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Recent Events Reported by Observers

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Detected by Roy Smart, Submitted at 2019-04-29T19:27:50
2019-04-18T14:06:57 --> 2019-04-18T14:18:34
Another example of a repeated microflare in on the north edge of the sunspot in AR12738.

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Detected by Roy Smart, Submitted at 2019-04-29T17:08:57
2019-04-17T23:57:52 --> 2019-04-18T00:16:32
A long-exposure example of the repeated microflare site on the south side of the sunspot in AR12738

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Detected by Roy Smart, Submitted at 2019-04-29T15:45:30
2019-04-16T14:16:10 --> 2019-04-16T14:26:35
One example of a recurring microflare on the north side of the sunspot in AR12738

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Detected by halocme, Submitted at 2019-04-29T00:03:18
2019-04-18T10:30:01 --> 2019-04-18T11:15:37
The northwestern part og AR 12738 also abounded in narrow outflows. These may be jets but look also like blobs that may represent plasmoids.

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Detected by halocme, Submitted at 2019-04-28T23:54:17
2019-04-17T21:55:13 --> 2019-04-18T00:50:25
This is another example of a jet period seen at the southwestern part of the sunspot of AR 12738

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Detected by halocme, Submitted at 2019-04-28T23:47:07
2019-04-17T08:15:01 --> 2019-04-17T08:59:25
The jet southward was seen multiple times from the western part of the big spot of AR 12738, probably reflecting long-lived coronal structures incluidng open field lines.

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Detected by Roy Smart, Submitted at 2019-04-28T21:18:33
2019-04-16T04:50:55 --> 2019-04-16T04:58:51
Microflare in the prenumbra of the sunspot in AR12738

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Detected by halocme, Submitted at 2019-04-26T06:41:26
2019-04-17T00:00:09 --> 2019-04-21T00:00:09
A rather simple active region, which was only 20 msh at maximum. No flares. But Dibyendu Nandi seemed to like it. See https://twitter.com/ydnadydnad/status/1118900920387944448. ?

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Detected by mkocher, Submitted at 2019-04-25T22:34:19
2019-03-09T12:10:09 --> 2019-03-09T14:50:09
Active Region filament matured into a brilliant eruption, close to the disk center in the North Western hemisphere of the Sun. This eruption is also observed in STEREO A.

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Detected by Vanessa Polito, Submitted at 2019-04-24T17:58:03
2019-04-13T06:54:24 --> 2019-04-13T07:51:33
Several bright points in AR 12738, very large emission lines. Possibly UV bursts

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Detected by Vanessa Polito, Submitted at 2019-04-24T17:54:31
2019-04-13T02:13:47 --> 2019-04-13T02:48:40
IRIS observes ribbon emission associated with a small B class flare

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Detected by Vanessa Polito, Submitted at 2019-04-24T17:48:13
2019-04-12T11:27:00 --> 2019-04-12T11:53:55
Filament eruption -associated B class flare in GOES

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Detected by Vanessa Polito, Submitted at 2019-04-24T17:45:00
2019-04-10T16:45:05 --> 2019-04-10T17:00:09
Filament eruption, B-class flare in GOES plots at the same time

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Detected by Vanessa Polito, Submitted at 2019-04-24T17:36:14
2019-04-09T17:56:42 --> 2019-04-09T18:17:47
Flows in AR 12738, possibly coronal rain or filament

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Detected by Vanessa Polito, Submitted at 2019-04-23T17:27:31
2019-04-10T22:04:20 --> 2019-04-10T22:17:36
Observation of spicules and a spray surge on the west limb, covered by IRIS slit.

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Detected by Tiago Pereira, Submitted at 2019-04-10T14:49:02
2019-03-23T09:22:14 --> 2019-03-23T11:21:43
Several recurrent eruptive jets on AR 12736. Maybe small flares?

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Detected by Arkadiusz Berlicki, Submitted at 2019-04-10T14:47:36
2019-03-28T08:27:26 --> 2019-03-28T10:24:49
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.

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Detected by Tiago Pereira, Submitted at 2019-04-10T14:35:39
2019-03-22T21:38:58 --> 2019-03-23T00:02:41
Several B-class flares and other eruptions/jets taking place on AR 12736 as it approaches the limb.

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Detected by Tiago Pereira, Submitted at 2019-04-10T14:28:53
2019-03-22T12:40:44 --> 2019-03-22T15:46:29
Several B-class flares occur in quick succession on the same region of AR 12736.

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Detected by Krzysztof Barczynski, Submitted at 2019-04-09T14:53:28
2019-03-08T14:08:24 --> 2019-03-08T14:25:02
An eruption of the material in AR 12376. The erupted material is significantly broader than typical jet.

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