Recent Events Reported by Observers
Previous Next
Detected by Navdeep Panesar, Submitted at 2025-07-09T18:15:22
2025-05-08T15:57:18 --> 2025-05-10T09:37:54
A small-scale prominence appears on the SW solar limb that slowly erupts
Detected by Navdeep Panesar, Submitted at 2025-07-09T18:13:35
2025-05-08T06:14:34 --> 2025-05-08T20:00:34
Evolution solar plumes that are rooted on the unipolar magnetic field regions
Detected by Navdeep Panesar, Submitted at 2025-07-09T18:10:49
2025-05-08T17:01:22 --> 2025-05-08T19:50:58
A quiet region coronal jet resides above magnetic neutral line.
Detected by Navdeep Panesar, Submitted at 2025-07-09T18:07:05
2025-05-07T15:53:23 --> 2025-05-07T21:55:11
Evolution an active region coronal jet.
Detected by Navdeep Panesar, Submitted at 2025-07-09T18:05:13
2025-05-06T23:59:10 --> 2025-05-07T20:25:22
The eruption of a twisted flux rope along with a coronal cavity
Detected by Navdeep Panesar, Submitted at 2025-07-09T18:00:15
2025-05-07T05:19:22 --> 2025-05-07T14:49:22
Evolution of a prominence-filament system
Detected by Chunming Zhu, Submitted at 2025-07-07T06:38:54
2025-06-29T16:34:22 --> 2025-06-29T16:44:12
A solar flare was captured by IRIS during a flare observation on AR 14122. The IRIS slit crosses the flare ribbon.
Detected by Chunming Zhu, Submitted at 2025-07-07T06:32:39
2025-06-26T00:53:13 --> 2025-06-26T01:07:01
During a coordination with PSP, IRIS scans through AR 14117 and nearby regions. A flare occurred during this scan.
Detected by Chunming Zhu, Submitted at 2025-07-07T06:25:10
2025-06-24T07:31:18 --> 2025-06-24T09:36:09
Some coronal Jets were detected in AR 14118 by IRIS, with the slit crosses these small scale solar activities.
Detected by Tingyu Gou, Submitted at 2025-07-01T20:29:47
2025-06-19T19:22:57 --> 2025-06-19T19:50:30
IRIS observed a C5.9 flare in AR 14114 with high-cadence program. Flare ribbons are highly curved, captured by the slit.
Detected by Tingyu Gou, Submitted at 2025-07-01T20:11:20
2025-06-19T16:10:12 --> 2025-06-19T17:11:54
IRIS observed more than one C-class flares in AR 14114 with very high-cadence program. Multiple flare ribbons show in the SJI FOV and are captured by the slit.
Detected by Tingyu Gou, Submitted at 2025-07-01T19:52:39
2025-06-19T07:29:41 --> 2025-06-19T10:01:16
Two C-class flares in AR 14114 show in the IRIS's FOV. Flare ribbons are under the slit.
Detected by Tingyu Gou, Submitted at 2025-07-01T19:32:45
2025-06-17T21:00:28 --> 2025-06-17T21:45:29
IRIS observed the beginning of an X1.2 flare in AR 14114, bright ribbon under the slit.
Detected by halocme, Submitted at 2025-06-20T05:16:01
2025-06-19T23:25:30 --> 2025-06-20T00:54:45
Another X-class (X1.9) flare occurred in AR 14114 around midnight (in UT) to 20 June 2025. Again, no global eruptions were observed.
Detected by Aparna Venkataramanasastry, Submitted at 2025-05-25T06:43:48
2025-04-19T06:21:11 --> 2025-04-19T06:52:55
Coronal jet activity in AR 14062 in the left part of this field of view. Slit does not cross the base of the jet. Only base of the jet is seen in the fog, the spire is outside the fov.
Detected by Aparna Venkataramanasastry, Submitted at 2025-05-25T06:27:16
2025-04-18T15:59:49 --> 2025-04-18T17:11:13
Brightenings along and across arcs in AR 14062 that extend towards opposite polarities revealing loop structures. The brightenings go back and forth a few times during this recording, caused possibly by flux cancellation near the right ends of the loops.
Detected by Aparna Venkataramanasastry, Submitted at 2025-05-25T05:53:38
2025-04-18T11:15:26 --> 2025-04-18T13:36:04
Coronal rain and possibly nano jets at the solar east limb.
Detected by Aparna Venkataramanasastry, Submitted at 2025-05-25T05:35:10
2025-04-17T04:19:17 --> 2025-04-17T05:54:57
Multiple jets spewing from AR 14062.
Detected by Aparna Venkataramanasastry, Submitted at 2025-05-25T05:21:05
2025-04-16T10:45:37 --> 2025-04-16T12:04:23
East limb AR with surges, coronal rain and mass flows along loops.
Detected by Aparna Venkataramanasastry, Submitted at 2025-05-25T05:10:21
2025-04-15T21:11:36 --> 2025-04-15T21:44:04
A prolonged activation leading to a surge like flare.
