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

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

Detected by schryver, Submitted at 2014-10-14T22:17:23

2013-01-13T21:35:35 --> 2013-01-14T07:50:35

Filament activation, with beautiful (but fast) wrapping motions.

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

Detected by schryver, Submitted at 2014-10-14T22:16:51

2014-08-24T11:16:03 --> 2014-08-24T16:48:03

A mid-M clas flare near the E limb, associated with a large eruption, occurs synchronously with perturbations in a region halfway towards the W limb. Associated with the eruption from the E limb are oscillations in the high-coronal field. Shortly afterwards, a QS filament erupts from the S hemisphere, possibly in response to these preceding events.

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

Detected by schryver, Submitted at 2014-10-14T22:16:43

2014-04-16T08:28:03 --> 2014-04-16T14:28:03

Slowly progressing high-latitude SE-limb eruption with a pronounced 'cavity' forming and subsequent rotation of the lower parts of the erupting configuration.

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

Detected by schryver, Submitted at 2014-10-14T22:16:42

2014-01-20T20:16:03 --> 2014-01-21T00:00:03

E-limb eruption

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

Detected by schryver, Submitted at 2014-10-14T22:16:41

2012-11-02T15:00:03 --> 2012-11-03T00:00:03

Eruption of a prominence configuration off the NW limb, with hot coronal rain impacting the on-disk quiet Sun.

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

Detected by schryver, Submitted at 2014-10-14T22:16:24

2010-12-06T17:08:00 --> 2010-12-06T21:00:12

Coronal rain following the eruption of a large QS filament. The rain appears to follow field lines associated with the rope's initial structure rather than landing elsewhere (as in the 2011/06/07 eruption).

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

Detected by schryver, Submitted at 2014-10-14T22:16:21

2014-01-20T18:56:03 --> 2014-01-20T21:28:03

The interconnecting loops between two small, adjacent bipolar regions erupts, with flare ribbons, dimming, reconfiguration, and a propagating front primarily in the NW direction. That propagating disturbance appears to reflect off the QS/CH interface nearby, moving back and expanding into a wider opening angle as it moves towards the S and E.

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

Detected by schryver, Submitted at 2014-10-14T22:16:05

2012-12-23T19:08:35 --> 2012-12-23T23:48:35

An eruption occurs in the northern reaches of a N-hemisphere AR. There is no obvious filament in 211/193/171, but a clear post-eruption arcade. The perturbed field couples into QS field NE-ward of the region, and apparently even well eastward of that.

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

Detected by anny, Submitted at 2014-09-16T21:40:31

2014-08-05T15:12:03 --> 2014-08-05T18:09:03

A small and otherwise unremarkable spray surge results in the wave-like brightening in the quiet sun region to the North of the surge. A possible interpretation is the existing long-distance connectivity between the site of the surge (periphery of an AR on one side, the end of a filament on the other) and the northern quiet sun region. 171A and 211A did not show any prior evidence to such a connectivity.

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

Detected by halocme, Submitted at 2014-09-14T05:36:12

2014-09-12T16:00:03 --> 2014-09-12T22:00:03

An inverse-S was clear prior to the slow eruption. Coronal dimming is noted in 211 A images. These images emphasize the effects of the eruption rather than the initial part of the eruption - but examine the 304 A images between 17:30 and 17:50 UT.

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

Detected by halocme, Submitted at 2014-09-14T05:36:12

2014-09-12T16:00:03 --> 2014-09-12T22:00:03

An inverse-S was clear prior to the slow eruption. Coronal dimming is noted in 211 A images. These images emphasize the effects of the eruption rather than the initial part of the eruption - but examine the 304 A images between 17:30 and 17:50 UT.

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

Detected by halocme, Submitted at 2014-09-13T23:03:56

2014-09-10T16:30:35 --> 2014-09-10T18:30:35

This eruption resulted in an Earth-directed CME, which arrived at L1 46 hours later. The active region (AR 12158) was not so extended, but it contained a delta configuration. The eruption accompanied other expected signatures (such as LCPF, dimming, loop oscillations, etc.)for this magnitude.

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

Detected by cheung, Submitted at 2014-09-10T21:40:31

2014-09-07T19:30:04 --> 2014-09-07T20:58:04

A nice C7.8 flare from AR 12157. The lack of a coronal dimming and the passiveness of neighboring loop structures suggest this flare is confined (i.e. no ejection of material out of the AR).

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

Detected by cheung, Submitted at 2014-09-10T21:40:30

2014-09-07T01:40:04 --> 2014-09-07T05:10:04

Hot loops (in the 94 channel, red) appear above the arcade loops following the flare.

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

Detected by cheung, Submitted at 2014-09-03T21:40:40

2014-09-03T13:20:03 --> 2014-09-03T16:10:03

The footpoints of the loops associated with this flare are occulted by the limb. There are no clear signatures of a coronal mass ejection.

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

Detected by halocme, Submitted at 2014-08-19T00:40:48

2014-08-15T15:20:23 --> 2014-08-15T20:20:23

Compared with the marginal eruption on the previous day, this seems to be a big event in the sense that the filament is clearly seen to erupt and traceable to a large distance. We also see spreading two-ribbon emission and dimming. We are predicting this to be Earth-affecting.

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

Detected by halocme, Submitted at 2014-08-19T00:40:45

2014-08-15T15:20:23 --> 2014-08-15T20:20:23

Compared with the marginal eruption on the previous day, this seems to be a big event in the sense that the filament is clearly seen to erupt and traceable to a large distance. We also see spreading two-ribbon emission and dimming. We are predicting this to be Earth-affecting.

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

Detected by anny, Submitted at 2014-08-14T00:40:28

2014-07-22T11:00:03 --> 2014-07-22T19:42:03

A large prominence eruption with associated cavity eruption on the NW limb.

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

Detected by anny, Submitted at 2014-08-04T20:02:48

2014-07-10T00:00:03 --> 2014-07-10T08:40:03

A large filament eruption on the W limb, followed by the "openning" of the surrounding 211A structures.

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

Detected by halocme, Submitted at 2014-07-11T05:15:10

2014-07-08T16:00:03 --> 2014-07-08T18:20:27

The propagation was mostly along the limb, more clockwise than counterclockwise. It went beyond the north pole.