LMSAL >> Sungate >> Heliophysics Events Knowledgebase

Recent Events Reported by Observers

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Detected by Juraj Lorincik, Submitted at 2023-06-26T17:43:55
2023-06-14T22:47:01 --> 2023-06-14T23:29:39
Failed eruption associated with a two-ribbon C-class flare.

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Detected by Juraj Lorincik, Submitted at 2023-06-26T17:40:05
2023-06-14T05:50:37 --> 2023-06-14T06:16:52
Microflare in the raster of IRIS.

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Detected by Juraj Lorincik, Submitted at 2023-06-26T17:38:15
2023-06-13T20:09:30 --> 2023-06-13T20:29:55
Limb observations of the initiation of a failed eruptive flare at W limb. Raster contains the brightest portion of the flare.

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Detected by Juraj Lorincik, Submitted at 2023-06-26T17:28:22
2023-06-13T09:05:17 --> 2023-06-13T11:01:17
Flare ribbon of a low C-class flare in the raster of IRIS.

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Detected by Juraj Lorincik, Submitted at 2023-06-26T17:22:21
2023-06-13T06:45:01 --> 2023-06-13T07:05:26
Short-living burst resembling of a peacock tail at NE limb in the FOV of IRIS raster.

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Detected by Paul Bryans, Submitted at 2023-06-12T19:55:44
2023-05-23T23:43:59 --> 2023-05-24T02:50:12
Very interesting peacock tail loops rising and falling under slit.

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Detected by Paul Bryans, Submitted at 2023-06-12T19:54:15
2023-05-29T16:29:34 --> 2023-05-29T16:29:34
Flare with no GOES categorization.

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Detected by Paul Bryans, Submitted at 2023-06-12T19:51:37
2023-05-23T12:09:11 --> 2023-05-23T12:09:11
Off-limb loops and coronal rain.

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Detected by Navdeep Panesar, Submitted at 2023-06-12T19:22:10
2023-03-13T03:29:58 --> 2023-03-15T22:59:58
Evolution of a polar crown prominenxe

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Detected by Navdeep Panesar, Submitted at 2023-06-11T00:53:52
2023-06-10T08:31:34 --> 2023-06-10T10:58:22
Eruption of a quiescent filament.

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Detected by Q. M. Wargnier, Submitted at 2023-06-08T18:43:12
2023-06-01T10:36:35 --> 2023-06-01T11:43:48
In AR13319, on 06/01/2023 a flare occurs nearby the left sunspot.

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Detected by Q. M. Wargnier, Submitted at 2023-06-08T18:39:08
2023-06-04T08:35:58 --> 2023-06-04T09:16:03
A flare is produced in the middle of the FOV in the 2796 line.

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Detected by Q. M. Wargnier, Submitted at 2023-06-08T18:36:20
2023-06-01T17:20:41 --> 2023-06-01T19:17:28
During BBSO coordination on 06/01/2023, a flare has emerged. A flow of plasma perpendicular to the plane can be noticed.

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Detected by Tingyu Gou, Submitted at 2023-05-26T21:45:44
2023-05-22T18:14:55 --> 2023-05-22T19:16:13
C3.0 flare (start at 18:25 UT) from AR 13312 partially captured by IRIS, one ribbon visible with slit on it.

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Detected by Tingyu Gou, Submitted at 2023-05-26T21:33:18
2023-05-22T10:03:47 --> 2023-05-22T12:02:31
The sunspot in AR 13310 was captured in IRIS's FOV, waves inside, the slit scans on the light bridge.

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Detected by Tingyu Gou, Submitted at 2023-05-26T21:19:14
2023-05-20T18:20:42 --> 2023-05-20T22:59:09
Flare activities in AR 13311 were partially captured under the high-cadence program, including C7.2(18:42), M1.2(18:57), C6.1(20:57), M5.2(22:52). Flare ribbons in the FOV, IRIS slit on the lower western ribbon.

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Detected by Tingyu Gou, Submitted at 2023-05-26T20:27:34
2023-05-20T13:11:39 --> 2023-05-20T18:08:49
A lot of flaring activities and britengings in AR 13311 were detected, including a C7.2 flare starting at 14:18 UT and an M5.7 one at 14:54 UT, and serval C-class flares in the following, two ribbons captured. IRIS slit sits right across the lower western ribbon.

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Detected by Tingyu Gou, Submitted at 2023-05-26T20:03:39
2023-05-19T04:50:25 --> 2023-05-19T06:25:40
Coronal loops seen at the NE limb, material of coronal rains falling down under the slit. An M2.5 flare from AR 13311 starting at 04:49 UT was partially captured in the right part of the FOV.

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Detected by Tingyu Gou, Submitted at 2023-05-26T19:50:30
2023-05-18T13:07:09 --> 2023-05-18T17:55:55
Coronal loops and rains observed at the solar southeast limb, outlining filed lines. Persistent nanojets and spicules occur at various points in time.

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Detected by Tingyu Gou, Submitted at 2023-05-26T19:29:29
2023-05-17T17:35:05 --> 2023-05-17T18:03:49
C2.8 flare from AR 13305, two flare ribbons captured in the IRIS's FOV, with slit across the flare loops

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