Recent Events Reported by Observers
Previous Next
Detected by Lucas Guliano, Submitted at 2025-05-05T15:40:09
2025-05-03T14:36:27 --> 2025-05-03T15:11:18
High cadence observation of a flare in the corner of the FOV
Detected by Lucas Guliano, Submitted at 2025-05-05T15:33:57
2025-05-02T20:49:27 --> 2025-05-02T21:56:57
Short flash in the bottom corner of the FOV
Detected by Lucas Guliano, Submitted at 2025-05-05T15:29:34
2025-05-02T12:39:19 --> 2025-05-02T13:11:22
Short ribbon flare partially under the slit
Detected by Lucas Guliano, Submitted at 2025-05-05T15:19:16
2025-04-29T19:24:19 --> 2025-04-30T00:27:41
Prominent oscillatory waves from the center of a sunspot.
Detected by Navdeep Panesar, Submitted at 2025-04-10T18:34:45
2025-04-07T03:48:05 --> 2025-04-08T22:55:05
Evolution of group of filaments that appear on south-east solar limb.
Detected by Navdeep Panesar, Submitted at 2025-04-10T18:32:33
2025-04-05T10:26:42 --> 2025-04-06T09:26:42
Evolution of a quiescent prominence.
Detected by Navdeep Panesar, Submitted at 2025-04-10T18:31:05
2025-04-03T23:10:17 --> 2025-04-04T06:22:41
Quiet region jet is driven by a small-scale filament eruption. There is flux cancellation goes on at the neutral line that trigger the eruption.
Detected by Navdeep Panesar, Submitted at 2025-04-10T18:28:49
2025-04-03T17:56:30 --> 2025-04-04T01:24:54
Coronal active region occurs at cancelling neutral line.
Detected by Navdeep Panesar, Submitted at 2025-04-10T18:26:28
2025-04-02T23:44:42 --> 2025-04-03T06:57:06
Active region jet is triggered by flux cancellation.
Detected by Navdeep Panesar, Submitted at 2025-04-10T18:24:13
2025-04-04T14:45:17 --> 2025-04-05T05:16:05
A quiescent filament erupts from a weak magnetic neutral line. Brightenings appear underneath the erupting filament.
Detected by Navdeep Panesar, Submitted at 2025-04-10T18:20:16
2025-04-03T22:41:34 --> 2025-04-04T19:20:34
Evolution of a prominence-filament system
Detected by Navdeep Panesar, Submitted at 2025-04-10T18:19:00
2025-04-03T09:40:22 --> 2025-04-04T13:31:34
Evolution solar plumes
Detected by Navdeep Panesar, Submitted at 2025-04-10T18:11:26
2025-04-05T14:10:53 --> 2025-04-05T23:21:29
M-class flare from active region NOAA 14045
Detected by Navdeep Panesar, Submitted at 2025-04-10T18:09:10
2025-04-02T10:46:41 --> 2025-04-03T03:09:41
Active region NOAA 14045 produced multiple C-class flares and one M-class flare.
Detected by Catharine Bunn, Submitted at 2025-03-14T21:07:31
2025-02-25T04:42:19 --> 2025-02-25T04:50:15
A C5.9 flare from AR 13998.
Detected by Chad Madsen, Submitted at 2025-03-14T20:02:33
2025-03-07T09:27:10 --> 2025-03-07T10:48:58
A GOES C1.6 flare in the PIL region of AR14012. The flare is preceded by a number of less intense brightenings occurring in the location.
Detected by Chad Madsen, Submitted at 2025-03-14T19:50:55
2025-03-06T13:10:16 --> 2025-03-06T17:18:52
A peacock tail in the emerging AR14016 displaying an unusual degree of morphological evolution. The base of the peacock tail brightens as the undulating elements of the tail arc outward to form a loop that connects to an opposite polarity region.
Detected by Chad Madsen, Submitted at 2025-03-14T19:44:45
2025-03-04T16:08:05 --> 2025-03-04T16:33:08
A GOES C3.9 Flare in the PIL region of AR14012 featuring an extended serpentine ribbon.
Detected by Chad Madsen, Submitted at 2025-03-14T19:39:15
2025-03-04T10:18:03 --> 2025-03-04T10:36:16
A GOES C1.8 flare in the PIL region of AR14012 displaying a compact yet serpentine ribbon.
Detected by Chad Madsen, Submitted at 2025-02-26T18:50:33
2025-02-12T20:01:49 --> 2025-02-12T20:20:37
A GOES C1.7 flare in AR13990 producing a compact, serpentine ribbon.
