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

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

Detected by weiliu, Submitted at 2012-03-28T23:04:06

2012-03-13T10:50:04 --> 2012-03-13T11:10:04

A moderate-sized surges on the eastern hemisphere occurred at about the same time as a large-scale surge on the western hemisphere. Could there be any physical connections between these two remote events, like in sympathetic flares?

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

Detected by weiliu, Submitted at 2012-03-28T23:01:18

2012-03-13T10:50:04 --> 2012-03-13T11:10:04

A surge from the core of an active region near the northwest limb.

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

Detected by weiliu, Submitted at 2012-03-28T22:12:47

2012-03-12T11:40:04 --> 2012-03-12T17:20:04

Coronal rain above NE limb, condensing at the loop apex and falling along circular loops.

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

Detected by schryver, Submitted at 2012-03-27T17:18:29

2012-03-23T10:00:04 --> 2012-03-23T12:09:04

Eruption over SW limb, with subsequent coronal oscillations

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

Detected by schryver, Submitted at 2012-03-27T17:18:28

2012-03-23T10:00:04 --> 2012-03-23T12:09:04

Eruption over SW limb, with subsequent coronal oscillations

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

Detected by schryver, Submitted at 2012-03-27T17:15:19

2012-03-23T14:00:04 --> 2012-03-23T20:33:04

Prominence eruption from QS region over NW limb.

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

Detected by derosa, Submitted at 2012-03-26T23:42:09

2012-03-20T01:54:04 --> 2012-03-20T06:16:52

One small eruption appears to trigger another small eruption.

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

Detected by derosa, Submitted at 2012-03-26T23:24:41

2012-03-19T00:00:04 --> 2012-03-19T05:00:04

A dynamic prominence, that involves a filament apparently untwisting and erupting

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

Detected by berger, Submitted at 2012-03-26T18:13:39

2012-03-25T14:20:04 --> 2012-03-26T02:21:40

Two of the large mid-latitude filaments near the East limb interact to cause multiple eruptions. Small coronal cavities are visible above the filaments on the East limb.

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

Detected by berger, Submitted at 2012-03-26T17:37:41

2012-03-25T00:00:04 --> 2012-03-25T06:00:04

Moderate filament eruption on SE limb. Western side of filament seems to release to cause a "sling shot" effect of the filament upwards and to the East. Twisting motion evident throughout the event.

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

Detected by berger, Submitted at 2012-03-26T17:32:17

2012-03-25T09:35:04 --> 2012-03-25T23:30:04

C1.2 flare in AR 11438. Brightest kernel is at 12:45 UT but large-scale topological effects do not occur until ~14:30 UT. The reason seems to be that the initial flare causes a filament expansion that only slowly grows/rises until it collides with overlying coronal loops to then initiate rapid reconnection and "two-ribbon" flaring.

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

Detected by berger, Submitted at 2012-03-26T17:24:21

2012-03-25T19:10:04 --> 2012-03-26T00:00:04

Emerging flux just below AR 11442 causes a rapid rearrangement of coronal loop structure accompanied by a small flare. The flare did not register in the GOES data. The emerging flux apppears to grow to the West and collide with an existing separatrix dome to trigger the rearrangement.

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

Detected by berger, Submitted at 2012-03-26T17:11:24

2012-03-25T00:00:04 --> 2012-03-25T04:35:04

C3.0 flare from AR 11442 near disk center. The magnetic topology of this active region is interesting and the flare spreads rapidly from the center to the periphery to "circle around" the Northern half of the AR.

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

Detected by weiliu, Submitted at 2012-03-24T00:16:07

2012-03-11T21:20:04 --> 2012-03-11T23:20:04

Two surges, one on the east limb and the other on the western hemisphere, occur almost simultaneously. The eastern one appears much larger in size.

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

Detected by halocme, Submitted at 2012-03-22T21:28:14

2010-05-12T13:30:05 --> 2010-05-12T15:30:05

Not spectacular as expected of a B1.6 flare, but the disturbance front is at least seen along the limb.

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

Detected by halocme, Submitted at 2012-03-16T22:20:39

2012-02-23T07:30:00 --> 2012-02-23T09:00:00

The SolarSoft Latest Events page describes this event as "NW Limb Eruption, Partially Occulted, B6.4 LDE, EUVME/CME, SECCHI-Ahead EUVI Wave." But as I looked at EUVI science data, I found it was only marginally a wave.

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

Detected by halocme, Submitted at 2012-03-16T02:00:29

2012-01-19T11:00:04 --> 2012-01-19T16:00:04

A major eruption in the northeastern quadrant takes place close in time with two other eruptions in the northwestern quadrant. Are these regions somehow connected?

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

Detected by halocme, Submitted at 2012-03-15T22:12:42

2012-03-10T16:50:24 --> 2012-03-10T19:20:24

The global propagating front seems to have started earlier than mentioned in the previous report. But it seems that the region south of the flare was disturbed twice, possibly by a flare-related wave and then by the CME (just a speculation, which needs to be supported by more careful analysis.)

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

Detected by halocme, Submitted at 2012-03-15T21:59:12

2012-03-10T16:50:25 --> 2012-03-10T19:20:25

Compared with the M6.3 flare from 9-Mar-2012, this movie may give an impression that the large-scale eruption starts earlier in the flare development. Indeed, clear northwestward motions are seen around 17:22 UT. However, global waves seem to start only after 17:40 UT at a greater distance from the flare center, and southward moving fronts are more easily seen in difference images (as shown in the next movie.)

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

Detected by halocme, Submitted at 2012-03-15T17:19:00

2012-03-09T03:15:01 --> 2012-03-09T04:45:01

This movie shows that the initial brightening around 03:25 UT has little to do with the associated eruption, which seems to start only around 03:37 UT. Indeed the GOES light curve consists of an impulsive peak preceding the main flare. Of course it is possible that the apparently confined flaring at the earlier time somehow makes it easier for the main flare to be eruptive (e.g., via breakout).