Parameters | |||
name: | hec_id | ||
datatype: | int | ucd: | meta.record |
xtype: | utype: | ||
description: | Event identification number (HEC internal number) | ||
name: | time_start | ||
datatype: | char | ucd: | time.start |
xtype: | iso8601 | utype: | helio:time_period.time_start |
description: | Start time of the type II burst. | ||
name: | time_end | ||
datatype: | char | ucd: | time.end |
xtype: | iso8601 | utype: | helio:time_period.time_end |
description: | End time of the type II burst. | ||
name: | freq_start | ||
datatype: | int | ucd: | em.freq |
xtype: | utype: | helio:radio.frequency_start | |
description: | Starting frequency of type II burst (kHz). | ||
name: | freq_end | ||
datatype: | int | ucd: | em.freq |
xtype: | utype: | helio:radio.frequency_end | |
description: | Ending frequency of type II burst (kHz). | ||
name: | lat_hg | ||
datatype: | %datatype% | ucd: | %ucd% |
xtype: | %xtype% | utype: | %utype% |
description: | %description% | ||
name: | long_hg | ||
datatype: | %datatype% | ucd: | %ucd% |
xtype: | %xtype% | utype: | %utype% |
description: | %description% | ||
name: | long_carr | ||
datatype: | %datatype% | ucd: | %ucd% |
xtype: | %xtype% | utype: | %utype% |
description: | %description% | ||
name: | loc | ||
datatype: | char | ucd: | pos.bodyrc;pos.heliographic |
xtype: | utype: | helio | |
description: | Solar source location (Loc) of the associated eruption in heliographic coordinates. S25E16 means the latitude is 25 deg south and 16 deg east (source located in the southeast quadrant of the Sun. N denotes northern latitudes and W denotes western longitudes. Entries like SW90 indicate that the source information is not complete, but we can say that the eruption occurs on the west limb but at southern latitudes; if such entries have a subscript b (e.g., NE90b) it means that the source is behind the particular limb. This information is usually gathered from SOHO/EIT difference images, which show dimming above the limb in question. Completely backside events with no information on the source location are marked as BACK. | ||
name: | nar | ||
datatype: | int | ucd: | meta.id.cross |
xtype: | utype: | :helio:flare.nar | |
description: | NOAA active region index. If the active region number is not available or if the source region is not an active region, the entry is blank. Filament regions are denoted by FILA or DSF for disappearing solar filament. | ||
name: | filar | ||
datatype: | %datatype% | ucd: | %ucd% |
xtype: | %xtype% | utype: | %utype% |
description: | %description% | ||
name: | xray_class | ||
datatype: | char | ucd: | meta.code.class;em.X-ray |
xtype: | utype: | helio:flare.magnitude.xray_class | |
description: | Importance of flare at X-ray wavelengths -- the peak flux measured at Earth in the 0.1 to 0.8 nm range in units of Watts/sq meter. (See the 'X-ray Class' in the HEC glossary for the specification of this field) | ||
name: | time_cme | ||
datatype: | char | ucd: | |
xtype: | iso8601 | utype: | |
description: | Time of the associated CME. | ||
name: | pa | ||
datatype: | double | ucd: | pos.posAng |
xtype: | utype: | helio:location.pa | |
description: | Central position angle for non-halo CMEs. (See the 'Central position angle' in the HEC glossary for the specification of this field) | ||
name: | pa_width_ll | ||
datatype: | %datatype% | ucd: | %ucd% |
xtype: | %xtype% | utype: | %utype% |
description: | %description% | ||
name: | pa_width | ||
datatype: | double | ucd: | pos.posAng;phys.angSize |
xtype: | utype: | helio:location.pa_width | |
description: | CME width in the sky plane. Width = 360 means the CME is a fill halo. For some entries, there is a prefix >, which means the reported width is a lower limit. | ||
name: | v_ps | ||
datatype: | double | ucd: | phys.veloc |
xtype: | utype: | helio:cme.velocity.v_plane_of_sky | |
description: | CME speed in the sky plane (km/s). | ||
name: | comment | ||
datatype: | char | ucd: | meta.note |
xtype: | utype: | helio:comment | |
description: | Comments. |
Extracted from VOTable generated by HEC HQI on: 07-Sep-17 18:38:13