Recent Events Reported by Observers
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Detected by Patricia Jibben, Submitted at 2018-01-08T14:49:18
2017-12-30T01:47:38 --> 2017-12-30T01:59:54
The base of the jet stays bright in both 1330 and 1400. When the slit nears the limb, the jet leaves the bright base.
Detected by Patricia Jibben, Submitted at 2018-01-08T14:42:24
2017-12-29T18:48:44 --> 2017-12-29T19:01:00
This minor brightening occurs on the limb and is best seen in 1330 and 1400. There is corresponding movement in 2796 but it the feature is not as bright. This event is not a GOES event.
Detected by halocme, Submitted at 2018-01-05T18:10:09
2018-01-03T22:55:13 --> 2018-01-04T01:31:13
Essentially a repeat of the earlier event during 3 Jan 2018 09:00-10:40.
Detected by halocme, Submitted at 2018-01-05T18:04:51
2018-01-03T09:00:02 --> 2018-01-03T10:40:02
A mini filament eruption occurred in the northern part of the region which later became AR 12693 (during 4 Jan 2018 with a 20 MSH sunspot). In addiion to the post-eruption arcade, this eruption disturbed another region to the northeast, which may have been already magnetically connected.
Detected by halocme, Submitted at 2018-01-05T17:52:59
2018-01-02T22:20:25 --> 2018-01-03T02:20:25
This event looks like a confined eruption in 304 A images alone, but a flux-rope-like structure may be traced to the edge of the AIA field of view, deflected to southwest.
Detected by halocme, Submitted at 2018-01-05T17:41:52
2018-01-02T08:15:01 --> 2018-01-02T12:45:01
It appears that an outflow of cool material leads to slow reconfiguration of overlying coronal field as traced in 171 A images (but not 211 A). There was no indication that this structure later erupted.
Detected by halocme, Submitted at 2018-01-05T17:21:03
2018-01-01T21:40:13 --> 2018-01-01T23:40:13
This was likely from a region slighly occulted. Cool material fell back but material with coronal temperature seemed to be ejected, producing weak dimming.
Detected by halocme, Submitted at 2018-01-05T17:13:40
2018-01-01T16:00:09 --> 2018-01-01T17:50:33
Eruption of cool material seen against hot coronal background. It was likely from backside. The corona at high altitudes slightly dimmed. This eruption may give a false impreession of being stuck. This was due to missing frames in PRGB (all science data are unaffected).
Detected by halocme, Submitted at 2017-12-31T22:46:45
2017-12-31T14:30:01 --> 2017-12-31T15:15:37
Miniature sigmoid eruption.
Detected by halocme, Submitted at 2017-12-31T22:42:43
2017-12-30T19:20:25 --> 2017-12-30T20:20:25
The eruption was largely horizontal. In difference images, it looks like a jet.
Detected by halocme, Submitted at 2017-12-31T22:37:14
2017-12-29T11:30:01 --> 2017-12-29T13:10:01
An eruption, initially looking like a flux rope. This probably became an unimpressive CME (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171229.132545.w025.v0226.p302&frame=10&r)
Detected by halocme, Submitted at 2017-12-31T22:28:39
2017-12-28T22:20:25 --> 2017-12-28T23:09:37
The B8.3 flare was an isolated event. The wave propagted along the limb. The associated CME was not impressive (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171228.223607.w029.v0440.p103&frame=10&r).
Detected by halocme, Submitted at 2017-12-31T22:23:09
2017-12-27T22:45:01 --> 2017-12-27T23:35:25
A mini filament eruption led first to a jet and then to a more extended but still narrow eruption, to be observed by LASCO (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171228.002407.w011.v0193.p266&frame=3&r).
Detected by halocme, Submitted at 2017-12-31T22:16:24
2017-12-27T06:45:01 --> 2017-12-27T07:45:01
A small eruption and post-eruption arcade in a quiescent region.
Detected by halocme, Submitted at 2017-12-31T22:12:05
2017-12-27T04:40:13 --> 2017-12-27T05:21:01
Cool material was seen to be ejected horizontally as the jet started. The jet was then deflected to west by adjacent coronal structures. There was contemporaneous smaller jet activity east of this jet.
Detected by halocme, Submitted at 2017-12-31T22:06:13
2017-12-26T01:00:09 --> 2017-12-26T01:30:09
It appears that helical motions were involved in the initial stage.
Detected by halocme, Submitted at 2017-12-23T11:18:04
2017-12-23T06:30:01 --> 2017-12-23T07:20:25
An impressive jet that can be traced to the edge of the AIA FOV.
Detected by halocme, Submitted at 2017-12-23T11:04:44
2017-12-19T12:00:09 --> 2017-12-23T08:00:09
The region started to show sunspots on 20 December, although HMI data had revealed strong magnetic field more than a day earlier. The region has changed appearance since, even though the total sunspot area remains 70 msh and no significant eruptive activity has been seen (as of 23 December AM).
Detected by halocme, Submitted at 2017-12-23T10:41:18
2017-12-21T19:30:01 --> 2017-12-21T20:40:49
The eruption occurred in a region that was bright in EUV images but was not given a NOAA AR number because there were no spots. The eruption seems to have hit AR 12692 to the east, also producing dimming regions.
Detected by halocme, Submitted at 2017-12-23T10:41:17
2017-12-21T19:30:01 --> 2017-12-21T20:40:49
The eruption occurred in a region that was bright in EUV images but was not given a NOAA AR number because there were no spots. The eruption seems to have hit AR 12692 to the east, also producing dimming regions.