Recent Events Reported by Observers
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Detected by Llyr Humphries, Submitted at 2024-05-17T12:40:46
2024-05-08T18:28:26 --> 2024-05-08T20:59:25
Series of small, eruptive events in AR13664
Detected by Llyr Humphries, Submitted at 2024-05-17T12:36:21
2024-05-07T16:26:58 --> 2024-05-07T18:20:53
Large X-class flare can be seen in top-right of the dataset. The event is not captured by the slit. However, a series of precursory and follow-up brightenings do cross the slit.
Detected by Llyr Humphries, Submitted at 2024-05-17T12:31:44
2024-05-07T21:37:46 --> 2024-05-07T22:37:25
Series of ribbons cross the IRIS slit following increased activity within AR13664
Detected by Milan Gosic, Submitted at 2024-05-13T21:55:42
2024-04-12T07:06:33 --> 2024-04-12T07:25:51
An eruption under the slit followed by a C2.3 flare (not covered by the slit). Part of the material ejected during the flare seems to be caught under the slit.
Detected by Milan Gosic, Submitted at 2024-05-13T21:44:02
2024-04-12T12:44:58 --> 2024-04-12T17:50:04
Multiple microflares under the slit in AR 13633, and within an emerging flux region.
Detected by Milan Gosic, Submitted at 2024-05-13T21:06:28
2024-04-11T19:52:19 --> 2024-04-11T23:20:24
Two small flares (possibly C-class flares) in AR 13635. Only a small fraction of the second flare ribbon is under the slit.
Detected by Milan Gosic, Submitted at 2024-05-13T20:39:01
2024-04-11T06:16:42 --> 2024-04-11T06:27:32
C1.9 flare in AR 13633.
Detected by Milan Gosic, Submitted at 2024-05-13T20:32:14
2024-04-10T15:51:29 --> 2024-04-10T19:27:30
Flux emergence in AR 13633, one of the footpoints is under the slit.
Detected by Milan Gosic, Submitted at 2024-05-13T20:23:04
2024-04-10T19:49:19 --> 2024-04-11T00:10:40
Multiple eruptions and microflares under the slit in AR 13635.
Detected by Milan Gosic, Submitted at 2024-05-13T20:13:48
2024-04-09T21:47:28 --> 2024-04-10T00:05:46
Several eruptions and coronal jets are within the FOV, but not under the slit. However, there are a few microflares across AR 13635. which are caught under the slit.
Detected by Milan Gosic, Submitted at 2024-05-13T19:58:21
2024-04-09T15:28:04 --> 2024-04-09T15:44:32
A small flare whose ribbon extends under the slit.
Detected by Milan Gosic, Submitted at 2024-05-13T19:54:30
2024-04-09T07:26:44 --> 2024-04-09T07:58:27
Several coronal jets under the slit in AR 13628.
Detected by Milan Gosic, Submitted at 2024-05-13T19:49:41
2024-04-09T10:34:21 --> 2024-04-09T10:56:02
A flare is partially visible on the left side of the FOV, together with hot plasma moving along the field lines.
Detected by Chunming Zhu, Submitted at 2024-05-13T17:58:49
2024-05-05T17:01:36 --> 2024-05-05T20:00:19
This movie shows a few M class flares originated from AR 13663. The slit crosses both the flare ribbons and the hot loops in between.
Detected by Chunming Zhu, Submitted at 2024-05-13T17:54:47
2024-05-04T19:20:36 --> 2024-05-04T21:10:09
AR 13663 has been quite active and produced intensive flares.
Detected by Chunming Zhu, Submitted at 2024-05-13T17:48:45
2024-04-30T15:34:16 --> 2024-04-30T16:17:07
A spectacular prominence over solar limb was captured by IRIS. Some materials cooled down and fell back the solar surface.
Detected by Chunming Zhu, Submitted at 2024-05-13T17:14:07
2024-05-02T18:10:24 --> 2024-05-02T18:42:46
Some interesting coronal jets were observed by IRIS at the west limb of the Sun. Some hot and dense materials rises and then falls back towards the Sun.
Detected by Chunming Zhu, Submitted at 2024-05-13T17:08:55
2024-05-01T14:22:33 --> 2024-05-01T15:06:36
IRIS scanned through AR 13654 and captured an M1.2 flare. There is also a prominence over the limb in its field of view.
Detected by Tingyu Gou, Submitted at 2024-04-29T15:50:28
2024-04-23T20:46:42 --> 2024-04-23T21:21:44
A GOES-class C7.4 flare starts at 20:58 UT and peaks at 21:11 UT, in AR 13645. Both flare ribbons are visible in IRIS's FOV under the slit.
Detected by Tingyu Gou, Submitted at 2024-04-29T15:22:57
2024-04-23T10:17:55 --> 2024-04-23T12:12:49
Recurrent inverse-Y shaped coronal jets in AR 13655, loops brighten up in the bottom. Brightenings and bursts are also visible nearby, in the core of the active region.
