Recent Events Reported by Observers
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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
Detected by Navdeep Panesar, Submitted at 2023-11-09T11:44:01
2023-05-14T21:42:18 --> 2023-05-17T01:40:54
Evolution of an intermediate filament, whose one foot is rooted in the active region and other foot is away from the active region.
Detected by Navdeep Panesar, Submitted at 2023-11-09T11:41:00
2023-05-14T00:02:22 --> 2023-05-15T15:50:58
Evolution of on disk solar plumes
Detected by Navdeep Panesar, Submitted at 2023-11-09T11:38:10
2023-05-14T00:02:22 --> 2023-05-15T07:31:22
A quiescent prominence can be seen on SW solar limb along with a coronal cavity.
Detected by Q. M. Wargnier, Submitted at 2023-11-01T21:26:00
2023-10-30T22:56:02 --> 2023-10-30T23:16:11
Flares are emerging on the left side of this active region.
Detected by Q. M. Wargnier, Submitted at 2023-11-01T20:50:14
2023-10-28T05:28:56 --> 2023-10-28T05:43:43
A solar flare was observed during the coordination of the SPICE solar orbiter. The observation was part of a large raster.
Detected by Q. M. Wargnier, Submitted at 2023-11-01T20:05:04
2023-10-29T22:28:41 --> 2023-10-29T22:56:46
A sequence of brightenings occurred within the loop structure, and these brightenings are correlated with solar flares.
Detected by Navdeep Panesar, Submitted at 2023-10-28T11:24:05
2023-03-12T00:03:06 --> 2023-03-12T09:20:18
An evolution active region prominence
Detected by Navdeep Panesar, Submitted at 2023-10-28T11:20:17
2023-03-16T21:33:35 --> 2023-03-17T17:56:35
Active region filament erupts
Detected by Navdeep Panesar, Submitted at 2023-10-28T11:17:46
2023-03-12T00:03:11 --> 2023-03-13T07:19:23
A filament eruptions and flare arcade appears all along the neutral line
