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CH - Coronal Hole 2017-11-02T14:30:09 -> 2017-11-03T20:20:09 xcen, ycen = -253,559

http://www.lmsal.com/hek/her?cmd=view-voevent&ivorn=ivo://helio-informatics.org/CH6173_GeorgiosChintzoglou_20171107_220657

Description: A coronal hole (dark region on the North East quadrant of the solar disk) is accompanied by two filaments running parallel to it at higher latitudes. As the time goes by, the high-latitude filament erupts folllowed by the one nearest to the coronal hole ~10 hours later. No CME was identified with SOHO/LASCO; therefore, the eruptions were not ejective but rather contained in the low solar corona.

Solar Object Locator:
SOL2017-11-02T14:30:09L029C051

Properties:
Event Title A Coronal Hole Two (Sympathetic?) Confined Eruptions

Data Source
ObservatorySDO
InstrumentHMI
Mean Wavelength6.173e-05 cm
Channel ID6173

Rating:
Overall Rating 3.0 (0=lowest, 5=highest)
Number of Ratings1

Identification Method
FRM Namegchintzo (Other features and events submitted by gchintzo)
FRM InstituteLMSAL/UCAR
FRM ContactScott Green
FRM Date Run2017-11-07T22:06:57
FRM IdentifierAnnotator-build_20120514-avc
FRM Parametersn/a
FRM URLn/a
FRM Human Flagtrue

Nearby Events:
View in iSolSearch
Get SDO Data

References:
Movie
CH: HER Entry ivorn ivo://helio-informatics.org/CH211_GeorgiosChintzoglou_20171107_220657
CH: HER Entry ivorn ivo://helio-informatics.org/CH193_GeorgiosChintzoglou_20171107_220657
CH: HER Entry ivorn ivo://helio-informatics.org/CH171_GeorgiosChintzoglou_20171107_220657
Movie
HER VOEventXML
Full HER VOEvent

Links:
First Event IVORN Edge Type Second Event IVORN Strength Reported By
ivo://helio-informatics.org/CH6173_GeorgiosChintzoglou_20171107_220657 is_member_of ivo://helio-informatics.org/CHMET_GeorgiosChintzoglou_20171107_220657 1.0 chintzoglou_georgios

Revisions:
Revision # Revision Date Revised By
1 2017-11-07 chintzoglou_georgios

Comments:
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