Recent Events Reported by Observers
Previous Next
Detected by Alexander Pietrow, Submitted at 2023-12-14T20:00:10
2023-12-13T19:29:11 --> 2023-12-13T19:29:11
Small flare partially in slit
Detected by Alexander Pietrow, Submitted at 2023-12-14T19:57:35
2023-12-13T11:38:47 --> 2023-12-13T11:38:47
Eruption in slit
Detected by Alexander Pietrow, Submitted at 2023-12-14T12:37:45
2023-12-13T08:16:55 --> 2023-12-13T08:16:55
In slit
Detected by Alexander Pietrow, Submitted at 2023-12-14T12:36:15
2023-12-13T06:33:26 --> 2023-12-13T06:36:13
microflare in slit
Detected by Alexander Pietrow, Submitted at 2023-12-14T09:33:40
2023-12-12T22:29:44 --> 2023-12-12T22:29:44
B2 flare partially in slit
Detected by Alexander Pietrow, Submitted at 2023-12-14T09:31:24
2023-12-12T21:13:20 --> 2023-12-12T21:21:18
Eruption in slit
Detected by Alexander Pietrow, Submitted at 2023-12-14T09:28:55
2023-12-12T15:54:52 --> 2023-12-12T16:01:00
In slit High cad
Detected by Alexander Pietrow, Submitted at 2023-12-14T09:26:18
2023-12-12T19:12:21 --> 2023-12-12T19:22:40
Not in slit
Detected by Alexander Pietrow, Submitted at 2023-12-14T09:20:06
2023-12-12T12:36:00 --> 2023-12-12T12:46:16
Small flare, not in slit, High cad
Detected by Alexander Pietrow, Submitted at 2023-12-14T09:15:34
2023-12-12T11:02:22 --> 2023-12-12T11:03:32
Non slit flare
Detected by Alexander Pietrow, Submitted at 2023-12-14T09:11:40
2023-12-12T09:57:02 --> 2023-12-12T09:58:32
Microflare in slit
Detected by Alexander Pietrow, Submitted at 2023-12-14T09:10:27
2023-12-12T09:35:51 --> 2023-12-12T09:42:28
Jet in slit
Detected by Chad Madsen, Submitted at 2023-12-04T23:08:31
2023-11-28T00:00:00 --> 2023-11-28T00:43:14
An eruption of a small filament near the polarity inversion line of the decayed AR13489. The eruption appears to begin near the south-central region of the SJI field of view. The eruption corresponds with a number of brightenings in the FUV passbands along the thin, dark channel running from the south-central portion to the northwest portion of the SJI field of view.
Detected by Chad Madsen, Submitted at 2023-12-04T23:01:58
2023-11-27T05:53:35 --> 2023-11-27T06:52:01
A large erupting filament near the polarity inversion line of the decayed AR13489. The erupting filament fans out across much of the SJI field of view. Some material appears to return to the Sun toward the northeast corner of the SJI field of view while the remainder appears to escape outward.
Detected by Chad Madsen, Submitted at 2023-12-04T22:53:06
2023-11-24T05:32:27 --> 2023-11-24T05:53:29
A GOES C3.3 flare in AR13492 featuring a hook-shaped flare ribbon. The ribbon scar persists for the next few orbits and is host to a number of smaller-scale brightenings.
Detected by Aparna Venkataramanasastry, Submitted at 2023-11-28T07:25:10
2023-08-22T06:23:18 --> 2023-08-22T17:13:18
A small flare followed by an eruption is observed, the eruption is mainly cool dark material falling back on to the disk similar to coronal rain. Cancellation of opposite polarities are observed in HMI LOS at the location of the flare.
Detected by Aparna Venkataramanasastry, Submitted at 2023-11-28T07:04:13
2023-08-21T22:00:42 --> 2023-08-22T07:37:06
A flux rope like structure forms and a jet like eruption is seen with one end of the structure still connected to the Sun.
Detected by Aparna Venkataramanasastry, Submitted at 2023-11-27T07:44:46
2023-08-22T15:14:54 --> 2023-08-23T18:15:06
Flare ribbons in a circular pattern with possible flare in the center is observed. 171A shows loop brightening from the center towards the footpoints.
Detected by Aparna Venkataramanasastry, Submitted at 2023-11-27T07:23:15
2023-08-21T13:57:17 --> 2023-08-22T08:31:29
Small flare loops occur along with an explosive eruption from the same active region, around the same time but not the same location. The explosive material has a helical structure to it.
Detected by Meng Jin, Submitted at 2023-11-23T00:46:32
2023-03-22T17:12:35 --> 2023-03-23T10:49:11
An eruption was observed from AR 13257. The pre-existing coronal structures are significant disturbed, likely due to the reconnection between the flux rope and the strapping field.
