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

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

Detected by schryver, Submitted at 2014-10-14T22:17:42

2014-04-18T04:04:03 --> 2014-04-18T18:00:03

A long-lived polar-crown filament activates in association with an eruption from a QS region south of an AR towards the north of both. Then an M7 flare and eruption occurs that leads to oscillations and distortions in the polar-crown filament, which subsequently loses its configuration and disappears as much of its cool material slides towards the W and N to a QS region just on the li mb.

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

Detected by schryver, Submitted at 2014-10-14T22:17:42

2014-01-02T09:04:03 --> 2014-01-02T11:32:03

A near-equatorial QS filament erupts from near the W limb. Synchronously, an AR filament near DC activates, as does a filament SE of the primary eruption. A fragment of a prominence to the S of the eruption exhibits briefly oscillations.

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

Detected by schryver, Submitted at 2014-10-14T22:17:41

2014-01-01T18:28:03 --> 2014-01-01T21:04:03

An M9 flare from a region in the SW quadrant associated with a filament eruption, with much (most?) of the material falling back onto the surface.

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

Detected by schryver, Submitted at 2014-10-14T22:16:49

2014-06-15T10:36:03 --> 2014-06-15T15:48:03

An eruption from a region at the SW limb couples into QS field much of the way towards the south polar zone, with high coronal perturbations propagating over almost an entire quadrant.

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

Detected by schryver, Submitted at 2014-10-14T22:16:49

2014-04-28T01:04:03 --> 2014-04-28T21:20:03

Although the AIA 171/193/211 images show no direct evidence of a large-scale, slow eruption, the 'discoloration', as a signature of thermal changes in the quiet-Sun corona, are reminiscent of those typically seen during eruptions. The 304 channel shows a long, thin, multistranded filament erupting, and SOHO/LASCO C2 data show a large, northward CME at what appears to be the corresponding location and time.

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

Detected by schryver, Submitted at 2014-10-14T22:16:44

2014-04-16T18:16:03 --> 2014-04-16T21:48:03

A short filament trailing an AR erupts, immediately followed by an eruption of a filament configuration leading that AR, associated with loop oscillations in the AR between these two events.

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

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

2014-01-21T16:04:03 --> 2014-01-21T21:20:03

Eruption from a decayed region, associated with a pronounced propagating front, and later in the process distant, high oscillating loops.

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

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

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

Detected by schryver, Submitted at 2014-10-14T22:16:25

2012-10-11T00:20:03 --> 2012-10-11T12:32:03

A series of four rather insignificant eruptions from a moderate-sized AR rock the connections from that AR to a leading AR near the limb, in the process sending off coronal propagating fronts of which the last one travels over a good part of the disk. ....

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

Detected by schryver, Submitted at 2014-10-14T18:43:01

2014-09-25T00:00:03 --> 2014-09-26T00:00:03

Emerging flux region causing reconnection with adjacent coronal hole, proceeding in spurts with interesting patterns between the network concentrations of photospheric magnetic field. ?

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

Detected by halocme, Submitted at 2014-09-13T23:09:27

2014-09-10T16:50:23 --> 2014-09-10T19:10:47

The big eruption from AR 12158 produced a spectacular, nearly circular LCPF. Some noted a counter-clockwise rotation, but can that be a spurious effect of running difference images?

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

Detected by halocme, Submitted at 2014-09-13T23:03:57

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

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

2014-09-08T22:40:04 --> 2014-09-09T06:10:04

Beautifui ribbons and post-flare loops can be seen. In the declining phase of the flare, the red sheath (94) around the yellow loops (193) suggests the higher loops are hotter than lower ones.

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

Detected by cheung, Submitted at 2014-09-03T22:40:29

2014-09-01T21:40:04 --> 2014-09-01T22:50:04

This one occured just a few hours following a previous eruption from what seems like the same source region behind the limb. Unlike the previous eruption, this one launched a more pronounced coronal wave.

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

Detected by cheung, Submitted at 2014-09-03T22:40:29

2014-09-01T13:50:04 --> 2014-09-01T17:50:04

An eruption from behind the east limb. Red, green and yellow colors indicate signal in the 94, 335 and 193 channels, respectively. The eruption leaves behind a V-shaped void in the 193 image (yellow). The flanks of this V-shaped void have enhanced 94 brightness, which is likely due to plasma heated following the eruption. Another eruption follows a few hours later.

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

Detected by cheung, Submitted at 2014-09-03T22:40:28

2014-09-01T21:40:04 --> 2014-09-01T22:50:04

This one occured just a few hours following a previous eruption from what seems like the same source region behind the limb. Unlike the previous eruption, this one launched a more pronounced coronal wave.

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

Detected by cheung, Submitted at 2014-09-03T22:40:27

2014-09-01T10:50:04 --> 2014-09-01T12:00:04

First tweeted by Halo CME https://twitter.com/halocme/status/506699165594689536

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

Detected by cheung, Submitted at 2014-09-03T21:40:39

2014-09-02T11:10:03 --> 2014-09-02T20:30:03

This giant filament eruption was first tweeted by Halo CME https://twitter.com/halocme/status/506894190932799488 The filament took many hours to rise through the corona, so it is probably not going to result in a very fast CME.

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

Detected by halocme, Submitted at 2014-08-19T00:40:49

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

Detected by cheung, Submitted at 2014-08-04T20:03:03

2014-07-28T05:10:35 --> 2014-07-29T11:00:35

The condensations in this region seem to appear at places where one may expect coronal nulls and/or separators.