Recent Events Reported by Observers
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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.
Detected by Meng Jin, Submitted at 2023-11-23T00:39:43
2023-03-24T16:58:10 --> 2023-03-25T08:07:22
A series of eruptions occurred from different active regions on disk. There are possible magnetic connections among the eruptions.
Detected by Meng Jin, Submitted at 2023-11-22T23:03:14
2023-03-21T09:05:10 --> 2023-03-21T23:23:10
Synchronous eruptions are observed near the disk center and at the west limb. The west limb eruption results in large-scale coronal disturbance.
Detected by Meng Jin, Submitted at 2023-11-22T22:54:03
2023-03-19T22:43:10 --> 2023-03-20T12:51:34
Weak coronal waves are seen in the southern hemisphere, which might link to the activities from a small flux emergence region.
Detected by Meng Jin, Submitted at 2023-11-22T22:44:17
2023-03-18T23:59:10 --> 2023-03-19T07:40:10
Several confined eruptions / loop activities are observed at the east limb. At the end, some coronal material is released away from the Sun.
Detected by Meng Jin, Submitted at 2023-11-22T03:27:32
2023-02-01T00:00:46 --> 2023-02-01T12:20:22
A filament eruption near the west limb was observed. The filament activation first showed on disk, followed by large-scale coronal structures near the limb.
Detected by Meng Jin, Submitted at 2023-11-22T03:15:41
2023-01-29T06:38:46 --> 2023-01-29T15:04:34
A filament eruption near the east limb. The eruption seems to change the field configurations and bright loop structures formed following the eruption.
Detected by Meng Jin, Submitted at 2023-11-22T03:01:58
2023-01-30T17:16:29 --> 2023-01-31T08:11:05
A large-scale brightening near the northern polar region is observed, which might be triggered by a filament eruption near the west limb.
Detected by Meng Jin, Submitted at 2023-11-22T02:44:24
2023-01-29T17:02:58 --> 2023-01-30T04:50:34
Sympathetic eruptions are observed from AR 13192 and 13191. The first eruption started at 13192 with flare ribbons. Some brightenings are evident at the edge of the AR 13191 before the second eruption initiated.
Detected by Navdeep Panesar, Submitted at 2023-11-09T17:53:59
2023-05-16T03:41:42 --> 2023-05-19T01:36:06
Evolution of a prominence-filament system
Detected by Navdeep Panesar, Submitted at 2023-11-09T11:49:56
2023-05-17T05:50:30 --> 2023-05-18T06:23:18
Eruption of a polar crown filament
Detected by Navdeep Panesar, Submitted at 2023-11-09T11:46:30
2023-05-17T10:13:06 --> 2023-05-18T23:02:18
Eruption of an on disk filament
