Recent Events Reported by Observers
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Detected by Jacob Parker, Submitted at 2019-06-14T21:59:13
2019-05-30T02:53:50 --> 2019-05-30T03:07:43
Both a prominence off the east limb and part of small filament were captured via a large dense raster. This OBS was run twice, each with a few repeats, throughout the day.
Detected by Jacob Parker, Submitted at 2019-06-14T21:42:21
2019-05-29T05:05:21 --> 2019-05-29T05:13:48
This small region of emerging flux came and went in a couple days and produced multiple explosive events.
Detected by halocme, Submitted at 2019-05-29T07:07:16
2019-05-25T21:15:01 --> 2019-05-25T23:01:01
The eruption occurred in what could be considered a coronal bright point (although it was largish). The area south of the region dimmed temporarily.
Detected by halocme, Submitted at 2019-05-29T07:00:57
2019-05-25T06:45:01 --> 2019-05-25T09:45:01
A slow, plasmoid- or flux-rope-like eruption was seen exclusively in 171 A images. The ejecta was seen to deflected toward the equator.
Detected by halocme, Submitted at 2019-05-29T06:55:34
2019-05-25T05:05:25 --> 2019-05-25T06:45:25
The eruption likely occurred on the backside. It appeared to trigger another one to the north on the visible side.
Detected by halocme, Submitted at 2019-05-29T06:49:16
2019-05-23T06:40:13 --> 2019-05-23T07:30:37
This jet contains cool material initially ejected in helical motions.
Detected by halocme, Submitted at 2019-05-29T06:42:57
2019-05-23T04:20:25 --> 2019-05-24T05:50:25
A bipolar region hosted what looked like a coronal bright point in full-disk images. It lasted a few days. Its appearance traced the evolution of the underlying magnetic field structure.
Detected by halocme, Submitted at 2019-05-29T06:29:45
2019-05-22T12:45:01 --> 2019-05-22T14:01:01
A tiny eruption, causing the overlying structure to slightly dim.
Detected by halocme, Submitted at 2019-05-29T06:24:57
2019-05-22T07:15:01 --> 2019-05-22T11:15:01
This eruption was very diffuse and seen only in 171 A images. An ourflow seemed to precede a more localized filament eruption, which accelerated the eruption of a closed coronal structure. The eruption was deflected clockwise.
Detected by halocme, Submitted at 2019-05-29T06:17:15
2019-05-21T06:45:01 --> 2019-05-21T09:01:01
The coronal structure overlying AR 12741 was seen to gradually open up and dim, even though eruption itself was not clearly seen. This was associated with a CME (http://spaceweather.gmu.edu/seeds/mkmovie_ql.php?cme=20190521.083607.w041.v0323.p248&frame=12).
Detected by halocme, Submitted at 2019-05-29T06:11:01
2019-05-21T04:00:09 --> 2019-05-21T06:10:09
Low-lying filament activity around AR 12741 seemed to cause a minor eruption, which did not go beyond the AIA field of view, hence no CME.
Detected by halocme, Submitted at 2019-05-29T05:58:30
2019-05-20T13:35:25 --> 2019-05-20T14:25:25
This looked like a narrow eruption, different from a flux rope eruption (CME), but it started impulsively, causing the overlying structure to oscillate.
Detected by halocme, Submitted at 2019-05-29T05:58:30
2019-05-20T13:35:25 --> 2019-05-20T14:25:25
This looked like a narrow eruption, different from a flux rope eruption (CME), but it started impulsively, causing the overlying structure to oscillate.
Detected by halocme, Submitted at 2019-05-29T05:47:11
2019-05-19T21:00:33 --> 2019-05-19T21:50:33
This was probably a confined eruption, but the overlying structure was seen to be disturbed.
Detected by halocme, Submitted at 2019-05-29T05:32:34
2019-05-19T15:55:13 --> 2019-05-19T17:31:13
Evem though this was on a relatively small scale, it was probably an eruption of a flux rope, seen in dark to the north of the region in projection. A surge followed the eruption, propagating in SWW.
Detected by halocme, Submitted at 2019-05-29T05:32:33
2019-05-19T15:55:13 --> 2019-05-19T17:31:13
Evem though this was on a relatively small scale, it was probably an eruption of a flux rope, seen in dark to the north of the region in projection. A surge followed the eruption, propagating in SWW.
Detected by halocme, Submitted at 2019-05-29T05:22:51
2019-05-18T15:30:01 --> 2019-05-18T16:40:49
This happened in a quiescent region. The wave propagated preferentially in the northwestern direction. No flare was seen above the ~A8 beckground level.
Detected by halocme, Submitted at 2019-05-29T05:13:55
2019-05-18T10:15:01 --> 2019-05-18T13:11:01
Large-scale structure overlying AR 12741 is seen to gradually open up. This may be related to the slow CME observed around 12:00 (http://spaceweather.gmu.edu/seeds/mkmovie_ql.php?cme=20190518.120007.w041.v0170.p256&frame=19).
Detected by halocme, Submitted at 2019-05-29T05:06:25
2019-05-17T06:15:01 --> 2019-05-17T07:35:01
A small filament erupted, but it had far-reaching effects high in the corona for the outflow to be visible over the limb.
Detected by Roy Smart, Submitted at 2019-05-28T03:33:22
2019-01-21T10:13:10 --> 2019-01-21T11:18:06
Flux emerging into plage region
