Recent Events Reported by Observers
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Detected by jinmeng, Submitted at 2016-12-19T18:35:40
2016-12-17T23:40:06 --> 2016-12-19T00:00:06
A flux emerging region was observed in the on-disk coronal hole (near the boundary). The emerged flux then deveoped connections with the surrounding small-scale fluxes.
Detected by jinmeng, Submitted at 2016-12-17T00:59:26
2016-12-15T03:23:06 --> 2016-12-15T04:07:06
A failed eruption was observed at the west limb. Wave-feature was observed propagating across field lines. A flux-rope like structure was also observed to raise and fall back.
Detected by jinmeng, Submitted at 2016-12-17T01:40:35
2016-12-15T02:50:06 --> 2016-12-16T00:00:06
Possible sympathetic filament erutpions were observed with sepeartion about 8-10 hours.
Detected by jinmeng, Submitted at 2016-12-17T01:40:35
2016-12-15T18:57:06 --> 2016-12-16T00:00:06
A filament went unstable and erupted at last. Most of the filament material seems fall back to the Sun and lead to brightenings. The large-scale field might be changed due to the eruption that leads to a fast shrink of a coronal hole east of the source region. Moreover, there are synchronous activities from an active region at the west limb.
Detected by jinmeng, Submitted at 2016-12-17T00:05:31
2016-12-14T18:16:06 --> 2016-12-14T18:46:42
a coronal jet was observed in the northern coronal hole with mini-filament eruption. The brightening after eruption showed an S-shape.
Detected by jinmeng, Submitted at 2016-12-17T01:40:34
2016-12-13T02:30:06 --> 2016-12-13T09:10:06
A filament eruption was observed in the southern hemisphere.
Detected by Lakshmi Pradeep Chitta, Submitted at 2016-12-15T16:03:36
2016-11-21T11:44:34 --> 2016-11-21T11:49:39
This particular observation shows a significantly large blueshift in the transition region spectral lines.
Detected by Lakshmi Pradeep Chitta, Submitted at 2017-07-24T18:57:24
2016-11-16T09:29:54 --> 2016-11-16T09:55:19
Flux emergence combined with explosive events.
Detected by jinmeng, Submitted at 2016-12-13T20:22:21
2016-12-11T10:00:06 --> 2016-12-12T05:30:06
An emerging flux region was observed within the on-disk coronal hole. After the emerging phase, the region showed multiple activities with enhanced EUV emission.
Detected by jinmeng, Submitted at 2016-12-13T20:22:21
2016-12-10T15:20:06 --> 2016-12-10T21:50:06
An eruption at the west limb. The eruption disturbed coronal loops. The EUV emission reached maximum after the eruption onset.
Detected by jinmeng, Submitted at 2016-12-13T20:22:21
2016-12-10T01:00:06 --> 2016-12-10T04:20:06
A coronal jet from an on-disk coronal hole. It is a mini-filament eruption.
Detected by Jean-Pierre Wuelser, Submitted at 2016-12-13T00:28:45
2016-12-03T11:14:33 --> 2016-12-03T11:20:24
A tiny explosive event that happened to surge right along the slit in a high cadence sit&stare sequence.
Detected by Jean-Pierre Wuelser, Submitted at 2016-12-13T00:17:57
2016-12-02T17:40:09 --> 2016-12-02T17:45:24
A tiny flare that happened to occur on the slit during fast sit&stare observations. Broad spectral lines.
Detected by Jean-Pierre Wuelser, Submitted at 2016-12-13T00:08:13
2016-11-30T15:02:34 --> 2016-11-30T15:39:26
C 2.3 flare. Slit covers portion of event, but not the White Light kernel.
Detected by Jean-Pierre Wuelser, Submitted at 2016-12-12T23:58:24
2016-12-04T17:45:14 --> 2016-12-04T18:02:55
C 1.8 flare. IRIS slit scans once across the ribbons over the course of the event.
Detected by gchintzo, Submitted at 2016-12-08T19:54:41
2016-12-05T23:00:06 --> 2016-12-07T15:10:06
Filament Eruption on the North East limb of the sun. A nearby emerging flux region (shows up at the north of the filament) potentially played a role in destabilizing the long filament. This event is the source region of a slow CME (230 km/sec; http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161207.110007.w073.v0230.p067&frame=20&r)
Detected by gchintzo, Submitted at 2016-12-07T19:30:41
2016-12-05T05:30:06 --> 2016-12-05T13:20:06
Large scale faint connectivity in 171 (light blue) is seen to slowly move radially outwards above the East limb of the sun. At least close to the limb around the equator, this connectivity shows emmision in 304 (red). This is possibly a back-sided large filament eruption. This activity is likely the source region of a very slow CME (122 km/sec) observed by LASCO (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161205.162406.w063.v0122.p108&frame=30&r)
Detected by gchintzo, Submitted at 2016-12-07T19:09:24
2016-12-04T13:10:06 --> 2016-12-04T15:49:28
An Active Region filament erupts and breaks into dark radial "threads", possibly due to reconnection of the structure with the ambient field. Some of the filament material falls back down as coronal "rain". This is the source region of a jet-like (small angular size) CME observed by LASCO C2 (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161204.142406.w027.v0418.p298&frame=11&r)
Detected by gchintzo, Submitted at 2016-12-07T19:06:09
2016-12-04T13:10:06 --> 2016-12-04T15:49:28
An Active Region filament erupts and breaks into radial "threads", possibly due to reconnection of the structure with the ambient field. This is the source region of a jet-like (small angular size) CME observed by LASCO C2 (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161204.142406.w027.v0418.p298&frame=11&r)
Detected by jinmeng, Submitted at 2016-12-06T00:45:33
2016-11-25T02:20:06 --> 2016-11-28T00:00:06
Flux emergence and formation of a small active region was observed.
