Recent Events Reported by Observers
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Detected by Chad Madsen, Submitted at 2018-05-25T20:11:36
2018-05-24T09:33:41 --> 2018-05-24T11:00:10
Compact, transient brightenings near the leading sunspot of AR 12711.
Detected by Chad Madsen, Submitted at 2018-05-24T21:34:25
2018-05-23T19:59:46 --> 2018-05-23T20:47:33
Compact, transient brightenings in the low-lying loops near the leading sunspot of the recently emerged AR 12711.
Detected by Chad Madsen, Submitted at 2018-05-24T21:32:37
2018-05-23T19:06:07 --> 2018-05-23T19:39:01
Compact, transient brightenings in the low-lying loops near the leading sunspot of the recently emerged AR 12711
Detected by Chad Madsen, Submitted at 2020-08-03T18:30:13
2018-05-23T18:28:33 --> 2018-05-23T18:55:58
Compact, transient brightenings in the low-lying loops near the leading sunspot of the recently emerged AR 12711.
Detected by Chad Madsen, Submitted at 2018-05-24T21:27:18
2018-05-23T15:39:10 --> 2018-05-23T16:12:04
Compact, transient brightenings in the low-lying loops near the leading sunspot of the recently emerged AR 12711.
Detected by Chad Madsen, Submitted at 2018-05-24T21:25:31
2018-05-23T15:01:36 --> 2018-05-23T15:29:01
Compact, transient brightenings in the low-lying loops near the leading sunspot of the recently emerged AR 12711.
Detected by Chad Madsen, Submitted at 2018-05-24T21:19:23
2018-05-23T08:00:35 --> 2018-05-23T08:06:39
A small, weak B1.7 flare with a arch-like ribbon in AR 12710.
Detected by Chad Madsen, Submitted at 2018-05-24T21:09:23
2018-05-23T06:58:03 --> 2018-05-23T07:09:47
A narrow stream of erupting material from the northernmost regions of AR 12710. The eruption stream appears to be twisted with irregular brightenings throughout.
Detected by Chad Madsen, Submitted at 2018-05-24T21:02:25
2018-05-23T00:36:53 --> 2018-05-23T01:04:18
Compact, transient brightenings in the low-lying loop structure of the recently emerged AR 12711.
Detected by Chad Madsen, Submitted at 2018-05-24T20:57:31
2018-05-22T19:38:46 --> 2018-05-22T20:44:54
Compact, transient brightenings in the low-lying loop structure of the newly emerged AR 12711.
Detected by Chad Madsen, Submitted at 2018-05-24T20:54:51
2018-05-22T18:44:27 --> 2018-05-22T19:17:21
Compact, transient brightenings in the low-lying loop structure of the newly emerged AR 12711.
Detected by Chad Madsen, Submitted at 2018-05-24T20:51:38
2018-05-22T18:06:37 --> 2018-05-22T18:34:03
Compact, transient brightenings apparent in amongst the low-lying hot loops structure of the recently emerged AR 12711.
Detected by Chad Madsen, Submitted at 2018-05-24T20:46:26
2018-05-22T13:58:33 --> 2018-05-22T14:15:11
A serendipitous observation of the initial emergence of AR 12711 which appeared near a filament footprint in a decayed plage region. The dramatic, explosive birth of this active region occurs at the tail end of the observation.
Detected by Chad Madsen, Submitted at 2018-05-24T20:41:11
2018-05-22T08:27:37 --> 2018-05-22T08:36:14
A broad, brief jet emanating from a localized brightening in a QS network patch.
Detected by halocme, Submitted at 2018-05-18T19:09:16
2018-05-18T02:00:09 --> 2018-05-18T06:00:09
A minor prominence eruption precedes the formation of a larger front that slowly moves away from the Sun. This front is nearly exclusively seen in 171 A images (i.e. not 211 A), suggesting that it is rather cool. Such eruptions may be easily overlooked because they are diffuse, but they may take place not too infrequently. The associated CME is https://cdaw.gsfc.nasa.gov/movie/make_javamovie.php?img1=lasc2rdf&img2=goesx&stime=20180518_0200&etime=20180518_1000.
Detected by halocme, Submitted at 2018-05-18T17:32:20
2018-05-17T23:16:13 --> 2018-05-17T23:40:13
This eruption shows a nice three-part structure, the front loop, cavity and core (that corresponds to the prominence). But the associated CME is disappointingly minor (https://cdaw.gsfc.nasa.gov/movie/make_javamovie.php?img1=lasc2rdf&img2=goesx&stime=20180517_2230&etime=20180518_0100).
Detected by halocme, Submitted at 2018-05-18T05:02:55
2018-05-17T20:20:25 --> 2018-05-17T21:00:01
This looks like a normal jet in the sense that the moving linear structure is seen in coronal temperatures. A mini filament is also present as seen in absorption in 304 A images.
Detected by halocme, Submitted at 2018-05-18T04:41:38
2018-05-17T08:50:25 --> 2018-05-17T10:06:01
Progressively southeastern coronal base brightened before a linear (slightly curved) structure in the corona brightens. The brightening does not seem to propagate in altitudes, but large-scale loops appear to brighten nearly simultaneously,
Detected by halocme, Submitted at 2018-05-18T04:15:11
2018-05-16T13:45:01 --> 2018-05-16T14:45:01
As the mini filament erupts with clockwise motions, a linear structure brightens and also moves northward, assuming a jet-like structure. The associated heating appears to be at a low level, since the brightening does not reach coronal temperatures that should be captured in 171 A and 211 A images.
Detected by halocme, Submitted at 2018-05-18T04:05:04
2018-05-15T14:00:09 --> 2018-05-15T15:00:09
Two coronal bases eject material in absorption and brighten. It is not clear whether they represent one jet or two jets.
