Highest Rated Events (only 193 and 304 shown) All AR FE FL
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2018-01-31T21:45:23
2018-01-07T02:10:09 --> 2018-01-07T21:20:09
Multiple eruptions were observed from AR 12693 near the west limb beginning with a failed filament eruption. After the main filament eruption, a new filament formed near the north edge of the active region.
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3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2018-01-31T21:45:22
2018-01-07T02:10:09 --> 2018-01-07T21:20:09
Multiple eruptions were observed from AR 12693 near the west limb beginning with a failed filament eruption. After the main filament eruption, a new filament formed near the north edge of the active region.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2018-01-31T19:46:14
2018-01-03T16:54:09 --> 2018-01-03T18:02:09
A small-scale filament eruption, which seems failed at last.
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Num Ratings:1
Detected by jinmeng, Submitted at 2018-01-31T19:18:53
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2018-01-31T19:18:53
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2018-01-30T22:01:24
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2018-01-30T21:56:46
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2018-01-30T21:48:48
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2018-01-30T21:41:51
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
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2018-01-23T23:01:41
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)
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2018-01-19T04:48:58
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2018-01-10T03:32:04
2018-01-09T03:30:09 --> 2018-01-10T00:00:09
A small coronal hole in the north hemisphere of the sun. Note that it is primarily composed by positive polarities (green color in HMI magnetogram).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2018-01-10T03:27:47
2018-01-09T03:30:09 --> 2018-01-10T00:00:09
A highly non-radial confined eruption seen at the north east limb of the sun. A (potentially) polar crown filament becomes unstable and keeps gaining height until it reaches a certain altitude and halts to expand. Cool dark material is seen to be lifted with this "bubble" like structure.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2018-01-10T03:19:57
2018-01-04T00:00:09 --> 2018-01-08T00:00:09
The north coronal hole extends southward. Note the activity inside the hole in the form of bright points and small bright loops.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2018-01-10T03:09:55
2018-01-06T13:00:09 --> 2018-01-06T15:40:09
A jet eruption at the south pole of the sun. Note the dark material moving from east to west while a jet-like column brightens.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2018-01-10T02:55:44
2018-01-07T00:10:09 --> 2018-01-07T16:40:09
A failed eruption originating from AR12693. Note the large scale connectivities associated with the developing eruption. There was no CME originating from this AR.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-01-05T18:10:05
2018-01-03T22:55:13 --> 2018-01-04T01:31:13
Essentially a repeat of the earlier event during 3 Jan 2018 09:00-10:40.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-01-05T18:04:48
2018-01-03T09:00:02 --> 2018-01-03T10:40:02
A mini filament eruption occurred in the northern part of the region which later became AR 12693 (during 4 Jan 2018 with a 20 MSH sunspot). In addiion to the post-eruption arcade, this eruption disturbed another region to the northeast, which may have been already magnetically connected.