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 2017-09-21T21:13:37
2017-09-19T07:38:09 --> 2017-09-19T12:18:09
A mini-filament eruption was observed.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-21T21:04:21
2017-09-18T13:06:09 --> 2017-09-18T20:46:09
Filament eruption at the east limb. After the eruption, large-scale coronal loops could be seen. Looks like a failed eruption (?)
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-21T21:04:20
2017-09-18T13:06:09 --> 2017-09-18T20:46:09
Filament eruption at the east limb. After the eruption, large-scale coronal loops could be seen. Looks like a failed eruption (?)
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-21T18:45:56
2017-09-20T18:36:09 --> 2017-09-20T21:26:09
Sympthetic eruptions observed near the west limb. The activity started as filament activation near an active region. This activity seems to trigger an eruption from the active region.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-21T18:45:55
2017-09-20T18:36:09 --> 2017-09-20T21:26:09
Sympthetic eruptions observed near the west limb. The activity started as filament activation near an active region. This activity seems to trigger an eruption from the active region.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2017-09-19T19:44:05
2017-09-16T23:50:09 --> 2017-09-17T16:50:09
A view of the East limb of the Sun. A fast CME (663 km/sec) that occured in the back side of the sun produced a wake that propagates in the visible to the Earth face of the sun. See http://spaceweather.gmu.edu/seeds/mkmovie_ql.php?cme=20170917.120008.w154.v0663.p084&frame=6
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2017-09-19T18:36:04
2017-09-15T00:00:09 --> 2017-09-18T00:00:09
A large coronal hole in the North hemisphere of the sun (region of low EUV intensity). Note the fine structure and brightening events inside the coronal hole mostly due to canceling magnetic elements.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-15T05:54:39
2017-09-10T15:00:02 --> 2017-09-11T01:00:02
This concluded eruptive activity of AR 12673. Reconnection related features included plasmoid (flux rope) like eruption, followed by formation of a thin current sheet and supra arcade downflows (both in the main and southern systems). The cusp-like structure stands out in 94 A, indicative of high temperature.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-15T05:44:55
2017-09-13T05:15:01 --> 2017-09-13T06:15:01
AR 12680 consists of a single sunspot. This jet appears to originate in the mixed polarity region southwest of the spot. An associated brightening is seen next to a dark feature that runs across the spot umbra.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T08:28:24
2017-09-12T19:00:09 --> 2017-09-12T20:00:09
The flare was again in AR 12680, and there seemed two eruptions, producing a wave that moved mostly southward.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T08:23:59
2017-09-12T15:15:01 --> 2017-09-12T16:30:37
A B3.5 flare in AR 12680 was associated with an eruption moving northward, and as it hit coronal structures, it produced a wave, which is more diffuse than normal large-scale coronal propagating fronts.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T08:23:58
2017-09-12T15:15:01 --> 2017-09-12T16:30:37
A B3.5 flare in AR 12680 was associated with an eruption moving northward, and as it hit coronal structures, it produced a wave, which is more diffuse than normal large-scale coronal propagating fronts.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T08:13:20
2017-09-12T13:45:01 --> 2017-09-12T14:45:01
The eruption from AR 12677 accompanied waves moving into the solar disk.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T08:13:19
2017-09-12T13:45:01 --> 2017-09-12T14:45:01
The eruption from AR 12677 accompanied waves moving into the solar disk.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T07:47:07
2017-09-09T22:00:09 --> 2017-09-09T23:30:09
The eruption was mostly radial but lateral expansion drove a wave mostly counterclockwise. A fat CME was associated (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170909.233608.w070.v0739.p283&frame=5&r).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T07:47:06
2017-09-09T22:00:09 --> 2017-09-09T23:30:09
The eruption was mostly radial but lateral expansion drove a wave mostly counterclockwise. A fat CME was associated (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170909.233608.w070.v0739.p283&frame=5&r).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T07:37:38
2017-09-07T17:20:25 --> 2017-09-07T19:10:49
This coronal wave seems to be originated over the limb, not closely related to C-class flares in AR 12673.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T07:37:38
2017-09-07T17:20:25 --> 2017-09-07T19:10:49
This coronal wave seems to be originated over the limb, not closely related to C-class flares in AR 12673.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T07:19:10
2017-09-07T14:20:25 --> 2017-09-07T15:30:01
An eruption was mostly in the radial direction, and the associated wave on the disk was diffuse. The associated CME was not broad (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170907.153636.w043.v0334.p248&frame=13&r).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T07:19:10
2017-09-07T14:20:25 --> 2017-09-07T15:30:01
An eruption was mostly in the radial direction, and the associated wave on the disk was diffuse. The associated CME was not broad (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170907.153636.w043.v0334.p248&frame=13&r).