Recent Events Reported by Observers
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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.
Detected by Chad Madsen, Submitted at 2025-02-26T18:46:24
2025-02-11T23:54:36 --> 2025-02-12T01:22:48
A small arcade of loops of condensing material over AR13981 on the west limb.
Detected by Chad Madsen, Submitted at 2025-02-26T18:42:39
2025-02-11T14:53:58 --> 2025-02-11T15:39:15
Following a GOES C7.6 flare in AR13981, multiple arch-shaped strands of down-flowing condensed material appear over the west limb.
Detected by Lucas Guliano, Submitted at 2025-02-26T17:25:06
2025-02-24T20:52:19 --> 2025-02-24T21:17:37
Bright and quick flash of complex structure of flare ribbons from M class flare, not under the slit
Detected by Lucas Guliano, Submitted at 2025-02-26T17:06:48
2025-02-21T02:08:15 --> 2025-02-21T02:29:36
High Cadence observation of C3.8 flare, flare starts outside the FOV and then results in a ribbon flash and some flowing material across the slit
Detected by Lucas Guliano, Submitted at 2025-02-26T16:57:59
2025-02-20T02:38:01 --> 2025-02-20T02:50:14
High cadence observation of C1.5 flare, small bright ribbons, main activity missed by the slit
Detected by Lucas Guliano, Submitted at 2025-02-26T16:48:20
2025-02-19T14:43:08 --> 2025-02-19T17:18:17
Small amounts of coronal rain from AR at the limb
Detected by Navdeep Panesar, Submitted at 2025-02-24T22:53:53
2025-01-09T06:31:30 --> 2025-01-09T18:15:54
C-class flare occur from NOAA AR 13947, which leads to the coronal dimming. Flare ribbons appear all along the neutral line.
Detected by Navdeep Panesar, Submitted at 2025-02-24T19:54:13
2025-01-11T16:22:05 --> 2025-01-11T23:24:41
Coronal hole jet is driven by the minifilament eruption. That minifilament eruption is triggered by flux cancellation.
Detected by Navdeep Panesar, Submitted at 2025-02-24T19:51:13
2025-01-12T11:34:46 --> 2025-01-14T22:55:10
Evolution of on-disk coronal plumes that are rooted at the negative-polarity magnetic flux patch.
