FA - Filament Activation 2019-03-28T08:27:26 -> 2019-03-28T10:24:49 xcen, ycen = -711.8,684.5
Description: Fast re-build of the prominence body can be observed. Relatively complicated velocity field and fast motion result in large difference between the raster images obtained in blue and red wings of Mg II lines.
Solar Object Locator:
SOL2019-03-28T08:27:26L067C047 |
Properties:
Event Title | Dynamics of plasma in quiescent prominence |
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Data Source
Observatory | IRIS |
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Instrument | IRIS_SG |
Mean Wavelength | 2.796e-05 cm |
Channel ID | Mg II hk |
Rating:
Overall Rating | |
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Number of Ratings |
Identification Method
FRM Name | Arkadiusz Berlicki (Other features and events submitted by Arkadiusz Berlicki) |
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FRM Institute | LMSAL |
FRM Contact | Ryan Timmons |
FRM Date Run | 2019-04-10T14:47:32 |
FRM Identifier | WebAnnotator |
FRM Parameters | Build_20160418 |
FRM URL | n/a |
FRM Human Flag | true |
Nearby Events:
View in iSolSearch |
Get SDO Data |
References:
Movie | ||
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Get Data | ivorn | ivo://sot.lmsal.com/VOEvent#VOEvent_IRIS_20190328_060612_3600109762_2019-03-28T06:06:122019-03-28T06:06:12.xml |
Event Image | image | http://www.lmsal.com/solarsoft/irisa/data/level2/2019/03/28/20190328_060612_3600109762/www/l2_20190328_060612_3600109762_SJI_2796_t000_fits_20190328_060612_j_fthumb.gif |
Movie | ||
HER VOEvent | XML | |
Full HER VOEvent |
First Event IVORN | Edge Type | Second Event IVORN | Strength | Reported By |
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Revisions:
Revision # | Revision Date | Revised By |
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1 | 2019-04-10 | aberlick7 |
Comments:
Comment By | Comment Date | Comment |
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