Recent Events Reported by Observers
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Detected by jinmeng, Submitted at 2016-04-05T01:24:54
2016-04-04T09:50:06 --> 2016-04-04T22:00:06
A filament eruption with large-scale coronal activities. Before the main eruption, there is a small-scale eruption from a compact brighting region, which may play a role for triggering the following main eruption.
Detected by jinmeng, Submitted at 2016-04-05T01:05:27
2016-04-04T13:50:06 --> 2016-04-04T21:30:06
A small eruption near the west limb, which leads to loop activities above the source region.
Detected by jinmeng, Submitted at 2016-04-05T00:52:16
2016-04-04T00:00:06 --> 2016-04-04T09:10:06
A filament near east limb erupted with two-ribbons formed underneath. There are evident loop brightenings that associate with the eruption. Also, multiple loop activities from a distance region to the SW suggest large-scale magnetic coupling between the erupting and ambient field.
Detected by jinmeng, Submitted at 2016-04-04T18:40:40
2016-04-03T06:20:06 --> 2016-04-03T13:40:06
A coronal jet in the north coronal hole.
Detected by jinmeng, Submitted at 2016-04-04T18:30:25
2016-04-02T09:50:03 --> 2016-04-02T23:50:03
Small eruption near the west limb.
Detected by jinmeng, Submitted at 2016-04-04T18:21:02
2016-04-03T06:40:06 --> 2016-04-03T23:00:06
A small eruption from AR 12528. The eruption seems to relate to a flux emergence nearby. And this flux emergence also leads to coronal loop activitis and reconfigurations.
Detected by jinmeng, Submitted at 2016-04-04T17:55:10
2016-04-03T09:20:06 --> 2016-04-03T23:00:06
Coronal Rain observed near the west limb.
Detected by derosa, Submitted at 2016-03-29T01:21:11
2016-03-17T02:00:06 --> 2016-03-17T08:00:06
A circular filament is disturbed as flux emerges nearby.
Detected by derosa, Submitted at 2016-03-29T01:21:11
2016-03-17T02:00:06 --> 2016-03-17T08:00:06
A circular filament is disturbed as flux emerges nearby.
Detected by derosa, Submitted at 2016-03-29T00:06:02
2016-03-16T06:00:06 --> 2016-03-16T07:30:06
Two filament eruptions, one at the limb and one on disk, occur nearly simultaneously.
Detected by halocme, Submitted at 2016-03-26T05:36:53
2016-03-21T23:40:10 --> 2016-03-22T00:40:10
This LCPF was from an eruption in a quiescent region. No GOES X-ray flare was associated. No CME was detected either, partly because of the proximity of the eruption to the disk center.
Detected by halocme, Submitted at 2016-03-24T04:29:47
2016-03-23T02:00:06 --> 2016-03-23T05:00:06
Coronal dimming suggesting a slow rising motion of coronal structures long preceded the eruptive C1.1 flare from AR 12524. As was expected from these EUV images, the associated CME was largely seen toward north.
Detected by halocme, Submitted at 2016-03-24T04:29:46
2016-03-23T02:00:06 --> 2016-03-23T05:00:06
Coronal dimming suggesting a slow rising motion of coronal structures long preceded the eruptive C1.1 flare from AR 12524. As was expected from these EUV images, the associated CME was largely seen toward north.
Detected by halocme, Submitted at 2016-03-24T04:29:45
2016-03-23T02:00:06 --> 2016-03-23T05:00:06
Coronal dimming suggesting a slow rising motion of coronal structures long preceded the eruptive C1.1 flare from AR 12524. As was expected from these EUV images, the associated CME was largely seen toward north.
Detected by halocme, Submitted at 2016-03-24T04:21:30
2016-03-19T21:10:10 --> 2016-03-19T22:50:10
This is a filament eruption outside active regions. No X-ray flare was associated with it, but there is clear two-ribbon emission in 304 A images.
Detected by Paul Bryans, Submitted at 2016-03-23T16:19:41
2016-03-11T20:38:38 --> 2016-03-11T21:15:00
There is a jet-like surge near the end of the observation at the extreme top of the slit. The slit has passed by the time of the eruption but catches the end of it.
Detected by Paul Bryans, Submitted at 2016-03-23T16:13:56
2016-03-10T04:19:33 --> 2016-03-10T07:49:09
Coordinated observations with EIS. O IV lines in 1395-1405 A range are visible towards the bottom third of the slit position.
Detected by Paul Bryans, Submitted at 2016-04-18T20:57:22
2016-03-10T02:54:33 --> 2016-03-10T03:01:07
Coronal rain observations coordinated with HINODE/EIS. First look at the spectra shows the O IV lines to be fairly bright at certain times (one goal of the study was to measure these lines).
Detected by Paul Bryans, Submitted at 2016-03-23T04:28:47
2016-03-10T12:59:09 --> 2016-03-10T15:58:51
Coronal rain at east limb. Looks like the dust buster is not doing a great job here.
Detected by schryver, Submitted at 2016-03-22T23:32:46
2016-03-21T23:16:06 --> 2016-03-22T02:12:06
A coronal propagating front emanates from a very compact, small bipole at one scale length from the nearby sizeable AR with a nonpotential swirl in the loops from its leading spot. The wave and reflections extend over in excess of 0.5Rsun from the site into quiet Sun.
