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 2017-05-06T19:33:58

2017-04-28T13:55:13 --> 2017-04-28T15:01:13

At low temperatures, this event looks like a mini filament (prominence) eruption, but in 211 A channel (especially in running difference images, not shown here) it is more like a jet. Perhaps another example to suggest the intimacy between these two phenomena.

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

Detected by halocme, Submitted at 2017-05-06T19:33:57

2017-04-28T13:55:13 --> 2017-04-28T15:01:13

At low temperatures, this event looks like a mini filament (prominence) eruption, but in 211 A channel (especially in running difference images, not shown here) it is more like a jet. Perhaps another example to suggest the intimacy between these two phenomena.

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

Detected by halocme, Submitted at 2017-05-06T19:25:29

2017-04-27T00:10:13 --> 2017-04-27T01:00:13

One jet close to the limb was followed by another with clearer footpoint brightening. These may be nothing special, but they are more easily discernible than others.

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

Detected by jinmeng, Submitted at 2017-04-28T21:17:24

2017-04-26T02:10:09 --> 2017-04-26T04:00:09

A failed eruption was observed at the west limb.

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

Detected by jinmeng, Submitted at 2017-04-28T21:11:06

2017-04-25T11:40:09 --> 2017-04-25T21:26:09

A filament eruption was observed near the west limb. Although seems like a failed eruption, it did lead to a reconfiguration of the surroudning coronal field.

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

Detected by jinmeng, Submitted at 2017-04-28T20:51:12

2017-04-26T16:34:09 --> 2017-04-26T20:30:09

An eruption was observed in AR 12653, which seems like a failed filament eruption.

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

Detected by jinmeng, Submitted at 2017-04-28T20:41:31

2017-04-24T00:00:09 --> 2017-04-24T15:40:09

A filament eruption was observed near the east limb. The eruption influenced a large area, which leaded to a reconfiguration of coronal field. a narrow coronal hole to the NW of the filament disappeared after the eruption.

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

Detected by jinmeng, Submitted at 2017-04-28T18:47:57

2017-04-23T15:30:09 --> 2017-04-23T21:14:09

The eruption started from a decaying active region near the north pole. The filament materialwas first transfered to a region to the north of the active region and then erupted.

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

Detected by jinmeng, Submitted at 2017-04-28T18:36:03

2017-04-21T00:00:09 --> 2017-04-22T13:20:09

Multiple eruptions were observed from AR 12651&12652. A nearby quiet-Sun filament was also erupted during the period.

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

Detected by jinmeng, Submitted at 2017-04-28T18:36:02

2017-04-21T00:00:09 --> 2017-04-22T13:20:09

Multiple eruptions were observed from AR 12651&12652. A nearby quiet-Sun filament was also erupted during the period.

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

Detected by halocme, Submitted at 2017-04-22T10:10:13

2017-04-20T20:30:01 --> 2017-04-20T23:00:01

This seems to be a classic filament eruption, resulting in the formation of separating chromospheric ribbons. It occurred next to a decayed active region without spots. The associated CME was mostly toward north (see http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170420.221207.w054.v0227.p369&frame=15&r).

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

Detected by halocme, Submitted at 2017-04-22T09:56:21

2017-04-20T15:55:13 --> 2017-04-20T17:31:13

This gives an impression that one leg (north) of the filament got loose and erupted. It was located in a quiescent region detached from AR 12651. The eruption was associated with a CME (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170420.171207.w057.v0336.p077&frame=14&r).

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

Detected by halocme, Submitted at 2017-04-22T09:46:16

2017-04-18T18:55:14 --> 2017-04-19T02:01:14

The flare lasted long, and as expected, was associated with a more decent CME than the previous flare. This one does not show clear coronal waves, and the expansion was more in the radial than horizontal directions. After the peak downward motions are seen from the top of the arcade which is hot. Shortly after the eruption, big motions were seen, but these are image motions. Indeed, the peak of the flare coincided with AIA weekly calibration.

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

Detected by halocme, Submitted at 2017-04-22T09:46:16

2017-04-18T18:55:14 --> 2017-04-19T02:01:14

The flare lasted long, and as expected, was associated with a more decent CME than the previous flare. This one does not show clear coronal waves, and the expansion was more in the radial than horizontal directions. After the peak downward motions are seen from the top of the arcade which is hot. Shortly after the eruption, big motions were seen, but these are image motions. Indeed, the peak of the flare coincided with AIA weekly calibration.

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

Detected by halocme, Submitted at 2017-04-22T09:32:37

2017-04-18T09:20:25 --> 2017-04-18T10:50:25

AR 12644, which produced M-class flares on 1-2 April 2017 came back as AR 12651, producing two C-class flares on 18 April 2017. The first one was associated with a mediocre CME, but it accompanied a coronal wave propagating along the limb (counterclockwise) and into the disk.

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

Detected by gchintzo, Submitted at 2017-04-21T22:03:37

2017-04-17T18:10:09 --> 2017-04-18T00:00:09

A third occurence of a jet-like CME eruption originating from this source region on the East limb (320km/sec; http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170417.222407.w015.v0322.p091&frame=9&r). Same as previously, a confined eruption is followed by a more extended eruption.

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

Detected by gchintzo, Submitted at 2017-04-21T21:56:53

2017-04-17T10:00:09 --> 2017-04-17T18:00:09

The source region of a jet-like CME observed by LASCO (321 km/sec; http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170417.154807.w019.v0321.p090&frame=11&r). Same as in previous entry, a confined filament eruption is followed by an eruption which exceeds AIA's field of view.

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

Detected by gchintzo, Submitted at 2017-04-21T20:55:05

2017-04-17T05:00:09 --> 2017-04-17T10:50:09

The source region of a jet-like ejection seen in the LASCO observations ( ~400km /sec http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170417.080007.w024.v0404.p090&frame=10&r). A jet-like confined eruption is followed by a rapid dimming in the overlying corona suggesting a non-radial eruption. However, the ejection seen in LASCO from this part of the Sun shows a more radial-like jet-like CME.

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

Detected by gchintzo, Submitted at 2017-04-20T21:10:16

2017-04-17T02:40:09 --> 2017-04-18T00:00:09

A coronal hole around the equatorial region of the sun

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

Detected by jinmeng, Submitted at 2017-04-12T01:28:27

2017-04-10T18:00:09 --> 2017-04-10T20:28:09

A solar flare was observed near the east limb. It seems that this flare did not associate with a CME.