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FE - Filament Eruption 2019-01-02T19:25:13 -> 2019-01-03T00:41:13 xcen, ycen = 502,-690

http://www.lmsal.com/hek/her?cmd=view-voevent&ivorn=ivo://helio-informatics.org/FE171_halocme_20190105_220829

Description: This is best seen in intensity images in 304 A. Other low coronal signatures seem to be quite limited, implying that it is not a major event. The associated CME is not impressive (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20190102.234807.w012.v0596.p251&frame=6&r_. Part of the reason may be that equatorial coronal holes prevent the eruption extending toward the equator. This event was predicted by a famous solar physicist shortly before the occurrence (https://twitter.com/cosmic_jet/status/1080578605271273472).

Solar Object Locator:
SOL2019-01-02T19:25:13L234C137

Properties:
Event Title Eruption of a polar crown filament

Data Source
ObservatorySDO
InstrumentAIA
Mean Wavelength1.710e-06 cm
Channel ID171

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

Identification Method
FRM Namehalocme (Other features and events submitted by halocme)
FRM InstituteLMSAL
FRM ContactScott Green
FRM Date Run2019-01-05T22:08:29
FRM IdentifierAnnotator-20171220-ext
FRM Parametersn/a
FRM URLn/a
FRM Human Flagtrue

Nearby Events:
View in iSolSearch
Get SDO Data

References:
Movie
FE: HER Entry ivorn ivo://helio-informatics.org/FE304_halocme_20190105_220829
FE: HER Entry ivorn ivo://helio-informatics.org/FE211_halocme_20190105_220829
HER VOEventXML
Full HER VOEvent

Links:
First Event IVORN Edge Type Second Event IVORN Strength Reported By
ivo://helio-informatics.org/FE171_halocme_20190105_220829 is_member_of ivo://helio-informatics.org/FEMET_halocme_20190105_220829 1.0 nitta_nariaki

Revisions:
Revision # Revision Date Revised By
1 2019-01-05 nitta_nariaki

Comments:
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