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

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

Detected by cheung, Submitted at 2018-04-25T21:49:14

2018-04-25T09:20:09 --> 2018-04-25T13:10:09

Repeated filament activations in the core of AR 12706.

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

Detected by tiwari, Submitted at 2018-04-23T18:10:14

2018-04-20T04:50:09 --> 2018-04-21T03:30:09

A small filament erupts as a result of flux cancellation. The flux cancellation continues after the event.

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

Detected by tiwari, Submitted at 2018-04-20T18:27:29

2018-04-19T00:00:09 --> 2018-04-20T01:40:09

Flux cancellation leading to several small-scale jet-like eruptions in a coronal hole.

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

Detected by tiwari, Submitted at 2018-04-20T18:03:39

2018-04-19T00:00:09 --> 2018-04-20T05:00:09

A small prominence tornado inside a coronal cavity.

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

Detected by tiwari, Submitted at 2018-04-20T18:03:37

2018-04-19T00:00:09 --> 2018-04-20T05:00:09

A small prominence tornado inside a coronal cavity.

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

Detected by gchintzo, Submitted at 2018-04-17T23:52:30

2018-04-17T00:00:09 --> 2018-04-17T20:10:09

A filament erupting in the southwest quadrant of the solar disk. A narrow angle CME was associated with this event (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20180417.072424.w122.v0404.p159&frame=4&r&cor2=a)

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

Detected by gchintzo, Submitted at 2018-04-17T23:43:07

2018-04-14T10:40:09 --> 2018-04-15T15:00:09

An ephemeral region emerging in the southwest quadrant of the sun. Green colors show high temperatures of 2 MK.

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

Detected by gchintzo, Submitted at 2018-04-17T23:33:08

2018-04-14T10:40:09 --> 2018-04-15T15:00:09

A solar prominence (dark material) suspended in a coronal cavity. Here, the "envelope" of the the highest lying parts of the prominence mark the lower side of a coronal cavity.

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

Detected by gchintzo, Submitted at 2018-04-17T22:17:42

2018-04-14T10:40:09 --> 2018-04-15T15:00:09

Three narrow-angle eruptions from a back-sided AR. (2018/04/14 20:00 UT: 200 km/s; http://spaceweather.gmu.edu/seeds/dailymkmovie.php?cme=20180414&r 2018/04/15 00:48 UT: 162 km/s;http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20180415.004807.w033.v0162.p089&frame=6&r (2018/04/15 05:48 UT: 326 km/s;http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20180415.054807.w036.v0326.p092&frame=16&r)

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

Detected by gchintzo, Submitted at 2018-04-17T18:02:36

2018-04-14T06:20:09 --> 2018-04-15T10:40:09

A decaying active region in the northeast quadrant of the solar disk as seen in three different wavelengths (304 A: T=50kK; 171 A: T=0.6 MK; 211 A: T=2 MK). Note the magnetic flux distribution on the surface (green positive, red negative flux). A filament is seen as a dark feature in 304 A (diffuse s-shaped feature; top left panel).

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

Detected by gchintzo, Submitted at 2018-04-11T22:34:11

2018-04-10T00:00:09 --> 2018-04-10T13:40:09

Same as previously, but in a four panel view separating the wavelengths.

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

Detected by gchintzo, Submitted at 2018-04-11T22:03:38

2018-04-10T00:00:09 --> 2018-04-10T13:40:09

Recurrent eruptions (three?) near the solar disk center that seems to be associated with cancelling magnetic features on the surface (red and green structures)

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

Detected by halocme, Submitted at 2018-04-07T13:26:55

2018-04-01T00:00:09 --> 2018-04-07T00:00:09

This region had the number of 12703 only on one day, April 1, 2018 with the spot area of 10 MSH. It has been spotless since then, producing only minor activities. Note the formation of a sigmoid region to the east, which was also sluggish.

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

Detected by halocme, Submitted at 2018-04-07T05:23:46

2018-04-05T13:30:01 --> 2018-04-05T17:00:01

Slow eruption from the AR 12703 remnant. The big sigmoid to the east of this eruption somehow stayed intact.

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

Detected by halocme, Submitted at 2018-04-07T05:17:07

2018-04-04T08:40:13 --> 2018-04-04T10:40:13

A mini filament (prrominence) eruption triggered a highly deflected jet.

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

Detected by halocme, Submitted at 2018-04-07T05:11:10

2018-04-03T03:45:01 --> 2018-04-03T05:31:01

Initially looking like a jet, the ejected material traced closed field structure that was twisted.

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

Detected by halocme, Submitted at 2018-04-07T05:03:17

2018-04-02T10:15:01 --> 2018-04-02T11:25:01

A small eruption causing temporary dimming. This appears to be driven by cancellation of sub AR magnetic field.

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

Detected by halocme, Submitted at 2018-04-07T04:57:48

2018-04-01T15:50:25 --> 2018-04-01T16:50:25

This occurred in the northern part of AR 12703, where the magnetic configuration looked more or less open. The trajectory presumably reflected local magnetic field.

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

Detected by halocme, Submitted at 2018-04-07T04:51:38

2018-04-01T03:00:09 --> 2018-04-01T04:00:09

A small but explosive eruption in the following part of AR 12703, producing short-lived double ribbons with dimming in between.

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

Detected by gchintzo, Submitted at 2018-03-28T02:29:50

2018-03-23T00:00:09 --> 2018-03-24T06:10:09

A coronal cavity at the east limb of the sun containing a prominence. The prominence undergoes an interesting evolution of its shape.