stereoa_impactplastic_icme

Parameters
name: hec_id
datatype: int ucd: meta.record
xtype: utype:
description: Event Identification number (HEC internal number).
name: id
datatype: int ucd: meta.id
xtype: utype:
description: Event identifier (reset at beginning of year).
name: flag
datatype: char ucd: meta.code
xtype: utype:
description: ? indicates an ambiguous event * indicates a hybrid event (i.e. Combined with another solar wind structure)
name: spacecraft
datatype: char ucd: instr.obsty
xtype: utype:
description: STEREO spacecraft B.
name: time_start
datatype: char ucd: time.start
xtype: iso8601 utype:
description: Start time of the event.
name: time_mag_obstacle_start
datatype: char ucd: time.start;phys.magField
xtype: iso8601 utype:
description: tart time of magnetic obstacle (~ flux rope).
name: time_end
datatype: char ucd: time.end
xtype: iso8601 utype:
description: End time of the event.
name: pt_max
datatype: float ucd: phys.pressure;stat.max
xtype: utype:
description: The maximum total pressure (Pt, sum of magnetic and perpendicular plasma thermal pressures) perpendicular to the magnetic field.
name: pt_max_sheath
datatype: float ucd: phys.pressure;stat.max
xtype: utype:
description: Maximum Pt including the sheath region.
name: b_max
datatype: float ucd: stat.max;phys.magField
xtype: utype:
description: Maximum magnetic field measured in the event.
name: b_max_sheath
datatype: float ucd: stat.max;phys.magField
xtype: utype:
description: Maximum magnetic field including the sheath region.
name: v_max
datatype: int ucd: phys.veloc;stat.max
xtype: utype:
description: Maximum velocity.
name: v_max_sheath
datatype: int ucd: phys.veloc;stat.max
xtype: utype:
description: Maximum velocity including the sheath region.
name: delta_v
datatype: int ucd: arith.rate;phys.veloc
xtype: utype:
description: Temporal variation of solar wind speed over one event, negative value indicating solar wind is expanding. No value means the solar wind speed remains almost constant over the event.
name: groups
datatype: int ucd: meta.code.class
xtype: utype:
description: In the hypothesis that all ICMEs have a central flux rope, these three groups of Pt profiles are due to different approach distances to the central flux rope. Group 1 includes events that appear to be traversed near the ICME center, showing an apparent enhanced central Pt Group 3 represents ICMEs passed far away from the center, displaying a rapid rise and then gradual decay in Pt; Group 2 includes events with intermediate signatures.
name: comment
datatype: char ucd: meta.note
xtype: utype:
description: Short description of event.

Extracted from VOTable generated by HEC HQI on:   07-Sep-17 18:38:33