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OT - Other 2023-04-19T10:53:17 -> 2023-04-19T11:08:45 xcen, ycen = -331.3,-279.8

http://www.lmsal.com/hek/her?cmd=view-voevent&ivorn=ivo://helio-informatics.org/OT_IRIS_Si_IV_AparnaVenkataramanasastry_20230504_013804

Description: Loops overlying the filament, which is on the right side of the frame of observations, heat up and cause energy depositions along the ends of the loops in the chromosphere and transition region as seen in the 1330, 1400 and 2796 Angstrom movies, giving it a flare-ribbon like appearance. Hot loops can be seen in AIA 94 A channel, although evidence for a flare is not seen. The loop ends on the other side are not covered in the IRIS field of view in this observation.

Solar Object Locator:
SOL2023-04-19T10:53:17L355C111

Properties:
Event Title Ribbons
Event Peak time2023-04-19T10:54:46

Data Source
ObservatoryIRIS
InstrumentIRIS
Mean Wavelength1.400e-05 cm
Channel IDSi IV

Rating:
Overall Rating
Number of Ratings

Identification Method
FRM NameAparna Venkataramanasastry (Other features and events submitted by Aparna Venkataramanasastry)
FRM InstituteLMSAL
FRM ContactRyan Timmons
FRM Date Run2023-05-04T01:38:04
FRM IdentifierWebAnnotator
FRM ParametersBuild_20200519
FRM URLn/a
FRM Human Flagtrue

Nearby Events:
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Get SDO Data

References:
Movie
Event Image image https://www.lmsal.com/solarsoft/irisa/data/level2/2023/04/19/20230419_101008_3600104038/www/l2_20230419_101008_3600104038_SJI_1400_t000_fits_20230419_101018_j_fthumb.gif
Movie
Get Data ivorn ivo://sot.lmsal.com/VOEvent#VOEvent_IRIS_20230419_101008_3600104038_2023-04-19T10:10:082023-04-19T10:10:08.xml
HER VOEventXML
Full HER VOEvent

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

Revisions:
Revision # Revision Date Revised By
1 2023-05-04 Aparna Venkataramanasastry

Comments:
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