Highest Rated Events (only 193 and 304 shown) All AR FE FL

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-12-23T01:49:16

2017-12-15T12:00:09 --> 2017-12-15T15:40:09

A filament eruption was seen southeast of a non-numbered region. It led to a striking twin dimming and spreading flare ribbons. The associated CME is http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171215.170007.w070.v0226.p130&frame=15&r.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-12-23T01:42:40

2017-12-14T21:10:13 --> 2017-12-14T23:40:13

The eruption was associated with a B1.1 flare and from a region slightly occulted. It was loop-like, but produced a CME that was quite narrow (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171214.231214.w023.v0281.p081&frame=12&r).

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-12-23T01:42:39

2017-12-14T21:10:13 --> 2017-12-14T23:40:13

The eruption was associated with a B1.1 flare and from a region slightly occulted. It was loop-like, but produced a CME that was quite narrow (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171214.231214.w023.v0281.p081&frame=12&r).

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-12-23T01:22:48

2017-12-14T13:50:25 --> 2017-12-14T15:30:01

The slow eruption was narrow, centered in the direction of 8 o'clock. Later a post-eruption arcade was seen near the northern leg of the structure that erupted. The source region was slightly behind the limb.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-12-23T01:17:07

2017-12-14T04:40:13 --> 2017-12-14T06:29:25

The minor eruption was associated with a short-duration B1.1 flare in a non-numbered region. As the eruption showed a counterclockwise rotation, a diffuse EUV wave was observedtoward southwest to north.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-12-23T01:17:06

2017-12-14T04:40:13 --> 2017-12-14T06:29:25

The minor eruption was associated with a short-duration B1.1 flare in a non-numbered region. As the eruption showed a counterclockwise rotation, a diffuse EUV wave was observedtoward southwest to north.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-12-23T01:10:29

2017-12-11T00:30:01 --> 2017-12-11T01:50:01

The eruption seems to be confined, not reaching the coronagraph height. This was associated with a short-duration B6.2 flare.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-12-23T01:10:28

2017-12-11T00:30:01 --> 2017-12-11T01:50:01

The eruption seems to be confined, not reaching the coronagraph height. This was associated with a short-duration B6.2 flare.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-12-23T01:04:29

2017-12-10T21:30:01 --> 2017-12-10T22:40:01

Multiple jets are seen, but the one that was ejected non-radially was traceable for a longer distance. It also contained cool material as seen in 304 A images.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2017-12-19T01:24:34

2017-12-01T01:40:09 --> 2017-12-01T08:00:09

Slow filament eruption lasting several hours. It's unclear whether it's a confined or ejective eruption.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2017-12-19T01:03:14

2017-11-22T15:40:09 --> 2017-11-22T20:20:09

Quiescent filament eruption from behind the northeast limb.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-12-01T03:02:55

2017-11-14T00:00:09 --> 2017-11-16T00:00:09

Filament eruption observed near the west limb. The activation and eruption process occurred gradually in a day.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-12-01T02:56:37

2017-11-14T09:31:09 --> 2017-11-14T10:41:09

A mini-filament eruption from a quiet-Sun region.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-12-01T02:22:22

2017-11-13T11:00:09 --> 2017-11-13T13:00:09

A mini eruption from an on-disk coronal hole.

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Detected by jinmeng, Submitted at 2017-12-01T02:22:20

2017-11-13T11:00:09 --> 2017-11-13T13:00:09

A mini eruption from an on-disk coronal hole.

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Detected by jinmeng, Submitted at 2017-12-01T00:56:59

2017-11-12T09:10:09 --> 2017-11-12T19:40:09

A filament eruption was observed at the west limb. There was also synchrounous activity observed near the west limb. The eruption seems in two-steps: first, the flux rope slowly raised up, then it erupted abruptly.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-12-01T00:56:58

2017-11-12T09:10:09 --> 2017-11-12T19:40:09

A filament eruption was observed at the west limb. There was also synchrounous activity observed near the west limb. The eruption seems in two-steps: first, the flux rope slowly raised up, then it erupted abruptly.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-12-01T00:40:59

2017-11-10T05:00:09 --> 2017-11-11T01:40:09

A large-scale filament eruption from the NE. The filament at the limb is more evident. But the on-disk part of the filament eruption can be seen through coronal emission variation after the eruption.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-11-29T23:55:15

2017-11-08T11:00:09 --> 2017-11-08T20:30:09

A filament eruption was observed near the east limb.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-11-22T06:19:10

2017-11-21T07:00:09 --> 2017-11-21T13:00:09

Although the filament/prominence material seemed to largely move northward to lower heights, the overlying corona was also found dimmer in the direction of 9:30 or so. This event was responsible for a CME with a spiky front (see http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171121.121207.w045.v0089.p080&frame=34&r).