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

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by Annotator, Submitted at 2010-05-10T23:30:52

2010-05-08T01:58:25 --> 2010-05-08T08:13:31

A nice filament eruption with a fast moving wave traveling across the disk. This eruption is followed by several more very nice eruptions from the save active region, also with associated waves.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by Annotator, Submitted at 2010-05-06T22:19:07

2010-05-05T16:00:02 --> 2010-05-05T17:58:37

A nice filament eruption in the south with an associated wave. There is an M-class flare in the northern hemisphere that follows shortly after.in AR11069...

Rating: 4.5 (0=lowest, 5=highest)         Num Ratings:2

Detected by asainz, Submitted at 2011-03-23T17:47:13

2011-03-21T06:00:12 --> 2011-03-23T00:00:12

Evolution of coronal canopy and small jet.

Rating: 4.5 (0=lowest, 5=highest)         Num Ratings:2

Detected by schryver, Submitted at 2011-02-16T23:54:42

2011-02-16T13:37:16 --> 2011-02-16T16:08:28

Coronal wave emanating from the site of an M1 flare.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2021-05-09T18:16:23

2021-05-09T09:30:01 --> 2021-05-09T11:30:01

This filament was sitting neaxt to a plage region. The eruption is clearly traceable with aid by spreading ribbons at its base.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2021-03-17T00:17:11

2021-01-11T10:00:09 --> 2021-01-12T01:30:09

Coronal cavity and filament structures observed at the east limb.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by mkocher, Submitted at 2019-04-25T22:34:19

2019-03-09T12:10:09 --> 2019-03-09T14:50:09

Active Region filament matured into a brilliant eruption, close to the disk center in the North Western hemisphere of the Sun. This eruption is also observed in STEREO A.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by gchintzo, Submitted at 2019-02-25T19:49:51

2019-02-23T13:10:09 --> 2019-02-24T04:05:09

A filament eruption originating from the single decaying active region transiting the solar disk. This was a successful eruption as it can be seen in the movie from LASCO coronagraph data (http://spaceweather.gmu.edu/seeds/dailymkmovie.php?cme=20190224&r)

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by gchintzo, Submitted at 2019-02-14T00:51:55

2019-02-12T00:00:09 --> 2019-02-13T00:00:09

A Coronal Cavity at the northwest limb of the sun. Cool material (white/purple) extends high all the way to the core of the cavity. Red colors show emission from plasma at 2 MK.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by gchintzo, Submitted at 2019-02-14T00:03:18

2019-02-10T09:30:09 --> 2019-02-12T00:00:09

A coronal cavity in the northwest limb of the sun exhibiting rotational motions in its interior. It appears that material rises from lower heights and as it moves upwards within the cavity a sense of counterclockwise rotation occurs wirhin the cavity.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2019-01-04T00:45:30

2018-12-28T17:00:09 --> 2018-12-28T18:00:09

The low-temperature component traces the helical structure of the magnetic field involved in the ejection.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2018-08-29T22:02:06

2018-08-20T08:00:09 --> 2018-08-20T16:30:09

It is hard to tell how and when the eruption started, but the spreading ribbons and post-eruption arcade indicate an eruption. This eruption was later seen in STEREO-A COR2 images as an Earth-directed CME with a flux rope and in LASCO C2 images as a diffuse, slow CME. The CME was responsible for a G3 geomagnetic storm on August 26, the third largest in solar cycle 24.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2018-08-29T17:33:15

2018-08-22T11:45:01 --> 2018-08-22T13:00:37

The origin seems to be the following part of AR 12719. Probably no CME associated with this kind of events.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2018-07-08T03:33:38

2018-07-04T23:20:25 --> 2018-07-05T03:20:25

Eruption of a filament in a quiescent region, resulting in a post-eruption arcade (not hot/dense enough to contribute to GOES X-rays) and small dimming regions on either side.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2018-07-08T03:26:07

2018-07-04T23:00:09 --> 2018-07-05T00:30:09

A coronal wave that had not been observed for a few months. This occurred in a quiescent region and no flare was seen in GOES soft X-rays. Global disturbances are seen, for example, in the northeast direction, where quiet-Sun structures showed temporary enhancement in intensity at 193 A.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by tiwari, Submitted at 2018-04-10T21:06:51

2018-04-09T02:30:09 --> 2018-04-10T00:00:09

Beginning of a small bipolar flux emergence is observed.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by weiliu, Submitted at 2018-03-15T21:13:04

2018-03-06T04:00:09 --> 2018-03-06T20:00:09

An S-shaped long filament eruption resulted in double dimmings (transient coronal holes) with a figure-8 shape. There was partial IRIS coverage during the late stage of the filament eruption.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by weiliu, Submitted at 2018-03-15T21:13:04

2018-03-06T04:00:09 --> 2018-03-06T20:00:09

An S-shaped long filament eruption resulted in double dimmings (transient coronal holes) with a figure-8 shape. There was partial IRIS coverage during the late stage of the filament eruption.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2018-03-03T01:44:49

2018-03-02T00:00:09 --> 2018-03-02T02:00:09

AR 12770 had been dormant until late 1 March 2018, when it started to produce four flares above B1. This one was the most eruptive with relatively long duration soft X-rays. It was accompanied by coronal dimming and global waves.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-12-23T11:17:58

2017-12-23T06:30:01 --> 2017-12-23T07:20:25

An impressive jet that can be traced to the edge of the AIA FOV.