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FL - Flare 2014-10-24T21:09:08 -> 2014-10-24T21:42:09 xcen, ycen = 235,-309.7

http://www.lmsal.com/hek/her?cmd=view-voevent&ivorn=ivo://helio-informatics.org/FL_IRIS_SG_C_II_JakubPrchlik_20160920_152045

Description: IRIS observes a GOES X3.1 flare in AR 12192, which was the largest AR since November 1990. The flare occurs within the first few frames of the observation and crosses the slit. The flare's brightness comes from two ribbons, which are roughly parallel. After formation, the two ends of the larger ribbon pivot downward in the image towards the coronal hole in the bottom left. However, some structure near the center of the larger ribbon prevents the central part of the ribbon from capping the coronal hole. This is clearly seen in 1330 Å and 2796 Å, however, 2796 ?Å shows faint absorption flows following the flare not easily visible in 2796 Å. In the spectrum Fe XXI shows broad emission near the flare's end.

Solar Object Locator:
SOL2014-10-24T21:09:08L245C103

Properties:
Event Title GOES X3.1 Flare
Event Peak time2014-10-24T21:16:43

Data Source
ObservatoryIRIS
InstrumentIRIS_SG
Mean Wavelength1.330e-05 cm
Channel IDC II

Rating:
Overall Rating
Number of Ratings

Identification Method
FRM NameJakub Prchlik (Other features and events submitted by Jakub Prchlik)
FRM InstituteLMSAL
FRM ContactRyan Timmons
FRM Date Run2016-09-20T15:20:45
FRM IdentifierWebAnnotator
FRM ParametersBuild_20160418
FRM URLn/a
FRM Human Flagtrue

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References:
Movie
Get Data ivorn ivo://sot.lmsal.com/VOEvent#VOEvent_IRIS_20141024_205222_3860111353_2014-10-24T20:52:222014-10-24T20:52:22.xml
Event Image image http://www.lmsal.com/solarsoft/irisa/data/level2/2014/10/24/20141024_205222_3860111353/www/l2_20141024_205222_3860111353_SJI_1330_t000_fits_20141024_205222_j_fthumb.gif
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HER VOEventXML
Full HER VOEvent

Links:
First Event IVORN Edge Type Second Event IVORN Strength Reported By

Revisions:
Revision # Revision Date Revised By
1 2016-09-20 jprchlik

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