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

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

Detected by gchintzo, Submitted at 2016-11-12T02:12:22

2016-11-09T19:40:06 --> 2016-11-10T16:00:06

A prominence (i.e. a filament seen at the solar limb) erupts and causes a slow (~220 km/sec) CME (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161110.120006.w039.v0211.p107&frame=24&r).

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

Detected by gchintzo, Submitted at 2016-11-12T02:06:14

2016-11-08T18:17:36 --> 2016-11-09T03:10:06

A small flux emergence episode occurs next to a East-West oriented filament (dark absorption feature at the bottom left area of the field of view). The filament activates (sudden brightenings in the 304 (red) and 171 (blue) channels) and begins to lift rapidly, causing a slow (359 km/sec) Coronal Mass Ejection (see http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161109.012544.w063.v0359.p073&frame=13&r).

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

Detected by gchintzo, Submitted at 2016-11-12T01:47:31

2016-11-08T15:00:06 --> 2016-11-08T22:30:06

A South-North oriented filament (dark absorption feature) becomes unstable and lifts. Traces of cool material seem to move Northward and eventually hit the surface, resulting in brightenings seen in the 171 channel (~1MK). The corona in the original location of the filament seems to become hotter (211 A; ~2MK; green color)

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

Detected by gchintzo, Submitted at 2016-11-09T01:53:39

2016-11-03T18:20:06 --> 2016-11-04T10:10:06

Eruption of a long South-North oriented filament. South and North ends of the filament seem to be close to newly emerging active regions, that presumably modified the corona around them and near the filament. This filament eruption is the source region of a slow CME (207km/sec) seen in LASCO http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161104.081206.w037.v0207.p266&frame=19&r

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

Detected by gchintzo, Submitted at 2016-11-09T01:23:15

2016-10-30T23:10:54 --> 2016-10-31T00:27:54

The initial stage of a slow CME seen in LASCO on 2016/10/31 00:24 (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161031.002406.w069.v0233.p286&frame=11&r). The source AR is behind the solar limb. Oscillations are seen in the ambient corona after the eruption.

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

Detected by gchintzo, Submitted at 2016-11-09T00:52:27

2016-10-30T12:30:06 --> 2016-11-01T02:30:06

Flux emergence occurs in a region of predominantly negative flux (magnetogram is overlayed with red/negative flux and green/positive flux). A filament is seen to lengthen right by the positive polarity of this emerging active region.

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

Detected by gchintzo, Submitted at 2016-11-08T23:34:53

2016-10-30T02:29:54 --> 2016-10-30T03:26:18

A mini-filament (small scale twisted structure with cool material in 304 channel; red color) erupts and reconnects with the ambient field, making a jet like surge in the corona (211 A; green color).

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

Detected by halocme, Submitted at 2016-11-06T06:44:29

2016-10-22T09:40:10 --> 2016-10-22T10:40:10

A small eruption started northeastward, but then deflected to northwest or nearly radial. The jet was produced ahead of the eruption, probably tracing the pre-exisiting open field lines.

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

Detected by halocme, Submitted at 2016-11-06T00:49:17

2016-10-22T16:30:34 --> 2016-10-22T17:50:34

This occurred in the region immediately west of AR 12602. It showed dimming and oscillations. A CME was observed starting 17:24.

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

Detected by halocme, Submitted at 2016-11-06T00:49:16

2016-10-22T16:30:34 --> 2016-10-22T17:50:34

This occurred in the region immediately west of AR 12602. It showed dimming and oscillations. A CME was observed starting 17:24.

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

Detected by halocme, Submitted at 2016-11-05T23:15:17

2016-10-21T00:00:06 --> 2016-10-23T00:00:06

This two-day period coincides with the growth of AR 12603 from 10 msh to 30 msh. As more magnetic flux emerged and the two poles separated, many microflares occurred. However, major (only B-class) flares seem to have avoided this period.

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

Detected by halocme, Submitted at 2016-11-05T03:27:39

2016-11-04T11:50:22 --> 2016-11-04T15:00:22

This eruption occurred in a plage region immediately east of AR 12605. The dimming region moved into the coronal hole to southeast.

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

Detected by halocme, Submitted at 2016-11-04T21:42:37

2016-11-04T01:00:06 --> 2016-11-04T07:00:06

This filament lay in a quiescent region and erupted slowly without producing X-ray emitting high-temperature plasma.

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

Detected by jinmeng, Submitted at 2016-10-31T22:10:59

2016-10-28T05:00:06 --> 2016-10-28T17:34:06

An eruption behind the east limb (seems like a quiet Sun filament eruption) leads to the filament activation at the east limb. Part of the filament material was ejected and most of the rest returned back to the Sun.

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

Detected by jinmeng, Submitted at 2016-10-31T22:10:59

2016-10-28T05:00:06 --> 2016-10-28T17:34:06

An eruption behind the east limb (seems like a quiet Sun filament eruption) leads to the filament activation at the east limb. Part of the filament material was ejected and most of the rest returned back to the Sun.

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

Detected by jinmeng, Submitted at 2016-10-31T21:43:04

2016-10-27T15:00:06 --> 2016-10-28T09:20:06

An eruption from a flux emerging active region. The eruption seems to influence a large area to the south with brightenings. But EUV waves are not evident from running difference movies.

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

Detected by jinmeng, Submitted at 2016-10-31T21:43:04

2016-10-27T15:00:06 --> 2016-10-28T09:20:06

An eruption from a flux emerging active region. The eruption seems to influence a large area to the south with brightenings. But EUV waves are not evident from running difference movies.

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

Detected by jinmeng, Submitted at 2016-10-31T21:27:10

2016-10-27T11:30:06 --> 2016-10-27T18:40:06

An eruption near the east limb that leads to coronal loop activities (dimming). The source region is located at the northern part of the loop.

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

Detected by jinmeng, Submitted at 2016-10-31T21:14:13

2016-10-26T00:00:06 --> 2016-10-26T10:10:06

An eruption from a small active region near the big coronal hole.

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

Detected by jinmeng, Submitted at 2016-10-31T21:03:46

2016-10-26T04:40:06 --> 2016-10-26T13:20:06

A filament eruption was observed at the west limb.