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

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

Detected by halocme, Submitted at 2013-01-04T17:16:42

2013-01-01T00:10:11 --> 2013-01-01T00:50:11

This annotator (halocme) happens to be assigned for a generally CME-quiet period, but LASCO data sometimes show CMEs. For example, refer to the C2 difference image 01:25-00:48, which marks an unimpressive but broad CME from NE, making me wonder what its origin is. This AIA movie may show a marginal indication of the eruption between 00:24 and 00:46 to maybe wishful eyes. From STB, the source region is N20E15, meaning it is 56 degrees behind the east limb from Earth view.

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

Detected by halocme, Submitted at 2013-01-04T15:54:34

2012-12-31T02:50:23 --> 2012-12-31T04:31:11

The origin seems to be a region 5-10 degrees behind the limb. The propagation is preferentially northward. Alas, the cadence of EUVI on STB is reduced to 10 minutes.

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

Detected by halocme, Submitted at 2013-01-04T05:41:44

2012-12-29T13:30:35 --> 2012-12-29T15:00:35

STB images show that the source region of this eruption is 20 degs behind the limb, but a significant velocity component away from the plane of the sky makes it easier to see the eruption from Earth view. Only a minor CME is seen by LASCO.

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

Detected by halocme, Submitted at 2013-01-03T19:26:31

2012-12-26T16:50:23 --> 2012-12-26T18:30:23

This is not a big eruption, but the region to the north is seen to oscillate as the filament gets erupted. Dimming is also clear high in the corona, resulting in a minor CME. Only at 304 A do we see material fall back.

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

Detected by halocme, Submitted at 2013-01-03T17:14:08

2012-12-26T07:20:23 --> 2012-12-26T08:20:23

The erupting filament appears bright at 304 A and dark at 211 A. At a certain stage, it looks slinky-like, but it is not clear whether it represents a true twist. This movie shows how the eruption propagates into and transforms the corona above to become a CME.

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

Detected by schryver, Submitted at 2013-01-03T00:59:32

2012-12-25T08:52:35 --> 2012-12-25T12:40:35

A filament is seen to rise and erupt from just inside the E limb in a region that erupted similarly on 2012/12/23 when it was still just behind the l imb.

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

Detected by anny, Submitted at 2012-12-22T03:17:03

2012-12-21T05:28:03 --> 2012-12-21T10:52:03

A large pretty filament eruption at the S limb. The Sun clearly does not know much of the Maya calendar so the eruption is not directed earthwards.

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

Detected by schryver, Submitted at 2012-12-13T18:32:28

2012-12-12T19:25:03 --> 2012-12-13T10:00:03

A QS filament (connecting to a small near-equatorial AR) erupts. There is a dark cusp-like shape on the eastern leading edge of the coronal reconfiguration. Some 11h after the initial eruption started, a second occurs, now at the eastern end of the original eruption.

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

Detected by schryver, Submitted at 2012-12-12T23:21:41

2012-12-11T14:00:03 --> 2012-12-11T17:32:03

A repeatedly activation QS filament in the NE erupts simultaneously with a relatively compact decayed AR in the S hemisphere.

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

Detected by cheung, Submitted at 2012-12-10T18:19:29

2012-12-04T04:00:03 --> 2012-12-04T11:00:03

A filament straddling the horizon of the southeast limb erupts. The morphology of the erupting filament resembles an untwisting ribbon.

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

Detected by cheung, Submitted at 2012-12-10T18:14:19

2012-12-03T12:00:03 --> 2012-12-03T15:00:03

This odd shaped surge results from the reconfiguration of an existing filament. The impulsive reconfiguration seems to channel filament material into curved magnetic field lines before the material drains back down due to gravity.

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

Detected by cheung, Submitted at 2012-12-10T18:14:18

2012-12-03T12:00:03 --> 2012-12-03T15:00:03

This odd shaped surge results from the reconfiguration of an existing filament. The impulsive reconfiguration seems to channel filament material into curved magnetic field lines before the material drains back down due to gravity.

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

Detected by anny, Submitted at 2012-12-04T00:15:21

2012-11-29T17:36:03 --> 2012-11-29T20:33:03

A large filament eruption on the limb very close to the S pole.

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

Detected by anny, Submitted at 2012-11-27T01:58:55

2012-11-21T08:00:03 --> 2012-11-21T22:54:03

This filament eruption would be unremarkable if not the fact that it happens at the pole (in the plane of sky projection) and the flux rope takes off northwards (again, as appears in the projection).

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

Detected by schryver, Submitted at 2012-11-26T17:49:11

2012-11-25T00:20:03 --> 2012-11-25T03:08:03

Filament eruption from just N of a decaying compact AR.

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

Detected by schryver, Submitted at 2012-11-26T17:01:13

2012-11-23T20:04:03 --> 2012-11-23T23:28:03

An eruption on the E limb causes oscillations in high-arching transequatorial loops.

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

Detected by anny, Submitted at 2012-11-22T00:55:30

2012-11-20T11:39:03 --> 2012-11-20T14:48:03

A relatively large eruption on the W limb. The footpoint appears to be of conical shape and unswirling motions are clearly observed along it.

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

Detected by schryver, Submitted at 2012-11-17T01:25:16

2012-11-15T04:04:07 --> 2012-11-15T06:28:07

A compact AR flares and ejects a narrowly focused jet to a neighboring region, exciting some oscillations in the process.

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

Detected by schryver, Submitted at 2012-11-15T22:26:06

2012-11-14T02:38:35 --> 2012-11-14T06:02:35

A very compact AR displays three bright flares (with clear diffraction stars) in rapid succession in three different places within the multipolar region in the SE quadrant.

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

Detected by anny, Submitted at 2012-11-12T20:56:22

2012-11-10T22:03:03 --> 2012-11-11T01:45:03

Large prominence eruption on the SW limb.