Recent Events Reported by Observers
Previous Next
Detected by jinmeng, Submitted at 2018-01-31T19:19:02
2018-01-03T08:30:09 --> 2018-01-03T11:06:09
A small-scale filament eruption was observed. A remote dimming NE of the source region was seen, which might indicate the magnetic connectivity between them.
Detected by jinmeng, Submitted at 2018-01-31T19:19:01
2018-01-03T08:30:09 --> 2018-01-03T11:06:09
A small-scale filament eruption was observed. A remote dimming NE of the source region was seen, which might indicate the magnetic connectivity between them.
Detected by gchintzo, Submitted at 2018-01-30T22:01:29
2018-01-26T00:00:09 --> 2018-01-28T00:00:09
A slowly appearing circlular-shaped cavity with dark filament material extending to its core. The gradual appearance with the absence of rapid motions suggests that the system is brought to visibility due to the solar rotation.
Detected by gchintzo, Submitted at 2018-01-30T21:56:51
2018-01-23T00:00:09 --> 2018-01-26T00:00:09
A solar prominence seen in the northwest limb as dark strands that slowly darken and rise higher in the corona as the sun rotates. Note the appearance and disappearance of a dark circular-shaped cavity that appears gradually in the corona surrounding the prominence.
Detected by gchintzo, Submitted at 2018-01-30T21:48:53
2018-01-21T21:40:09 --> 2018-01-22T11:40:09
A large trans-Equatorial coronal hole system extending from near the south polar coronal hole and stretching towards the northwest. It appears fragmented i.e. with non-uniform intensity along its length. Note the narrow width of this system.
Detected by gchintzo, Submitted at 2018-01-30T21:41:56
2018-01-21T21:40:09 --> 2018-01-22T11:40:09
Filaments seen close to the solar limb begin to oscillate after the disturbance caused by the CME eruption of the AR in the East of the Field of View
Detected by Milan Gosic, Submitted at 2018-01-26T00:56:36
2018-01-21T11:24:52 --> 2018-01-21T11:51:53
Yet another filament eruption in AR 12696. The slit crosses the region.
Detected by Milan Gosic, Submitted at 2018-01-26T00:54:02
2018-01-20T17:33:13 --> 2018-01-20T18:00:14
Filament eruption in AR 12696. The slit crosses the region.
Detected by Milan Gosic, Submitted at 2018-01-25T20:06:17
2018-01-22T03:18:49 --> 2018-01-22T04:06:04
IRIS SJI 1400 filtergrams show post-CME loops in AR 12696. The slit is crossing the region.
Detected by Milan Gosic, Submitted at 2018-01-25T19:33:10
2018-01-20T13:58:11 --> 2018-01-20T14:44:51
SJI images reveal a filament eruption in AR 12696. The slit is crossing the region ~10 minutes later.
Detected by Milan Gosic, Submitted at 2018-01-25T19:29:42
2018-01-19T12:38:18 --> 2018-01-19T12:56:13
Filament eruption in AR 12696, resulting in a spreading ribbon. The slit does not cross the region.
Detected by Milan Gosic, Submitted at 2018-01-25T19:21:46
2018-01-19T01:00:33 --> 2018-01-19T01:14:40
Filament activation in the quiescent active reiogn 12696. The slit crosses the region.
Detected by Milan Gosic, Submitted at 2018-01-24T00:03:04
2018-01-18T18:06:23 --> 2018-01-18T18:41:22
Filament activation was detected around the PIL of AR 12696. The slit is partially crossing the filament.
Detected by gchintzo, Submitted at 2018-01-23T23:01:47
2018-01-21T21:40:09 --> 2018-01-22T11:40:09
A filament eruption in decaying AR 12696. This event produced a CME (~445 km sec-1; http://spaceweather.gmu.edu/seeds/dailymkmovie.php?cme=20180122&r)
Detected by cheung, Submitted at 2018-01-19T05:01:18
2018-01-11T15:00:09 --> 2018-01-12T17:20:09
The coronal rain appearing in this region does not stay in one place.
Detected by cheung, Submitted at 2018-01-19T04:53:17
2018-01-17T05:30:09 --> 2018-01-17T13:40:09
The faint filament in the bounding box is seen to rise but it's unclear whether this was an eruption.
Detected by cheung, Submitted at 2018-01-19T04:49:02
2018-01-15T17:30:09 --> 2018-01-15T19:20:09
The filament material (304) seems to be contained in a sheath around a light-bulb shaped void, suggestive of a magnetic flux cope.
Detected by Chad Madsen, Submitted at 2018-01-17T19:04:41
2018-01-15T00:54:44 --> 2018-01-15T01:07:37
Small, elongated, transient brightening observed on the trailing edge of AR12694. Spectra shows intensification and broadening of C II 1335 lines, Si IV 1394/1403, and Mg II h/k consistent with UV Bursts. The absence of O IV 1401 emission suggests the event takes place in the lower atmosphere.
Detected by Chad Madsen, Submitted at 2018-01-17T19:00:40
2018-01-12T07:55:14 --> 2018-01-12T08:25:19
Small, elongated, transient brightening along the eastern edge of the central plage structure of AR12694. Spectrum shows strong intensification and broadening across all strong UV lines sampled by IRIS, including the relatively weak O I 1355.6 and C I 1355.8 lines.
Detected by Chad Madsen, Submitted at 2018-01-17T18:49:10
2018-01-11T17:26:17 --> 2018-01-11T18:07:53
Small, compact brightening near slit center observed in a mid-latitude coronal hole. Spectrum reveals a profound enhancement of Mg II h/k winds similar to enhancements produced by Ellerman Bombs in H-alpha.
