stereo_euvi_event

Parameters
name: hec_id
datatype: int ucd: meta.record
xtype: utype:
description: Event identification number (HEC internal number)
name: id_num
datatype: int ucd: meta.id.cross
xtype: utype:
description: STEREO/EUVI event Catalogue Number.
name: time_start
datatype: char ucd: time.start
xtype: iso8601 utype: helio:time_period.time_start
description: Start time
name: time_end
datatype: char ucd: time.end
xtype: iso8601 utype: helio:time_period.time_end
description: End time
name: lat_hg
datatype: float ucd: pos.bodyrc.lat;pos.heliographic
xtype: utype: helio:location.lat_hg
description: Heliographic Latitude.
name: long_hg
datatype: float ucd: pos.bodyrc.long;pos.heliographic
xtype: utype: helio:location.long_hg
description: Heliographic Longitude.
name: long_carr
datatype: float ucd: pos
xtype: utype: helio:location.long_carr
description: Carrington longitude of active region
name: cadence
datatype: int ucd:
xtype: utype: helio:instr.cadence_s
description: Instrument cadence.
name: spacecraft
datatype: char ucd: instr.obsty
xtype: utype: helio:observatory.observatory_name
description: Spacecraft ID
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 W m^-2. (See the 'X-ray Class' in the HEC glossary for the specification of this field)
name: rhessi_peak_range
datatype: char ucd: phys.energy;stat.max;inst.bandwidth
xtype: utype:
description: Peak RHESSI energy range in which event is observed.
name: rhessi_peak_count
datatype: int ucd: phys.energy;stat.max;meta.number
xtype: utype:
description: Counts in peak RHESSI energy range.
name: comment
datatype: char ucd: meta.note
xtype: utype: helio:comment
description: Comments using the following EUVI Classification: A=Ahead only without Behind data B=Behind only without Ahead data I=Impulsive time profile (peak in coincidence with SXR) P=Postflare loop or arcade (delayed emission after SXR peak) D=Dimming (EUV flux decreases after SXR peak) E=Eruptive filament O=Occulted for A (if flare position is east) or B (if west) T=Test images (or poor image quality) W=Waves and oscillations
name: cme_event_source
datatype: char ucd: instr
xtype: utype:
description: CME reported by one or both of the following: L=LASCO/SOHO S=SECCHI/Cor-1,Cor-2

Extracted from VOTable generated by HEC HQI on:   07-Sep-17 18:38:14