wind_typeii_soho_cme

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