that may correspond to
different footpoints of the fast to slow solar wind. Therefore the
longitudinal coverage is essential.
This raster is used in combination with another study YKK_EqCHab_01N to
complete a set of observations on the coronal hole and its EAST boundary.
A default set of study is as follows.
a) Run the study YKK_EqCHab_01N (twice), one near the center of the
coronal hole, the other in between the center and the EAST coronal hole
boundary.
b) Run this study YKK_EqCHab_01W (once) at the EAST boundary of the
coronal hole, partly covering the 'visible' coronal hole, partly
covering the neighboring active region or quiet Sun at its east.
c) followed by one context raster study (PRY_slot_context_v3,
or PRY_slot_contextLITE if the available telemetry is tight)
covering the FOV of the above raster runs.
The two studies (YKK_EqCHab_01N and YKK_EqCHab_01W) can be used in
various combinations depending on the coronal hole size or planning
restrictions. At least three raster runs like the above default set
on one given coronal hole are requested in order to meet the objectives
of the study. If not possible, the priority is
1) East coronal hole boundary
2) In between the center and the EAST coronal hole boundary,
3) Center of the coronal hole.
The pointing of multi-raster runs should be made in a sequence toward
the EAST (i.e. from the center of the coronal hole toward its east boundary).
The FOV (relative to the CH) of the series of raster scans should not overlap.
Warning:
--------
None.
desc000380.txt
16367657
1
0
Coronal Hole
Scanning
132820080
0
2
2
364
1
100
Active region abundance variation study
YKK_ARabund01
000381 YKK_ARabund01
Yuan-Kuen Ko
Science
16-Nov-2009
Study 000381:
ACRONYM: YKK_ARabund01
The primary objective of this study is to measure the elemental abundance
in active regions. Especially, we target newly-formed active regions that
are within a few days old, and track their changes in physical properties,
especially in elemental abundance, with time.
TARGET: Active Region
EXPOSURE TIME: 45s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 3"
FOV: 194"x280"
RASTER DURATION: 53m19s
COMPRESSION: DPCM
VOLUME: 65 Mbits
Pointing:
---------
An active region that is within a few days old, the younger the better.
The raster field-of-view should cover the center of the active region.
Use/Instructions to planners:
-----------------------------
Once the target is identified, run this study twice a day
(separated by around 12 hours if possible) for 7 consecutive days
(or as many days as possible until the active region is behind the west limb,
or has decayed to no sunspot).
For **each raster run**, follow by one context raster study
(PRY_slot_context_v3, or PRY_slot_contextLITE if the available telemetry is
tight) covering the FOV of the above study.
Warning:
--------
None.
desc000381.txt
3221471
1
0
Active Region
Scanning
66281504
0
2
2
365
1
194
GDZ_AR_HOT_1_280X280_SLIT2_50S
GDZ_AR_HOT_1_280X280
000382 GDZ_AR_HOT_1_280X280
Giulio del Zanna
Science
25-Nov-2009
Study 000382:
ACRONYM: GDZ_AR_HOT_1_280X280
Perform a raster over an active region for cross-calibration
with XRT.
Scan a 280x280 area with the 2" slit and a sparse raster,
with long exposures (50s) and with all the brightest lines
formed at high temperatures, in particular Fe XVII.
TARGET : Active region at the limb.
EXPOSURE TIME : 50s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 4"
FOV : 280"x280"
DATA COMP. : DCPM
RASTER DURATON: 1h 3m
DATA volume : 108 Mbits
SPECTRAL WIN. : 22
LINES : Fe VIII, IX, X, XI, XII, XIII, XIV, XV ,XVI, XVII, XXIII
Ni XVII, O IV, V, VI, Mg VI, Si VII, Ca XIV, XV, XVI, XVII
POINTING:
---------
a quiescent active region observed at the solar limb.
INSTRUCTION TO PLANNERS:
------------------------
Make sure that the XRT images and the EIS rasters are taken
at the same time.
Study must be repeated at least 3 times.
Ideally, the study should be repeated twice. Once, when the
AR is visible on the disc, and once when it is slightly beyond the limb.
The study should also be repeated at the limb on the quiet Sun, with no
active regions present.
Fixed pointing is desirable.
WARNINGS:
---------
* The 50s exposure will likely saturate the srongest line.
* Preferably run during SAA-free time period.
desc000382.txt
3835046
1
0
Active Region
Scanning
114298106
0
2
2
366
1
278
Quiescent_filament_narrow
Quiet_fil_narrow
000383 Quiet_fil_narrow
Louise Harra
Science
25-Nov-2009
Study 000383:
ACRONYM: Quiet_fil_narrow
This study is for the small narrow filaments. This study should be
run for 24 hours
TARGET : Quiet Sun filament
EXPOSURE TIME : 60s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 10"
FOV : 102"x200"
DATA COMP. : JPEG95
RASTER DURATON: 12m 17s
DATA volume : 0.5 Mbits
SPECTRAL WIN. : 3
LINES : FeVIII 185.21, FeXII 195.12, HeII 256.3
Pointing:
---------
Pointing (when run as HOP 150):
Point at a short filament in the quiet Sun. Repeat the raster so that 1 day's
continuous data are taken at the same pointing. Hinode should track
the filament.
Points of contact for HOP 150:
Louise Harra (lkh[at]mssl.ucl.ac.uk) or
David Williams (drw[at]mssl.ucl.ac.uk) or
Len Culhane (Hinode contact; jlc[at]mssl.ucl.ac.uk)
Warning:
--------
Do not lower from the default compression quality if run for HOP 150.
desc000383.txt
621614
1
0
Quiet Sun
Scanning
508915
0
2
2
367
1
102
Quiescent_filament_wide
Quiet_fil_wide
000384 Quiet_fil_wide
Louise Harra
Science
25-Nov-2009
Study 000384:
ACRONYM: Quiet_fil_wide
Wider-FOV quiet Sun filament study (wider than study ID #383). For HOP 150,
this study should be run for 24 hours.
TARGET : Quiet Sun filament
EXPOSURE TIME : 60s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 20"
FOV : 202"x200"
DATA COMP. : JPEG95
RASTER DURATON: 12m 17s
DATA volume : 0.5 Mbits
SPECTRAL WIN. : 3
LINES : FeVIII 185.21, FeXII 195.12, HeII 256.3
POINTING:
---------
Centre the study on the middle of the filament where it is most likely
to erupt. Repeat the raster so that 1 day's continuous data are taken at
the same pointing. Hinode should track the filament.
Points of contact for HOP 150:
Louise Harra (lkh[at]mssl.ucl.ac.uk) or
David Williams (drw[at]mssl.ucl.ac.uk) or
Len Culhane (Hinode contact; jlc[at]mssl.ucl.ac.uk)
Warning:
--------
Do not lower from the default compression quality if run for HOP 150.
desc000384.txt
621614
1
0
Quiet Sun
Scanning
508915
0
2
2
368
1
202
Active_region_filament
AR_filament
000385 AR_filament
Louise Harra
Science
25-Nov-2009
Study 000385:
ACRONYM: AR_filament
Active region filament study designed to monitor changes in flows before
eruption. For HOP 150, this study should be run for 24 hours.
TARGET : Active Region filament
EXPOSURE TIME : 10s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 10"
FOV : 242"x200"
DATA COMP. : JPEG95
RASTER DURATON: 5m 11s
DATA volume : 2 Mbits
SPECTRAL WIN. : 5
LINES : FeVIII 185.21, FeXXIV 192.04, FeXII 195.12,
HeII 256.32, SiVII 275.35
Pointing:
---------
Pointing (when run as HOP 150):
Point at an active region filament. Repeat the raster so that 1 day's
continuous data are taken at the same pointing. Hinode should track
the filament.
Points of contact for HOP 150:
Louise Harra (lkh[at]mssl.ucl.ac.uk) or
David Williams (drw[at]mssl.ucl.ac.uk) or
Len Culhane (Hinode contact; jlc[at]mssl.ucl.ac.uk)
Warning:
--------
Do not lower the default compression quality if run for HOP 150.
desc000385.txt
334124
1
0
Active Region
Scanning
1927710
0
2
2
369
1
242
HH_Flare_180"x160"_5"steps_8sExp
HH_Flare_180x160_1
000386 HH_Flare_180x160_1
Hiro Hara
Science
15-Dec-2009
Study 000386:
ACRONYM:HH_Flare_180x160_1
This study is used to hunt for various flow structures in solar
flares. It can also be used for studies of the active regions.
Target: Active region
Type: scanning raster
Field of view: 180"x160"
Exposure time: 8s
Slit: 2"
step size: 5"
Raster Duration: 6m 13s
Data Volume: 4 Mbits
lines:
O VI: detection of TR response at the impulsive phase
Fe X: hunting of reconnection inflow
Fe XII: hunting of reconnection inflow
Fe XIV: study for normal coronal loops with density sensitive pairs
Fe XV : study of flare loops in a cooling phase
Fe XVI: study of flare loops in a cooling phase
Fe XVII: study of flare-loop heating and reconnection outflow
Fe XXIII: study of loop-top hot region and reconnection outflow
Fe XXIV: study of loop-top hot region and reconnection outflow
The non-thermal velocity component in solar flares is
studied by combinations of Fe XXIII and Fe XXIV.
Pointing:
---------
Active region including those with the potential for flaring
Instruction to planners:
------------------------
1) Centre the raster on an active region
2) When flare hunting, adjust the raster repeat for a maximum run-time
possible, accounting for the TM constraint.
Eg:
Raster repeat: 160
Run time: 16h 30m
Data volume: 782 Mbits (JPEG85)
Data Volume: 635 Mbits (JPEG75)
Note: When the telemetry is limited, change the compression parameter
from JPEG85 to JPEG75. If in doubt, consult:
hirohisa.hara[at]nao.ac.jp
WARNING:
--------
Do not adjust the data compression below JPEG75
desc000386.txt
395638
1
0
Active Region
Scanning
4699792
0
2
2
370
1
177
Five-arcsecond rapid scan for TR line assymetries
VHH_HI_BRT_SCAN
000387 VHH_HI_BRT_SCAN
Viggo Hansteen
Science
2-Feb-2010
Study 000387:
ACRONYM: VHH_HI_BRT_SCAN
This study is intended to be run on active region (or quiet sun) to look for
the time variations of spectral line assymetries.
The study consists of a single raster, with 5 contiguous positions
of EIS's narrow slit, making a narrow but tall scan with 60-second
exposures at each position. This scanning raster should be repeated 12 times
to make an approximately one-hour duration study.
Target: Active region or quiet sun
Type: scanning raster
Field of view: 5"x240"
Exposure time: 60s
Slit: 1"
step size: 1"
Raster Duration: 5m 47s
Data Volume: 3.8 Mbits
Instruction to planners:
-----------------------
Repeat the raster 12 times at least. Fill the TM slot available
It should be run, where possible, in co-ordinated observations with SOT.
The study is identical with DRW001_hi_brt_scan with the exception of the
line list which has been chosen to have as few blends as possible.
WARNING:
--------
None
desc000387.txt
347325
1
0
Active Region
Scanning
3470460
0
0
0
371
1
5
AR loop velocity study, 300"x512", 50s, 1"
PRY_loop_velocity
000388 PRY_loop_velocity
Peter Young
Science
2-Feb-2010
Study 000388:
ACRONYM: PRY_loop_velocity
Large raster covering 300" x 512" with a just a few iron
lines. Intended for measuring velocities in coronal loops.
Target: AR
Raster type: scanning
Duration: 4hr 32min
Slit: 1"
Pointing positions: 300, 1" step
Compression: JPEG95
Data volume: 99 Mbits
Exposure time: 50s
Pointing:
---------
The raster should be positioned so that quiet Sun is clearly visible
in some part of the raster.
WARNING:
--------
None
desc000388.txt
16361983
1
0
Active Region
Scanning
100672764
0
0
0
372
1
300
Calibration study for measuring slit tilts and widths
calib_slit_slot_v2
000389 calib_slit_slot_v2
Peter Young
Science
2-Feb-2010
Study 000389:
ACRONYM: calib_slit_slot_v2
**** CALIBRATION study, replacement for Study ID #352 ****
This study takes 3 small rasters using the 40", 1" and 2" slits (in
this order) to allow the intensity calibration for each to be
compared, and also to check the instrumental width of the 2" slit.
DURATION: 56 mins
VOLUME: 35 Mbits
Pointing:
--------
The study should be run in quiet Sun, either at disk center, or at the
limb.
Instruction to planners:
-----------------------
The CO should ensure that, when setting the pointing, the same
heliocentric coordinates are used for all three rasters
Warning:
-------
1 - Do not use within SAA
2 - Do not use within Eclipse passes
desc000389.txt
3303343
3
0
Quiet Sun
Scanning
35448050
2
3
2
335
1
104
373
1
15
374
1
30
HH_Flare_180"x160"_5"steps_8sExp_v2
HH_Flare_180x160_v2
000390 HH_Flare_180x160_v2
Hiro Hara
Science
2-Feb-2010
Study 000390:
ACRONYM:HH_Flare_180x160_v2
This study is used to hunt for various flow structures in solar
flares. It can also be used for studies of the active regions.
Target: Active region / Flare
Type: scanning raster
Field of view: 180"x160"
Exposure time: 8s
Slit: 2"
step size: 5"
Raster Duration: 6m 36s
Data Volume: 4.7 Mbits
lines:
O VI: detection of TR response at the impulsive phase
Fe X: hunting of reconnection inflow
Fe XII: hunting of reconnection inflow
Fe XIV: study for normal coronal loops with density sensitive pairs
Fe XV : study of flare loops in a cooling phase
Fe XVI: study of flare loops in a cooling phase
Fe XVII: study of flare-loop heating and reconnection outflow
Fe XXIII: study of loop-top hot region and reconnection outflow
Fe XXIV: study of loop-top hot region and reconnection outflow
The non-thermal velocity component in solar flares is
studied by combinations of Fe XXIII and Fe XXIV.
Pointing:
---------
Active region including those with the potential for flaring
Instruction to planners:
------------------------
1) Centre the raster on an active region
2) When flare hunting, adjust the raster repeat for a maximum run-time
possible, accounting for the TM constraint.
Eg:
Raster repeat: 160
Run time: 16h 30m
Data volume: 757 Mbits (JPEG85)
Data Volume: 633 Mbits (JPEG75)
Note: When the telemetry is limited, change the compression parameter
from JPEG85 to JPEG75. If in doubt, consult:
hirohisa.hara[at]nao.ac.jp
WARNING:
--------
Do not adjust the data compression below JPEG75
desc000390.txt
395638
1
0
Flare
Scanning
4846661
0
2
2
375
1
177
Coronal Hole study: JS_CH_400x256_2arc, XFOV = 400arc, exp. time = 160s
JS_CH_400x256_V4
000391 JS_CH_400x256_V4
Jian Sun
Science
2-Feb-2010
Study 000391:
Acronym: JS_CH_400x256_V4
Coronal Hole study, 160s exposure time version.
Modified version of study #368 (120s to 160s exposure time to increase DN/pixel
and the number of pointing positions from 140 to 200).
Summary:
-------
2"slit scan, 200 pointing positions (FOV = 400"x256"), 160s exp. time.
DCPM compression is used to get good line profile.
TARGET: Coronal Hole
Duration: 9h 26m
Volume: 139 Mbits
Pointing:
---------
The target of this study is a polar coronal hole. EIS should be pointed
to include the boundary of the coronal hole and the limb. The purpose
is to obtain velocity maps of million degree plasma.
Instruction to planners:
-----------------------
1. It would be better to run REGCAL 071 & 072 studies prior to run this study.
*** Run REGCAL 071 & 072 only ONCE prior to multiple JS_CH run(s), per
day. I.e do not run the regcals more than once per 24h ***
2. Ideally this study should run repeatedly (fill the time slot available).
WARNING:
-------
None
desc000391.txt
34015489
1
0
Coronal Hole
Scanning
142588783
0
2
2
376
1
400
Sit-and-stare study for measuring nanoflare signature
nanoflare_sas_v1
000392 nanoflare_sas_v1
Peter Young
Science
2-Mar-2010
Study 000392:
ACRONYM: nanoflare_sas_v1
Sit-and-stare study with 30 sets of (5s and 50s) exposures. Intended to
search for the signatures of nanoflares through blue wing enhancements
on hot emission lines.
Duration: 31min
Compression: DPCM
Data volume: 83 Mbits
Exposure time: 5s + 50s
Slit: 2"
Pointing:
---------
Pointing should be above moss regions within the core of an active region.
Instruction to planners:
------------------------
1) Run context raster PRY_slot_contest_v3 or PRY_slot_contextLITE
(depending on the TM availability)
2) Run this study to fill the available time-slot.
Warning:
--------
None
desc000392.txt
1883719
1
0
Active Region
Scanning
84447864
0
2
2
377
1
2
Alignment_Modify_40slot_1slit_v2
Alignment_modify_v2
000393 Alignment_modify_v2
Shin Imada
Science
2-Mar-2010
Study 000393:
ACRONYM: alignment_modified_v2
Alignment study for North Pole or East limb using 1"slit and 40"slot
**************************************************************************
* This is an alignment study. Please follow the "instruction to planner" *
* section in details *
* *
* Please email imada.shinsuke@jaxa.jp before using this study. *
* Coordination with SOT and XRT is needed. *
**************************************************************************
Study summary:
-------------
2 Rasters study
slit: 1" and 40"
S/C pointing: North Pole or East limb
window height: 512"
exposure time: 60s and 30s
# of pointing: 1 and 3
step size: SNS and 20"
duration: 14m28s
Lines: FeXI (180.47), FeXII(195.12), HeII (256.35), SiX(272.01), FeXV(284.16).
Pointing:
---------
This study is designed to observe the solar limb.
Target will be the north pole or east limb.
This study is relatively sensitive to the Hinode pointing.
Instruction to planner:
-----------------------
1) Place the study on the timeline and point (both) rasters
2) Advance the Cursor Time by 30s (leave a gab)
3) Copy the study to the cursor position (Study -> Select (single) entry ->
Copy to Cursor time)
4) Repeat steps 2 & 3 until 7 study runs (IN TOTAL) are placed
on the timeline.
Total run time is approximately 1h46m
Warning:
--------
None
desc000393.txt
868545
2
0
Quiet Sun
Scanning
2708384
1
0
3
378
1
1
379
4
80
Magnetoseismology pof bright points 3
mbps_3
000394 mbps_3
R. Erdelyi
Science
2-Mar-2010
Study 000394:
Acronym: mbps_3
HOP152: Observations of magnetic bright points (MBPs) and pores.
The primary objective of this HOP is clarifying the degree of magnetic wave
coupling from the photosphere to corona, topological 3D magnetic connectivity
and the efficiency of wave energy dissipation.
Pointing:
---------
MBP on 1st 6 days (Quiet Sun).
AR pore or similar structure (small sunspot) on remaining 4 days.
Pointing information for HOP152 will be provided by
Robertus Erdelyi <robertus [at] sheffield.ac.uk> at Sac Peak
or
Mihalis Mathioudakis <M.Mathioudakis [@] qub.ac.uk>, tel.: +44-(0)28-90973573
Use/Instructions to planners:
-----------------------------
Requested observation of an MBP in a Quiet Sun region for the first 6 days
and a pore or a similar structure (small sunspot) for the remaining 4 days.
The studies should be run from 15:00 UT for around 3 hours on 8-17 March 2010.
The observing sequence is the following:
***** 1st 6 days (8-13 March 2009), Quiet Sun *****
1) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
2) Run mbps_1 for approx 1.5 hours
3) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
4) Run mbps_2qs for about 1.5 hours
5) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
***** 2nd 4 days (14-17 March 2009), Active Region *****
1) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
2) Run mbps_1 for approx 1.5 hours
3) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
4) Run mbps_2ar for about 1.5 hours
5) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
Warning:
--------
Do not run within SAAs
desc000394.txt
711448
1
0
Quiet Sun
Scanning
2725011
0
2
2
380
1
60
Magnetoseismology of bright points 2 (quiet sun)
mbps_2qs
000395 mbps_2qs
R. Erdelyi
Science
2-Mar-2010
Study 000395:
Acronym: mbps_2qs
HOP152: Observations of magnetic bright points (MBPs) and pores.
The primary objective of this HOP is clarifying the degree of magnetic wave
coupling from the photosphere to corona, topological 3D magnetic connectivity
and the efficiency of wave energy dissipation.
Pointing:
---------
MBP on 1st 6 days (Quiet Sun).
AR pore or similar structure (small sunspot) on remaining 4 days.
Pointing information for HOP152 will be provided by
Robertus Erdelyi <robertus [at] sheffield.ac.uk> at Sac Peak
or
Mihalis Mathioudakis <M.Mathioudakis [@] qub.ac.uk>, tel.: +44-(0)28-90973573
Use/Instructions to planners:
-----------------------------
Requested observation of an MBP in a Quiet Sun region for the first 6 days
and a pore or a similar structure (small sunspot) for the remaining 4 days.
The studies should be run from 15:00 UT for around 3 hours on 8-17 March 2010.
The observing sequence is the following:
***** 1st 6 days (8-13 March 2009), Quiet Sun *****
1) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
2) Run mbps_1 for approx 1.5 hours
3) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
4) Run mbps_2qs for about 1.5 hours
5) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
***** 2nd 4 days (14-17 March 2009), Active Region *****
1) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
2) Run mbps_1 for approx 1.5 hours
3) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
4) Run mbps_2ar for about 1.5 hours
5) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
Warning:
-------
Do not run within SAAs
desc000395.txt
521100
1
0
Quiet Sun
Scanning
6094650
0
0
0
381
10
4
Magnetoseismology of bright points 2 (active region)
mbps_2ar
000396 mbps_2ar
R. Erdelyi
Science
2-Mar-2010
Study 000396:
Acronym: mbps_2ar
HOP152: Observations of magnetic bright points (MBPs) and pores.
The primary objective of this HOP is clarifying the degree of magnetic wave
coupling from the photosphere to corona, topological 3D magnetic connectivity
and the efficiency of wave energy dissipation.
Pointing:
---------
MBP on 1st 6 days (Quiet Sun).
AR pore or similar structure (small sunspot) on remaining 4 days.
Pointing information for HOP152 will be provided by
Robertus Erdelyi <robertus [at] sheffield.ac.uk> at Sac Peak
or
Mihalis Mathioudakis <M.Mathioudakis [@] qub.ac.uk>, tel.: +44-(0)28-90973573
Use/Instructions to planners:
-----------------------------
Requested observation of an MBP in a Quiet Sun region for the first 6 days
and a pore or a similar structure (small sunspot) for the remaining 4 days.
The studies should be run from 15:00 UT for around 3 hours on 8-17 March 2010.
The observing sequence is the following:
***** 1st 6 days (8-13 March 2009), Quiet Sun *****
1) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
2) Run mbps_1 for approx 1.5 hours
3) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
4) Run mbps_2qs for about 1.5 hours
5) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
***** 2nd 4 days (14-17 March 2009), Active Region *****
1) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
2) Run mbps_1 for approx 1.5 hours
3) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
4) Run mbps_2ar for about 1.5 hours
5) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
Warning:
-------
Do not run within SAAs
desc000396.txt
527550
1
0
Active Region
Scanning
6563460
0
0
0
382
10
7
Magnetoseismology of bright points
mbps_1
000397 mbps_1
R. Erdelyi
Science
2-Mar-2010
Study 000397:
Acronym: mbps_1
HOP152: Observations of magnetic bright points (MBPs) and pores.
The primary objective of this HOP is clarifying the degree of magnetic wave
coupling from the photosphere to corona, topological 3D magnetic connectivity
and the efficiency of wave energy dissipation.
Pointing:
---------
MBP on 1st 6 days (Quiet Sun).
AR pore or similar structure (small sunspot) on remaining 4 days.
Pointing information for HOP152 will be provided by
Robertus Erdelyi <robertus [at] sheffield.ac.uk> at Sac Peak
or
Mihalis Mathioudakis <M.Mathioudakis [@] qub.ac.uk>, tel.: +44-(0)28-90973573
Use/Instructions to planners:
-----------------------------
Requested observation of an MBP in a Quiet Sun region for the first 6 days
and a pore or a similar structure (small sunspot) for the remaining 4 days.
The studies should be run from 15:00 UT for around 3 hours on 8-17 March 2010.
The observing sequence is the following:
***** 1st 6 days (8-13 March 2009), Quiet Sun *****
1) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
2) Run mbps_1 for approx 1.5 hours
3) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
4) Run mbps_2qs for about 1.5 hours
5) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
***** 2nd 4 days (14-17 March 2009), Active Region *****
1) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
2) Run mbps_1 for approx 1.5 hours
3) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
4) Run mbps_2ar for about 1.5 hours
5) Run mbps_3 (context raster for about 5 mins) with 29 step x 2 arcsec scan
for context image purposes.
Warning:
--------
Do not run within SAAs
desc000397.txt
521100
1
0
Quiet Sun
Scanning
3750550
0
2
2
383
10
8
Hot_loop_oscillations_at_limb
Hot_loop_osci_1
000398 Hot_loop_osci_1
Tongjiang Wang
Science
16-Mar-2010
Study 000398:
ACRONYM: Hot_loop_osci_1
This study is for hot loop oscillations at limb
TARGET Active Region
RASTER TYPE: SCANNING
NO. OF POINTING POSITIONS: 9
SLIT/SLOT: 2"
SCAN STEP SIZE (arcsec): 2
EXPOSURE TIMES (ms): 5000
NO. OF WINDOWS: 6
WINDOW WIDTHS (pixels): 24,24,24,24,24,32
WINDOW HEIGHT (pixels): 112
Line List:
Line Wavelength
Ca XV 181.90
Fe XII 195.12
Ca XV 200.98
He II 256.32
Fe XVI 262.98
Fe XXIII 263.76
WARNING:
None
desc000398.txt
94649
1
0
Active Region
Scanning
664351
0
2
2
384
1
20
Hot_loop_oscillations_at_limb_2
Hot_loop_osci_2
000399 Hot_loop_osci_2
Tongjiang Wang
Science
16-Mar-2010
Study 000399:
ACRONYM: Hot_loop_osci_2
This study is for hot loop oscillations at limb
TARGET: Active Region
RASTER TYPE: SCANNING
NO. OF POINTING POSITIONS: 5
SCAN STEP SIZE (arcsec): 2
NO. OF WINDOWS: 8
WINDOW WIDTHS (pixels): 24,24,24,24,24,24,32,24
WINDOW HEIGHT (pixels): 112
SLIT/SLOT: 2"
EXPOSURE TIMES (ms): 10000
Line List:
Line Wavelength (Angstroms)
Ca XV 181.90
Ca XVII 192.85
Fe XII 195.12
Ca XV 200.98
He II 256.32
Fe XVI 262.98
Fe XXIII 263.76
Fe XVII 269.42
WARNING:
None
desc000399.txt
97290
1
0
Active Region
Scanning
524487
0
2
2
385
1
12
Active_region_raster_new
arm_raster_ar
000400 arm_raster_ar
Dipankar Banerjee
Science
8-Apr-2010
Study 000400:
ACRONYM: arm_raster_ar
This is context raster for HOP 156 studies. Line list is chosen such
that we can produce a density map also. Therefor, DPCM compression is chosen
to get good line profiles. This raster is part of the study # 174
arm_fastslot_waves.
TARGET : Active region.
EXPOSURE TIME : 25s
RASTER TYPE : Scanning
SLIT : 2"
STEP_SIZE : 2"
FOV : 82"x400"
DATA COMP. : DPCM
RASTER DURATON: 20m
DATA volume : 61 Mbits
LINES : Fe X, XII, XIII, XV, He II, Mg VI, Si VII, Ca XVII
POINTING:
---------
Active region on disk showing many distinct loops. If the loops are
just off-limb they could also be considered.
INSTRUCTION TO PLANNERS:
------------------------
For HOP 156 the studies should be run in the following order.
* Run arm_raster_ar (context raster)
* Run arm_fastslot_v2 (slot sit'n'stare)
* Run High_cadence_AR_dens (slit sit'n'stare). This study should be
repeated 3 times at 3 different locations (loop top & foot point are must)
on a well defined loop within the slot.
WARNINGS:
---------
* Run preferably during SAA-free time period.
desc000400.txt
1179313
1
0
Active Region
Scanning
61482843
0
2
2
143
1
82
fast slot for high frequency oscillations
arm_fastslot_v2
000401 arm_fastslot_v2
Dipankar Banerjee
Science
8-Apr-2010
Study 000401:
ACRONYM: arm_fastslot_v2
This study is slightly modified version of raster 'arm_fastslot' which
is part of arm_fastslot_waves (study # 174). Mainly for high frequency
oscillation study. Modifications are done to suit current data rates
and volume.
Modifications: No. of pointings reduced from 1000 to 150, exposure times
are doubled, and Fe XIII 202.04 line is added to the line list.
TARGET : Active region.
EXPOSURE TIME : 4s
RASTER TYPE : Sit'n'Stare
SLOT : 40"
# of pointings: 150
DATA COMP. : JPEG98
RASTER DURATON: 16m
DATA volume : 85 Mbits
LINES : Fe X, XII, XIII, XV, He II, Si VII, Ca XVII
POINTING:
---------
Active region on disk showing many distinct loops. if the loops
are just off-limb they could also be considered. Keep the position of
slot such that it covers a set of loops inside the contex raster completely.
INSTRUCTION TO PLANNERS:
------------------------
For HOP 156 the studies should be run in the following order.
* Run arm_raster_ar (context raster)
* Run arm_fastslot_v2 (slot sit'n'stare)
* Run High_cadence_AR_dens (slit sit'n'stare). This study should be repeated
3 times at 3 different locations (loop top & foot point are must) on a well
defined loop within the slot.
WARNINGS:
---------
* Run preferably during SAA-free time period.
* The data rates are slightly higher (~90 Kbps)
desc000401.txt
947242
1
0
Active Region
Scanning
86540487
0
3
3
386
1
40
Active region high cadence study
High_cadence_AR_dens
000402 High_cadence_AR_dens
Dipankar Banerjee
Science
8-Apr-2010
Study 000402:
ACRONYM: High_cadence_AR_dens
This is sit'n'stare observation using 1" slit. This can be used for high
frequency oscillation studies and loop diagnostics. DPCM is requested to
ensure good line profiles.
TARGET : Active region.
EXPOSURE TIME : 5s
RASTER TYPE : Sit'n'Stare
SLIT : 1"
# of pointings: 100
DATA COMP. : DPCM
RASTER DURATON: 13m
DATA volume : 32 Mbits
LINES : Fe XII, XIII, He II, Ca XVII
POINTING:
---------
For HOP156 slit should be positioned at a min. of 3 different locations
(loop top & foot point are must) on a well defined loop inside the region
covered by 40" slot.
INSTRUCTION TO PLANNERS:
------------------------
For HOP 156 the studies should be run in the following order.
* Run arm_raster_ar (context raster)
* Run arm_fastslot_v2 (slot sit'n'stare)
* Run High_cadence_AR_dens (slit sit'n'stare). This study should be
repeated 3 times at 3 different locations(loop top & foot point are must)
on a well defined loop within the slot.
WARNINGS:
---------
* Run preferably during SAA-free time period.
desc000402.txt
743994
1
0
Active Region
Scanning
32562342
0
0
0
45
1
1
Spectral atlas covering 120x160 with 2" slit - 30s exposures
Atlas_30
000403 Atlas_30
Peter Young
Science
28-Apr-2010
Study 000403:
ACRONYM: Atlas_30
Raster that covers 120" x 160" with the 2" slit and takes the complete
EIS spectrum. This version uses 30s exposure times.
Duration: 33min 50s
Compression: DPCM
Data volume: 257 Mbit
Exposure time: 30s
Slit: 2"
Pointing:
--------
The study is intended to be run regularly as part of the EIS synoptic
program to obtain reference spectra for active regions, quiet Sun and
coronal holes both on-disk and off-limb.
Intruction to planners:
----------------------
It is recommended that the slot context study PRY_slot_context_v3 be
run beforehand to provide context.
Warning:
-------
High data rate (126 kbits/s) but the overall data volume is OK (257 Mbits)
desc000403.txt
2030397
1
0
Quiet Sun
Scanning
263240831
0
2
2
387
1
120
Spectral atlas covering 120x160 with 2" slit - 60s exposures
Atlas_60
000404 Atlas_60
Peter Young
Science
28-Apr-2010
Study 000404:
ACRONYM: Atlas_60
Raster that covers 120" x 160" with the 2" slit and takes the complete
EIS spectrum. This version uses 60s exposure times.
Duration: 1h 5m
Compression: DPCM
Data volume: 257 Mbit
Exposure time: 60s
Slit: 2"
Pointing:
--------
The study is intended to be run regularly as part of the EIS synoptic
program to obtain reference spectra for active regions, quiet Sun and
coronal holes both on-disk and off-limb.
Intruction to planners:
----------------------
It is recommended that the slot context study PRY_slot_context_v3 be
run beforehand to provide context.
Warning:
-------
High data rate (65 kbits/s) but the overall data volume is OK (257 Mbits)
desc000404.txt
3920397
1
0
Quiet Sun
Scanning
263240831
0
2
2
388
1
120
Spectral atlas covering 120x160 with 2" slit - 120s exposures
Atlas_120
000405 Atlas_120
Peter Young
Science
28-Apr-2010
Study 000405:
ACRONYM: Atlas_120
Raster that covers 120" x 160" with the 2" slit and takes the complete
EIS spectrum. This version uses 120s exposure times.
Duration: 2h 8m
Compression: DPCM
Data volume: 257 Mbit
Exposure time: 120s
Slit: 2"
Pointing:
--------
The study is intended to be run regularly as part of the EIS synoptic
program to obtain reference spectra for active regions, quiet Sun and
coronal holes both on-disk and off-limb.
Intruction to planners:
----------------------
It is recommended that the slot context study PRY_slot_context_v3 be
run beforehand to provide context.
Warning:
-------
None
desc000405.txt
7700397
1
0
Quiet Sun
Scanning
263240831
0
2
2
389
1
120
Engineering sequence which delays for 1 minute
delay60
000406 delay60
Khalid al Janabi
Engineering
Study 000406:
ACRONYM: delay60
An engineering sequence (dummy study) that delays for 1 minute. It uses
an ICU internal clock and delays for 1 minute with 1 second accuracy or
better. No TM is generated. It's intended to be used for bridging
chained studies
Warning:
-------
None
desc000406.txt
60001
0
0
Engineering
SnS
0
0
0
0
Engineering sequence which delays for 5 minutes
delay300
000407 delay300
Khalid al Janabi
Engineering
Study 000407:
ACRONYM: delay300
An engineering sequence (dummy study) that delays for 5 minutes. It uses
an ICU internal clock and delays for 5 minute with 1 second accuracy or
better. No TM is generated. It's intended to be used for bridging
chained studies.
Warning:
-------
None
desc000407.txt
300001
0
0
Engineering
SnS
0
0
0
0
Engineering sequence which delays for 10 minutes
delay600
000408 delay600
Khalid al Janabi
Engineering
Study 000408:
ACRONYM: delay600
An engineering sequence (dummy study) that delays for 10 minutes. It uses
an ICU internal clock and delays for 10 minutes with 1 second accuracy or
better. No TM is generated. It's intended to be used for bridging
chained studies
Warning:
-------
None
desc000408.txt
600001
0
0
Engineering
SnS
0
0
0
0
Engineering sequence which delays for 20 minutes
delay1200
000409 delay1200
Khalid al Janabi
Engineering
Study 000409:
ACRONYM: delay1200
An engineering sequence (dummy study) that delays for 20 minutes. It uses
an ICU internal clock and delays for 10 minutes with 1 second accuracy or
better. No TM is generated. It's intended to be used for bridging
chained studies
Warning:
-------
None
desc000409.txt
1200001
0
0
Engineering
SnS
0
0
0
0
Engineering sequence which delays for 30 minutes
delay1800
000410 delay1800
Khalid al Janabi
Engineering
Study 000410:
ACRONYM: delay1800
An engineering sequence (dummy study) that delays for 30 minutes. It uses
an ICU internal clock and delays for 10 minutes with 1 second accuracy or
better. No TM is generated. It's intended to be used for bridging
chained studies
Warning:
-------
None
desc000410.txt
1800001
0
0
Engineering
SnS
0
0
0
0
Engineering sequence which delays for 40 minutes
delay2400
000411 delay2400
Khalid al Janabi
Engineering
Study 000411:
ACRONYM: delay2400
An engineering sequence (dummy study) that delays for 40 minutes. It uses
an ICU internal clock and delays for 40 minutes with 1 second accuracy or
better. No TM is generated. It's intended to be used for bridging
chained studies
Warning:
-------
None
desc000411.txt
2400001
0
0
Engineering
SnS
0
0
0
0
YLin et al.: for HOP158 multiple-line observations of solar FL&AR (sit&stare part) - V2
YL_FL0158_V2
000412 YL_FL0158_V2
Tetsuya Watanabe
Science
11-May-2010
Study 000412:
ACRONYM: YL_FL0158_V2
This sit&stare observation is designed to follow EIS
study ID: 390 - HH_Flare_180x160_V2 (HH_Flare_180"x160"_5"steps_8sExp_v2)
scanning several times over an active region (or flare region).
TARGET : AR & FL
EXPOSURE TIME : 10s
SLIT : 2"
FOV : 2" x 160"
TOTAL TIME : 37m46s
Volume : 33 Mbits
DC : USES JPEG 85 COMPRESSION.
WINDOWS : 15
LINES : Fe XXIV 192.03
Fe XXIII 263.76
Ca XVII 192.82
Fe XVII 254.87
Fe XVI 262.98
Fe XV 264.16
Fe XIV 274.20/264.79
Fe XIII 202.02
Fe XII 195.12
Fe XI 182.16
Fe X 184.54
Fe VIII 185.21
Si VII 275.35
Mg VI 268.99
He II 256.32
Pointing:
--------
Highest priority: to observe the flares near the disk center,
and the flare impulsive phase.
Warning:
-------
None
desc000412.txt
2266190
1
0
Active Region
Scanning
33779761
0
2
2
390
1
2
HPW020_VEL_FULLs1
HPW020_VEL_FULLs1
000413 HPW020_VEL_FULLs1
Harry Warren
Science
11-May-2010
Study 000413:
ACRONYM: HPW020_VEL_FULLs1
This study is designed to take the full wavelength range and slit height.
The primary purpose is to accumulate data for checking the relative
wavelengths of emission lines above the limb and in the quiet Sun on the
disk and so the exposure times are very long (120s). It may also be possible
to use this study in an active region to check for the
presence of very high temperature emission at low emission measure.
This is likely to saturate the strongest lines, however.
The data rate for this study is very high and it cannot be run for very long.
TARGET: Quiet Sun
EXPOSURE TIME: 120s
RASTER: Sit-and-Stare
SLIT: 1"
FOV: 1"x400"
RASTER DURATION: 44m47s
VOLUME: 243 Mbits
RATE: 90 kbits/s
COMPRESSION: JPEG95
Pointing:
---------
Quiet Sun above the limb or disk-center quiet Sun.
Warning:
--------
1) DO NOT RUN DURING SAA OR ECLIPSE!
2) High data rate (90 kbits/s) and volume (243 Mbits), hence
it cannot be run for very long.
desc000413.txt
2709764
1
0
Quiet Sun
Scanning
248113761
0
0
0
391
1
1
GDZ_300x360_S2S3_30S
GDZ_300x360_S2S3_30S
000414 GDZ_300x360_S2S3_30S
Giulio del Zanna
Science
26-May-2010
Study 000414:
ACRONYM: GDZ_300x360_S2S3_30S
Perform a large (300x260) sparse (3") raster over an active region
with the 2" slit and long exposures (30s).
TARGET : Active region
EXPOSURE TIME : 30s
RASTER : Scanning
SLIT : 2"
STEP_SIZE : 3"
FOV : 300"x260"
SPECTRAL WIND.: 20
DATA COMP. : DCPM
RASTER DURATON: 56m
DATA volume : 99 Mbits (29 kBits/s)
LINES : Fe VIII, IX, X,XI,XII,XIII,XIV,XVI,XVII, XXIII, XXIV
O V, Mg VI, Si VI, VII, Ca XIV, XVII
POINTING:
--------
a quiescent active region observed across the disk.
INSTRUCTION TO PLANNERS:
-----------------------
It is important to coordinate with CDS planners so that the study
ARCONT (ID 11, VAR 105) containing the Fe XIX and Ne VI lines is run.
Warning:
-------
None
desc000414.txt
3402459
1
0
Active Region
Scanning
157862235
0
2
2
392
1
302
js2_40slot_decon_v1
js2_40slot_decon_v1
000415 js2_40slot_decon_v1
Jian Sun
Calibration
26-May-2010
Study 000415:
ACRONYM: js2_40slot_decon_v1
This is a Calibration study which consists of two rasters:
Raster 1: js2_1slit_scan_v1 (context)
Raster 2: js2_40slot_scan_v1
TARGET : Active region.
EXPOSURE TIME : 10s
RASTER TYPE : Scan
SLOT : 1" & 40"
# of pointings: 339 & 10"
DATA COMP. : DPCM
RASTER DURATON: 1h33m53s
DATA volume : 381 Mbits
LINES : Fe XII, XIV, XXIV, He II
POINTING:
---------
Simple configuration Active region is prefered. The scan FOV is better to cover
the edge of active region, where possible outflow is expected.
both raster should use *the same pointings*
INSTRUCTION TO PLANNERS:
------------------------
This study includes two rasters: js2_1slit_scan_v1 and js2_40slot_scan_v1
* First raster: js2_1slit_scan_v1
* Second raster: js2_40slot_scan_v1. Repeatable for (10 to 20 times)
* both raster should use *the same pointings* (ie. same FOV)
WARNINGS:
---------
* Run preferably during SAA-free period.
desc000415.txt
5633221
2
0
Active Region
Scanning
391061125
1
0
3
393
1
340
394
10
340
NNK_SNS_WAVE_PROP_v1 [EWxNS = 2"x296"; nstep: 3 (30")] Wave propagation in AR
NNK_SNS_WAVE_PROP_v1
000416 NNK_SNS_WAVE_PROP_v1
Unknown
Science
26-May-2010
Study 000416:
ACRONYM: NNK_SNS_WAVE_PROP_v1
This study is intended to be run in active regions to search
the signatures of wave propagation and dissipation along coronal structures
at temperature around 1-2MK. Different from previous rasters, the slit are
pointed at three locations in order (a, b, c, a, b, c,...),
which enables us to investigate the evolution of waves passing the
observed location.
TARGET: Active Region
EXPOSURE TIME: 20s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 30"
FOV: 62"x296"
RASTER DURATION: 60m 9s
DATA VOLUME: 68 Mbits
2) Pointing
-----------
- Fan-like loops (open field)
- or usual AR loops (close field)
3) Use/Instructions to planners
------------------------------
- Run ACRONYM: PRY_slot_context_v2 (ID: 249) as a context study
- Run NNK_SNS_WAVE_PROP_v1 consecutively.
Recommended 3 times repeat or fill the available time slot.
- Run PRY_slot_context_v2.
4) WARNING
----------
- If possible, please run this study in the period 10-15UT (SAA free period).
- Do not start the context raster within SAA
desc000416.txt
4156200
1
0
Active Region
Scanning
64836480
0
2
2
395
60
62
Hot_loop_oscillations_at_limb_v2
Hot_loop_osci_1_v2
000417 Hot_loop_osci_1_v2
Tongjiang Wang
Science
26-May-2010
Study 000417:
ACRONYM: Hot_loop_osci_1_v2 (modified version for study ID=398)
Note: This observation requires running three studies:
ACRONYM: PRY_slot_contextLITE (study ID=354)
ACRONYM: Hot_loop_osci_1_v2 (modified version for study ID=398)
ACRONYM: Hot_loop_osci_2_v2 (modified version for study ID=399)
This study is designed to detect Doppler shifts and intensity variations
mainly in hot coronal and flare emission lines.
The observation consists of three studies. Study A is
using slot-40 to quickly scan whole AR for obtaining a context image.
Studies B and C are using the repeated short raster in high cadence (<2 min)
to search for flare-excited oscillations in hot coronal loops, such as
standing slow mode waves as observed by SUMER. It also includes a pair of
density sensitive Ca XV lines for density diagnostics. The study is
designed to detect oscillations and waves in coronal loops of T =1-10 MK.
#Study A: Context study
ACRONYM: PRY_slot_contextLITE
TARGET: AR loops on the limb
EXPOSURE TIME: 10 s
RASTER: Scanning
SLOT: 40"
STEP SIZE: 32"
FOV: 488"x488"
RASTER DURATION: 3m29s
REPEAT TIMES: 1
#Study B:
ACRONYM: Hot_loop_osci_1_v2
TARGET: AR loops on the limb
EXPOSURE TIME: 5 s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 20"x112"
RASTER DURATION: 1m35s
REPEAT TIMES: 1
N_LINES 6
Ca XV, Ca XVII, Fe XII, Ca XV, Fe XVI and Fe XXIII
#Study C:
ACRONYM: Hot_loop_osci_2_v2
TARGET: AR loops on the limb
EXPOSURE TIME: 10 s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 12"x112"
RASTER DURATION: 1m37s
REPEAT TIMES: 1
N_LINES 8
Ca XV, Ca XVII, Ca XIV, Fe XII, Ca XV, Fe XVI, Fe XXIII and Fe XVII
Pointing:
--------
Flare-productive active region on the limb, better located at the eastern limb.
For Study A, the 1/3 FOV is on the disk and 2/3 FOV off the limb.
For Studies B and and C the slit center position is set about 30-50 arcsec
above the AR on the limb (close to the core of the AR)
Use/Instructions to planners:
-----------------------------
i) Run Study A (ID=354) first to get a context image of AR.
ii) Repeat Study B (Hot_loop_osci_1) for about 5 hours, and then
run Study A again for a context image.
iii) Repeat Study C (Hot_loop_osci_2) for about 5 hours, and then
run Study A again.
iv) Stop or repeat ii) and iii) once more if possible.
Note: The above 10 hrs observations are better not interrupted.
We hope to make observations of at least 10 hrs every day
(better 20 hrs/day if allowed), and last for 4-5 days so we can track
the AR passing from behind the limb to the front
disk to catch loops of different sizes and different parts of loops
during this period.
Warning:
--------
The squence above should be run uninterrupted (preferably use chained studies),
i.e.(append to hilighted entry).
desc000417.txt
94649
1
0
Active Region
Scanning
664351
0
2
2
396
1
20
Hot_loop_oscillations_at_limb_2_v2
Hot_loop_osci_2_v2
000418 Hot_loop_osci_2_v2
Tongjiang Wang
Science
26-May-2010
Study 000418:
ACRONYM: Hot_loop_osci_2_v2 (modified version for study ID=399)
Note: This observation requires running three studies:
ACRONYM: PRY_slot_contextLITE (study ID=354)
ACRONYM: Hot_loop_osci_1_v2 (modified version for study ID=398)
ACRONYM: Hot_loop_osci_2_v2 (modified version for study ID=399)
This study is designed to detect Doppler shifts and intensity variations
mainly in hot coronal and flare emission lines.
The observation consists of three studies. Study A is
using slot-40 to quickly scan whole AR for obtaining a context image.
Studies B and C are using the repeated short raster in high cadence (<2 min)
to search for flare-excited oscillations in hot coronal loops, such as
standing slow mode waves as observed by SUMER. It also includes a pair of
density sensitive Ca XV lines for density diagnostics. The study is
designed to detect oscillations and waves in coronal loops of T =1-10 MK.
#Study A: Context study
ACRONYM: PRY_slot_contextLITE
TARGET: AR loops on the limb
EXPOSURE TIME: 10 s
RASTER: Scanning
SLOT: 40"
STEP SIZE: 32"
FOV: 488"x488"
RASTER DURATION: 3m29s
REPEAT TIMES: 1
#Study B:
ACRONYM: Hot_loop_osci_1_v2
TARGET: AR loops on the limb
EXPOSURE TIME: 5 s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 20"x112"
RASTER DURATION: 1m35s
REPEAT TIMES: 1
N_LINES 6
Ca XV, Ca XVII, Fe XII, Ca XV, Fe XVI and Fe XXIII
#Study C:
ACRONYM: Hot_loop_osci_2_v2
TARGET: AR loops on the limb
EXPOSURE TIME: 10 s
RASTER: Scanning
SLIT: 2"
STEP SIZE: 2"
FOV: 12"x112"
RASTER DURATION: 1m37s
REPEAT TIMES: 1
N_LINES 8
Ca XV, Ca XVII, Ca XIV, Fe XII, Ca XV, Fe XVI, Fe XXIII and Fe XVII
Pointing:
--------
Flare-productive active region on the limb, better located at the eastern limb.
For Study A, the 1/3 FOV is on the disk and 2/3 FOV off the limb.
For Studies B and and C the slit center position is set about 30-50 arcsec
above the AR on the limb (close to the core of the AR)
Use/Instructions to planners:
-----------------------------
i) Run Study A (ID=354) first to get a context image of AR.
ii) Repeat Study B (Hot_loop_osci_1) for about 5 hours, and then
run Study A again for a context image.
iii) Repeat Study C (Hot_loop_osci_2) for about 5 hours, and then
run Study A again.
iv) Stop or repeat ii) and iii) once more if possible.
Note: The above 10 hrs observations are better not interrupted.
We hope to make observations of at least 10 hrs every day
(better 20 hrs/day if allowed), and last for 4-5 days so we can track
the AR passing from behind the limb to the front
disk to catch loops of different sizes and different parts of loops
during this period.
Warning:
--------
The squence above should be run uninterrupted (preferably use chained studies),
i.e.(append to hilighted entry).
desc000418.txt
97290
1
0
Active Region
Scanning
524487
0
2
2
397
1
12
Off Limb AR loop sit and stare (V2)
DEI_AR_LOOP_V2
000419 DEI_AR_LOOP_V2
Davina Innes
Science
9-Jun-2010
Study 000419:
ACRONYM: DEI_AR_LOOP_V2
This study is designed to observe Doppler shift oscillations
in off-limb active region loop.
Its sustainable data rate (10kbps) allows continuous
observation.
TARGET: Active region
SLIT: 2"
RASTER: Sit-and-Stare
EXPOSURES #: 37
EXPOSURE TIME: 90 sec
RASTER DURATION: 59m 29s
VOLUME: 36 Mbits
LINELIST:
Fe XXIV 192.03
Fe XXIII 263.76
Ca XVII 192.82
Fe XVI 262.98
Fe XV 284.16
Fe XIV 274.20/264.79
Fe XII 195.12
Si VII 275.35
He II 256.32
Pointing:
---------
Active region loops above the limb.
Duration of 8 hours or longer is desired.
Warning:
--------
None
desc000419.txt
3591703
1
0
Active Region
Scanning
37253890
0
2
2
398
1
2
HPW021_VEL_120x512v1
HPW021_VEL_120x512v1
000420 HPW021_VEL_120x512v1
Harry Warren
Science
9-Jun-2010
Study 000420:
ACRONYM: HPW021_VEL_120x512v1
TARGET: Active Region
EXPOSURE TIME: 60s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 2"
FOV: 120"x512"
RASTER DURATION: 1h4m58s
VOLUME: 135 Mbits
RATE: 35 kbits/s
COMPRESSION: JPEG95
This study is designed for velocity studies in and around active
regions during eclipse season. The primary features of this study are:
[1] full slit, [2] relatively deep exposures (60s), and [3] extensive
line list. The current thinking is that the Fe VIII 185 and Si VII 275
lines are the best lines for velocity calibration.
The planner should not put the feature of interest in the middle of
the slit. Using the bottom or top third will provide more quiet Sun
for velocity calibration.
To accelerate the observing during eclipse season and to conserve
telemetry a 2" step is taken between exposures. The raster is also
relatively narrow (120" in 60 steps) so the duration will fit in
between eclipses.
The primary lines for each data window are:
1 180.40 32 # Fe XI 180.401
2 182.10 32 # Ca XV 181.900, Fe XI 182.167, Fe X 182.310
3 184.33 32 # O VI 184.117, Fe X 184.536
4 185.21 24 # Fe VIII 185.213
5 186.75 32 # Fe VIII 186.601, Ca XIV 186.610, Fe XII 186.880
6 188.40 48 # Ar XIV 187.964, Fe XI 188.216, Fe XI 188.299,
Fe IX 188.497, S XI 188.675
7 192.47 56 # Fe XXIV 192.040, Fe XII 192.394, Fe XI 192.813,
Ca XVII 192.858, O V 192.906
8 194.10 40 # Fe X 193.715, Ca XIV 193.874, Ar XIV 194.396
9 195.12 24 # Fe XII 195.119, Fe XII 195.179
10 197.86 24 # Fe IX 197.862
11 201.05 24 # Ca XV 200.972, Fe XIII 201.121
12 202.04 24 # Fe XIII 202.044
13 203.83 24 # Fe XII 203.720, Fe XIII 203.826
14 208.50 32 # Ca XV 208.324, Ca XVI 208.604, Fe XIII 208.679,
Ca XV 208.722
15 255.00 32 # Fe XVII 254.87, Fe XXIV 255.100
16 256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
17 258.37 24 # Si X 258.375
18 262.98 24 # Fe XVI 262.984
19 264.30 72 # Fe XXIII 263.760, S X 264.233, Fe XIV 264.787,
Fe XVI 265.003
20 270.52 24 # Mg VI 270.394, Fe XIV 270.519
21 275.40 24 # Si VII 275.368, Fe XVII 275.54
22 276.30 40 # Mg VII 276.153, Mg V 276.579
23 278.40 32 # Mg VII 278.402, Si VII 278.445
24 280.74 24 # Mg VII 280.737
25 284.16 24 # Al IX 284.015, Fe XV 284.160
Pointing:
---------
Adjust the pointing so that there is plenty of quiet Sun at the top OR
the bottom of the slit.
Instructions to planners:
-------------------------
** Do not ** put the feature of interest in the middle of
the slit. Put it in the bottom or top third of the slit
so that more quiet Sun will be provided for velocity calibration.
Warning:
-------
2" steps are taken between exposures (sparse raster)
desc000420.txt
3920397
1
0
Active Region
Scanning
138456339
0
0
0
399
1
119
Bright point response study (test) (2 rasters)
BP_response1_2raster
000421 BP_response1_2raster
Peter Young
Science
11-Jun-2010
Study 000421:
ACRONYM: BP_response1_2rasters
Small raster covering 100" x 128" and containing a selection of
lines. It is intended to be used as a response study for quiet Sun
bright points trigger (used in conjunction with ID #422)
Duration: 38m 38s (2 raster repeat)
Compression: DPCM
Data volume: 27 Mbits
Exposure time: 20s
Slit: 2"
Instruction to planners:
------------------------
See BP_hunter1
Warning:
--------
None
desc000421.txt
2318994
1
0
Quiet Sun
Scanning
28106442
0
2
2
400
2
100
Bright point hunter study (test)
BP_hunter1
000422 BP_hunter1
Peter Young
Science
11-Jun-2010
Study 000422:
ACRONYM: BP_hunter1
Large raster covering 456" x 512" and containing only Fe XII
195.12. It is intended to be used as a hunter study for quiet Sun
bright points.
Target: *** QS only ***
FOV: 456" x 512"
Compression: DPCM
Duration: 1 hr 30 mins
Data volume: 12.2 Mbits
Exposure time: 20s
Slit: 2"
Pointing:
---------
A patch of QS. Point the study (FIXED pointing) at:
MIP = 380
YIP = 306
Instruction to planners:
-------------------------
1) Run this study, once, during the (SAA-free) period.
The trigger settings for this study are:
X-threshold: 11161
Y-threshold: 258560
X-MIN limit: 7
Y-MIN limit: 1
2) Point the study as given in the pointing section above
(fixed pointing)
3) Use BP_response1 as a response study
4) Allow 1h gab following the hunt study completion on the timeline
(leave room for possible response run).
Warning:
--------
Do not run during SAA passes
desc000422.txt
5258507
1
0
Quiet Sun
Scanning
12503939
0
2
2
401
1
456
sit-n-stare slit for density measurements
arm_loop_ne_slit
000423 arm_loop_ne_slit
Dipankar Banerjee
Science
2-Jul-2010
Study 000423:
ACRONYM: arm_loop_ne_slit
This raster(id: 148) is part of the study arm_loop_ne (study id: 176). It
was designed for the density measurements in loops but we plan to use it as a
sit and stare support for our eclipse study in polar regions. We ended up in choosing
this in a trade off between the good signal and high cadence required during the
short eclispe duration.
TARGET : polar region.
RASTER TYPE : Sit'n'Stare
SLIT/SLOT : 2"
# Exposures : 30
EXPOSURE TIME : 45s
RASTER DURATON : 25m
DATA VOLUME : 31 Mbits
DATA COMP. : DPCM
LINES : Fe XII, XIII, He II, Ca XVII
POINTING:
---------
Polar region. some portion of the slit(atleast 50 pixels) should be on disk and
the slit should be placed inside the region scanned by the small raster
PRY_CH_density.
INSTRUCTION TO PLANNERS:
------------------------
For this Eclipse plan, the studies should be run in the following order:
* Run PRY_CH_density - once before the eclipse
* Run arm_loop_ne_slit - during the eclipse
* Run PRY_CH_density - once after the eclipse
WARNINGS:
---------
None
desc000423.txt
1498948
1
0
Polar region
Scanning
31491212
0
2
2
148
1
2
js2_decon_slot_scan
js2_decon_slot_scan
000424 js2_decon_slot_scan
Jian Sun
Calibration
6-Jul-2010
Study 000424:
ACRONYM: js2_decon_slot_scan
TARGET : Active region
EXPOSURE TIME : 15s
RASTER TYPE : 40" slot, Scan
# of pointings: 10
DATA COMP. : DPCM
RASTER DURATON: 3m37s
DATA volume : 1.02 MBytes
LINES : Fe XII, XIV, XXIV
POINTING:
---------
Simple configuration Active region is prefer. The scan FOV is better to cover
the edge of active region, where possible outflow is expected.
INSTRUCTION TO PLANNERS:
------------------------
1. This study ideally is used together with study js2_decon_ref_vel which is to get
reference velocity, so it's better to use same pointing for both studies.
2. This study requires repeatable runs (at least 10 times)
WARNINGS:
---------
* Run preferably during SAA-free time period.
desc000424.txt
217364
1
0
Active Region
Scanning
8558582
0
3
3
402
1
340
js2_decon_ref_vel
js2_decon_ref_vel
000425 js2_decon_ref_vel
Jian Sun
Calibration
6-Jul-2010
Study 000425:
ACRONYM: js2_decon_ref_vel
TARGET : Active region
EXPOSURE TIME : 15s
RASTER TYPE : 1" slit, Scan
# of pointings: 339
DATA COMP. : DPCM
RASTER DURATON: 1h40m46s
DATA volume : 23.34 MBytes
LINES : Fe XII, XIV, XXIV
POINTING:
---------
Simple configuration Active Region near disk center is prefer. The scan FOV
is better to cover the edge of active region, where possible outflow is expected.
INSTRUCTION TO PLANNERS:
------------------------
1. This study ideally is used together with study js2_decon_slot_scan - to get
reference velocity, so it's better to use same pointing as study js2_decon_slot_scan.
2. This study could be run before/after study js2_decon_slot_scan, but it's better
to run it in the middle of repeatable runs of js2_decon_slot_scan.
WARNINGS:
---------
* Run preferably during SAA-free time period.
desc000425.txt
6045581
1
0
Active Region
Scanning
195785368
0
0
0
403
1
340
Atlas_060x512_45s
Atlas_060x512_45s
000426 Atlas_060x512_45s
Harry Warren
Science
14-Jul-2010
Study 000426:
ACRONYM: ATLAS_060X512_45S
TARGET: Active Region
EXPOSURE TIME: 45s
RASTER: Scanning
SLIT: 1"
FOV: 60"x512" (1" steps)
RASTER DURATION: 49m35s
VOLUME: 823 Mbits
RATE: 276 kbits/s
COMPRESSION: DPCM
This is a VERY high data rate study for times during eclipse when SOT is not operating,
such as during a bakeout. The full CCD is taken over a relatively small field of view
(60x512) so that larger areas can be built up over time.
Pointing:
---------
If using for velocity studies, adjust the pointing so that there is plenty of quiet Sun at
the top OR the bottom of the slit. Position the active region at the top or bottom third
of the slit.
Instruction to planners:
------------------------
This study only does 60 steps of 45s exposures so that it can be during eclipse
season. This version of the study uses 45s exposures and can be run when there are both
hard eclipses and SAAs.
***
Use the 60s version (ID #427) of this raster (atlas_060x512_60s) for
observing during the Golden period (non SAA).
***
Use DPCM if possble, otherwise use JPEG95 or JPEG92.
Warning:
-------
* VERY HIGH DATA RATE!
* Do (not) run during SAA passes or eclipse
desc000426.txt
2975397
1
0
Active Region
Scanning
842370660
0
0
0
404
1
60
Atlas_060x512_60s
Atlas_060x512_60s
000427 Atlas_060x512_60s
Harry Warren
Science
14-Jul-2010
Study 000427:
ACRONYM: ATLAS_060X512_60S
TARGET: Active Region
EXPOSURE TIME: 60s
RASTER: Scanning
SLIT: 1"
FOV: 60"x512" (1" steps)
RASTER DURATION: 1h4m57s
VOLUME: 823 Mbits
RATE: 210 kbits/s
COMPRESSION: DPCM
This is a VERY high data rate study for times during eclipse when SOT is not operating,
such as during a bakeout. The full CCD is taken over a relatively small field of view
(60x512) so that larger areas can be built up over time.
Pointing:
---------
If using for velocity studies, adjust the pointing so that there is plenty of quiet Sun at
the top OR the bottom of the slit. Position the active region at the top or bottom third
of the slit.
Instruction to planners:
------------------------
This study only does 60 steps of 60s exposures so that it can be used during eclipse
season. This version of the study uses 60s exposures and can be run when there are no
SAAs (Golden period). Use the 45s version (ID #426) of this raster (atlas_060x512_45s)
for times with with both hard eclipse and SAA periods.
Use DPCM if possble, otherwise use JPEG95 or JPEG92.
Warning:
-------
* VERY HIGH DATA RATE!
* Do (not) run during SAA passes or eclipse
desc000427.txt
3920397
1
0
Active Region
Scanning
842370660
0
0
0
405
1
60
HPW021_VEL_120x512v2
HPW021_VEL_120x512v2
000428 HPW021_VEL_120x512v2
Harry Warren
Science
14-Jul-2010
Study 000428:
ACRONYM: HPW021_VEL_120x512v2
*** HPW021_VEL_120x512v2 is the same as HPW021_VEL_120x512v1
*** except for the exposure time, which has been shortened
*** to 45s to allow for running in between eclipses and SAA
*** periods.
TARGET: Active Region
EXPOSURE TIME: 45s
RASTER: Scanning
SLIT: 1"
FOV: 120"x512" (2" steps)
RASTER DURATION: 49m13s
VOLUME: 135 Mbits
RATE: 35 kbits/s
COMPRESSION: JPEG95
This study is designed for velocity studies in and around active
regions during eclipse season. The primary features of this study are:
[1] full slit, [2] relatively deep exposures (45s), and [3] extensive
line list. The current thinking is that the Fe VIII 185 and Si VII 275
lines are the best lines for velocity calibration.
To accelerate the observing during eclipse season and to conserve
telemetry a 2" step is taken between exposures. The raster is also
relatively narrow (120" in 60 steps) so the duration will fit in
between eclipses.
Pointing:
---------
Adjust the pointing so that there is plenty of quiet Sun at the top OR
the bottom of the slit.
Instruction to planners:
------------------------
The planner should (not) put the feature of interest in the middle of
the slit. Using the bottom or top third of the slit will provide more quiet Sun
for velocity calibration.
Warning:
-------
2" steps are taken between exposures.
desc000428.txt
2975397
1
0
Active Region
Scanning
138456339
0
0
0
406
1
119
js2_decon_slot_scan_LT
js2_decon_slot_sc_LT
000429 js2_decon_slot_sc_LT
Jian Sun
Science
20-Jul-2010
Study 000429:
ACRONYM: js2_decon_slot_sc_LT
TARGET : Active region
EXPOSURE TIME : 15s
RASTER TYPE : 40" slot, Scan
# of pointings: 4
DATA COMP. : DPCM
RASTER DURATON: 1m51s
DATA volume : 3.71 Mbits
LINES : Fe XII, XIV, XXIV
POINTING:
---------
Simple configuration Active Region is prefer; The scan FOV is better to cover the edge
of Active Region (include part of AR/part of surrounding area); cover possible outflow site.
INSTRUCTION TO PLANNERS:
------------------------
1. This study ideally is used together with study js2_decon_ref_vel_LT so that a reference
velocity could be collected; Please use _same pointing_ for both studies!
2. This study requires repeatable runs (~ 10 times) if possible.
WARNINGS:
---------
* Run preferably during SAA and Eclipse free time period.
desc000429.txt
111075
1
0
Active Region
Scanning
3890264
0
3
3
407
1
160
js2_decon_ref_vel_LT
js2_decon_ref_vel_LT
000430 js2_decon_ref_vel_LT
Jian Sun
Science
20-Jul-2010
Study 000430:
ACRONYM: js2_decon_ref_vel_LT
TARGET : Active region
EXPOSURE TIME : 15s
RASTER TYPE : 1" slit, Scan
# of pointings: 159
DATA COMP. : DPCM
RASTER DURATON: 47m37s
DATA volume : 87.87 Mbits
LINES : Fe XII, XIV, XXIV
POINTING:
---------
Simple configuration Active Region is prefer; The scan FOV is better to cover the edge
of Active Region (include part of AR/part of surrounding area); cover possible outflow site.
INSTRUCTION TO PLANNERS:
------------------------
1. This study ideally is used together with study js2_decon_slot_sc_LT to provide
reference velocity; Please use _same pointing_ for both studies!
2. This study could be run before/after study js2_decon_slot_sc_LT, however it's
better to run it in the middle of repeatable runs of js2_decon_slot_sc_LT.
WARNINGS:
---------
* Run preferably during SAA and Eclipse free time period.
desc000430.txt
2856891
1
0
Active Region
Scanning
92134290
0
0
0
408
1
160
Quiet Sun bright point response study, 40" slit (12 raster repeat)
BP_response_slot_tst
000431 BP_response_slot_tst
Peter Young
Science
28-Jul-2010
Study 000431:
ACRONYM: BP_response_slot_tst
Small raster covering 96" x 128" and containing a selection of
lines. It is intended to be used as a response study for quiet Sun
bright points trigger (used in conjunction with ID #432)
Duration: 20m 04s (12 raster repeat)
Raster duration: 1m 40s
Compression: DPCM
Data volume: 12 Mbits
Exposure time: 30s
Slot: 40"
Instruction to planners:
------------------------
See BP_hunter_v2
Warning:
--------
None
desc000431.txt
1227240
1
0
Quiet Sun
Scanning
12119664
0
3
3
409
12
104
Bright_point_hunter_study,test (v2)
BP_hunter_v2
000432 BP_hunter_v2
Peter Young
Science
28-Jul-2010
Study 000432:
ACRONYM: BP_hunter_v2
This study is similar to BP_hunter1 but half the number of exposures (114) and
double the mirror step size (4")
Large raster covering 456" x 512" and containing only Fe XII
195.12. It is intended to be used as a hunter study for quiet Sun
bright points.
Target: *** QS only ***
FOV: 456" x 512"
# Pointings: 114
Step size: 4"
Slit: 2"
Compression: DPCM
Duration: 44m
Data volume: 6 Mbits
Exposure time: 20s
Pointing:
---------
A patch of QS. Point the study (FIXED pointing) at:
MIP = 380
YIP = 306
Instruction to planners:
-------------------------
1) Run this study, once, during the (SAA-free) period.
The trigger settings for this study are:
X-threshold: 11161
Y-threshold: 258560
X-MIN limit: 7
Y-MIN limit: 1
2) Point the study as given in the pointing section above
(fixed pointing)
3) Use BP_response_slot_tst as a response study
4) Allow 21m gap following the hunt study completion on the timeline
(leave room for possible response run).
Warning:
--------
Do not run during SAA passes
desc000432.txt
2640504
1
0
Quiet Sun
Scanning
6251969
0
2
2
410
1
454
VHH_SlowAR_slow_scan_of_AR_to_search_for_line_assymetries_V2M_2
VHH_SlowAR_1h12_V2_2
000433 VHH_SlowAR_1h12_V2_2
Viggo Hansteen
Science
16-Aug-2010
Study 000433:
OBSOLETE : Imported by a mistake
desc000433.txt
4339478
1
0
Active Region
Scanning
34796020
0
0
0
356
1
257
VHH_SaS_of_AR_to_search_for_line_assymetries
vhh_slowar_sas_1h6m
000434 vhh_slowar_sas_1h6m
Viggo Hansteen
Science
16-Aug-2010
Study 000434:
ACRONYM: vhh_slowar_sas_1h6m (Asymmtery_sas)
This study is intended to be run on active region (or quiet sun) to look for
spectral line assymetries and their time variations
The study consists of a sit and stare with 120 exposures of 30s with
of EIS's 2 arcsec slit, producing a continuous observation of a given
location in an active region or on the quiet sun over roughly one hour.
Target: Active region or quiet sun
Type: sit and stare
Field of view: 2"x296"
Exposure time: 30s
Slit: 2"
step size: 2"
Study Duration: 1h 7m 18s
Data Volume: 106 Mbits
Instruction to planners:
-----------------------
It should be run, where possible, in co-ordinated observations with SOT
and if possible in conjuction with a raster (VHH_SlowARbig_1h23m) of the
surrounding region that has the same line list.
WARNING:
--------
None
desc000434.txt
4038293
1
0
Active Region
Scanning
108432600
0
2
2
411
1
2
VHH_SlowAR_slow_scan_of_300arcsec_AR_to_search_for_line_assymetries
VHH_SlowARbig_1h23
000435 VHH_SlowARbig_1h23
Viggo Hansteen
Science
16-Aug-2010
Study 000435:
ACRONYM: VHH_SlowARbig_1h23 (Assymmetry_big)
This study is intended to be run on active region (or quiet sun) to look for
spectral line assymetries and their time variations
The study consists of a large raster (300x300 arcsec) with 150 exposures
of 30s with of EIS's 2 arcsec slit to produce a context image and line profile
data for use in conjuction with a small fast raster (VHH_HI_BRT_SCAN_EXT)
or a sit and stare study (vhh_slowar_sas_1h6m) that are designed to
concentrate on time variations in a small regions.
Target: Active region or quiet sun
Type: scanning raster
Field of view: 296"x300"
Exposure time: 30s
Slit: 2"
step size: 2"
Study Duration: 1h 24m 2s
Data Volume: 77 Mbits
Instruction to planners:
-----------------------
It should be run, where possible, in co-ordinated observations with SOT and
preceding or followed by either the VHH_HI_BRT_SCAN_EXT or vhh_slowar_sas_1h6m
WARNING:
--------
None
desc000435.txt
5042242
1
0
Active Region
Scanning
79010343
0
2
2
412
1
300
Sixteen-arcsecond rapid scan for TR line assymetries
VHH_HI_BRT_SCAN_EXT
000436 VHH_HI_BRT_SCAN_EXT
Viggo Hansteen
Science
16-Aug-2010
Study 000436:
ACRONYM: VHH_HI_BRT_SCAN_EXT
This study is intended to be run on active region (or quiet sun) to look for
spectral line assymetries and their time variations
The study consists of a single raster, with 8 contiguous positions
of EIS's narrow slit, making a narrow but tall scan with 25-second
exposures at each position. This scanning raster should be repeated
at least 12-16 times to make an approximately one-hour duration study.
Target: Active region or quiet sun
Type: scanning raster
Field of view: 16"x240"
Exposure time: 25s
Slit: 2"
step size: 2"
Study Duration: 4m 8s
Data Volume: 5.6 Mbits
Instruction to planners:
-----------------------
Repeat the raster 12 times, at least. Fill the TM slot available
It should be run, where possible, in co-ordinated observations with SOT.
The study is an extension of VHH_HI_BRT_SCAN with slightly altered line
window widths and a larger FOV to make co-alignment with SOT easier.
If possible this study should be run in conjuction with
(VHH_SlowARbig_1h23m) of the surrounding region that has the same line list.
WARNING:
--------
None
desc000436.txt
248220
1
0
Active Region
Scanning
5758393
0
2
2
413
1
16
HPW021_VEL_240x512v1
HPW021_VEL_240x512v1
000437 HPW021_VEL_240x512v1
Harry Warren
Science
19-Aug-2010
Study 000437:
ACRONYM: HPW021_VEL_240x512v1
TARGET: Active Region
EXPOSURE TIME: 60s
RASTER: Scanning
SLIT: 1"
STEP SIZE: 2"
FOV: 240"x512" (2" steps)
RASTER DURATION: 2h9m56s
VOLUME: 270 Mbits
RATE: 35 kbits/s
COMPRESSION: JPEG95
This study is designed for velocity studies in and around active
regions. The primary features of this study are: [1] full slit, [2]
relatively deep exposures (60s), and [3] extensive line list. The
current thinking is that the Fe VIII 185 and Si VII 275 lines are the
best lines for velocity calibration.
The planner should (not) put the feature of interest in the middle of
the slit. Using the bottom or top third will provide more quiet Sun
for velocity calibration.
To accelerate the observing and to conserve telemetry a 2" step is
taken between exposures.
The primary lines for each data window are:
1 180.40 32 # Fe XI 180.401
2 182.10 32 # Ca XV 181.900, Fe XI 182.167, Fe X 182.310
3 184.33 32 # O VI 184.117, Fe X 184.536
4 185.21 24 # Fe VIII 185.213
5 186.75 32 # Fe VIII 186.601, Ca XIV 186.610, Fe XII 186.880
6 188.40 48 # Ar XIV 187.964, Fe XI 188.216, Fe XI 188.299,
Fe IX 188.497, S XI 188.675
7 192.47 56 # Fe XXIV 192.040, Fe XII 192.394, Fe XI 192.813,
Ca XVII 192.858, O V 192.906
8 194.10 40 # Fe X 193.715, Ca XIV 193.874, Ar XIV 194.396
9 195.12 24 # Fe XII 195.119, Fe XII 195.179
10 197.86 24 # Fe IX 197.862
11 201.05 24 # Ca XV 200.972, Fe XIII 201.121
12 202.04 24 # Fe XIII 202.044
13 203.83 24 # Fe XII 203.720, Fe XIII 203.826
14 208.50 32 # Ca XV 208.324, Ca XVI 208.604, Fe XIII 208.679,
Ca XV 208.722
15 255.00 32 # Fe XVII 254.87, Fe XXIV 255.100
16 256.48 32 # He II 256.317, Si X 256.366, S XIII 256.686
17 258.37 24 # Si X 258.375
18 262.98 24 # Fe XVI 262.984
19 264.30 72 # Fe XXIII 263.760, S X 264.233, Fe XIV 264.787,
Fe XVI 265.003
20 270.52 24 # Mg VI 270.394, Fe XIV 270.519
21 275.40 24 # Si VII 275.368, Fe XVII 275.54
22 276.30 40 # Mg VII 276.153, Mg V 276.579
23 278.40 32 # Mg VII 278.402, Si VII 278.445
24 280.74 24 # Mg VII 280.737
25 284.16 24 # Al IX 284.015, Fe XV 284.160
Pointing:
---------
Adjust the pointing so that there is plenty of quiet Sun at the top OR
the bottom of the slit.
Instructions to planners:
-------------------------
** Do not ** put the feature of interest in the middle of
the slit. Put it in the bottom or top third of the slit
so that more quiet Sun will be provided for velocity calibration.
Warning:
-------
2" steps are taken between exposures (sparse raster), 1" slit
desc000437.txt
7818293
1
0
Active Region
Scanning
276912679
0
0
0
414
1
239
on_nature_of_propagating_waves_in_polar_coronal_holes_v2
iiap_ch_ctxt_v2
000438 iiap_ch_ctxt_v2
Banerjee D
Science
6-Sep-2010
Study 000438:
ACRONYM: iiap_ch_ctxt_v2
This is a context study for HOP 0175 to detect propagating waves in polar coronal hole
(to be used with SNS study #ID 439). The line list is chosen such that a density map
can also be produced from the context raster. Therefore, DPCM is requested to ensure
good line profiles.
TARGET : Coronal Hole.
EXPOSURE TIME : 60s
RASTER TYPE : Scanning
SLIT : 2"
# of pointings: 59
DATA COMP. : DPCM
RASTER DURATON: 1h 4m
DATA volume : 86 Mbits
LINES : Fe X, Fe XII, Ca XVII, Fe XII, Fe XIII, Fe XIII, He II
Pointing:
--------
For HOP 0175, the 512" long slit should be positioned on a coronal hole such
that 300" of the slit should be above the limb.
INSTRUCTION TO PLANNERS:
------------------------
See study #ID 439
Warning:
--------
None
desc000438.txt
3920397
1
0
Coronal Hole
Scanning
88843780
0
2
2
415
1
120
on_nature_of_propagating_waves_in_polar_coronal_holes_v2_SNS
iiap_ch_sns_v2
000439 iiap_ch_sns_v2
Banerjee D
Science
6-Sep-2010
Study 000439:
ACRONYM: iiap_ch_sns_v2
This is a SNS study for HOP 0175 to detect propagating waves in polar coronal hole.
DPCM is requested to ensure good line profiles.
TARGET : Coronal Hole.
EXPOSURE TIME : 60s
RASTER TYPE : Sit'n'stare
SLIT : 2"
# of pointings: 180
DATA COMP. : DPCM
RASTER DURATON: 3h 14m
DATA VOLUME : 260 Mbits
LINES : Fe X, Fe XII, Ca XVII, Fe XII, Fe XIII, Fe XIII, He II
POINTING:
---------
For HOP 0175, the 512" long slit should be positioned on a coronal hole such that
300" part of the slit should be above the limb.
INSTRUCTION TO PLANNERS:
------------------------
For HOP 0175 the studies should be run in the following order (preferably chained,
i.e. appended to the context raster).
1) Run iia_ch_ctxt_v2 (context study, #ID 438)
2) Run this study TWICE (sit'n'stare study), as follows
* For first run choose X=0" and
* For the second run shift the X position by about 30" so that both the plume
and interplume regions are covered.
Total Run-time: ~7h 35m
Total data volume: 620 Mbits
WARNING:
--------
* Run preferably during SAA-free time period (start of golden period)
* High data volume HOP
desc000439.txt
11716190
1
0
Coronal Hole
Scanning
266531341
0
2
2
416
1
2
EIS/SDO diagnostics, AR
madj_ar_sns_15m
000440 madj_ar_sns_15m
Maria Madjarska
Science
7-Sep-2010
Study 000440:
ACRONYM: madj_ar_sns_15m
The study will run in Active regions.
Target: active region
Expsore time: 5 sec
# Exposures: 120
Type: Sit-and-stare
slit: 2"
FOV: 2"x240"
Run-time: 14m 25s
Data Volume: 66 Mbits
Pointing:
---------
Active region
Instruction to planners:
------------------------
Solar rotational compensation i.e., tracking the same region on the Sun
1) Run madj_ar (context study, #ID 348)
2) Run this study. Adjust the raster repeat to fill the available TM
Warning:
-------
Do not run it within SAA.
desc000440.txt
888293
1
0
Active Region
Scanning
68333269
0
2
2
417
1
2
EIS/SDO_diagnostics, QS
madj_qs_sns_15m
000441 madj_qs_sns_15m
Maria Madjarska
Science
7-Sep-2010
Study 000441:
ACRONYM: madj_qs_sns_15m
The study will run in Quiet sun.
Target: QS
Expsore time: 25 sec
# Exposures: 30
Type: Sit-and-stare
slit: 2"
FOV: 2"x240"
Run-time: 14m 29s
Data Volume: 16 Mbits
Pointing:
---------
Quiet sun region
Instruction to planners:
------------------------
Solar rotational compensation i.e., tracking the same region on the Sun
1) Run madj_ar ONCE (context study, #ID 348)
2) Run this study. Adjust the raster repeat to fill the available TM.
Warning:
-------
Do not run within SAA.
desc000441.txt
868948
1
0
Quiet Sun
Scanning
16858536
0
2
2
418
1
2
FullSunSlit_SI
FullSunSlit_SI
000442 FullSunSlit_SI
Shin Imada
Science
10-Sep-2010
Study 000442:
ACRONYM: FullSunSlit_SI
This study is design to observe Full Sun or large FOV.
Lines: FeX (184.54), CaXVII(192.82), FeVIII(194.66), FeXII(195.12),
HeII (256.35), FeXV(284.16).
Study summary:
-------------
slit: 2"
S/C pointing: Full sun or large FOV
window height: 512"
exposure time: 20s
# of pointing: 255 (total X size is 512)
step size: 2"
FOV: 512X512
duration: 1h38m33s
data volume: 69 Mbits
Instruction to planner:
----------------------
This study is design to observe Full Sun or large FOV.
To observe the Full sun, you have to run this study at least 16 times.
It takes 26h + 16 S/C pointing duration, Data Volume of 1100 Mbits (1.1 Gbits)
Warning:
--------
If run for Full Sun scan, a total of 1100 Mbits (1.1 Gbits) is required
desc000442.txt
5901526
1
0
Quiet Sun
Scanning
69564068
0
2
2
419
1
512