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 2014-02-12T17:29:23

2014-02-11T00:28:35 --> 2014-02-11T10:20:35

Filament eruption

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

Detected by schryver, Submitted at 2014-02-12T17:24:07

2014-02-10T19:52:35 --> 2014-02-11T00:00:35

Off the E limb, sets of loops exhibit multiple pulse-like quasi-synchronous motions, wave-like in their displacements, but not obvisously oscillatory.

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

Detected by schryver, Submitted at 2014-02-12T17:08:50

2014-02-09T11:20:03 --> 2014-02-09T17:16:03

A region east of central meridian erupts (with ribbons and a mainly southward propagating perturbation seen best in the loops projecting onto the southern polar cap). Note that a filament activation in the region leading it (just west of CM) also exhibits a simultaneous activation, while a region approaching the W limb does also, all timed to within about 6 min. of each other.

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

Detected by weiliu, Submitted at 2014-02-10T02:14:40

2011-10-22T00:40:04 --> 2011-10-22T12:40:04

Large flux rope on the west limb eruped, acommpanied by a large surge toward the south and large post-flare loops, following an earlier filament eruption on the disk producing beautiful two-ribbon flare.

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

Detected by cheung, Submitted at 2014-02-10T02:14:33

2012-04-26T00:40:04 --> 2012-04-26T03:20:04

A very pretty surge with much of the material falling back down.

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

Detected by cheung, Submitted at 2014-02-10T02:14:31

2012-04-07T17:45:04 --> 2012-04-07T23:40:04

More the the loops that are seen to shift here seem to be anchored on the far side of the solar disk.The shifting of the loops may be a response to the filament eruption (source region in the north) that occured earlier in the day.

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

Detected by cheung, Submitted at 2014-02-10T02:14:30

2012-04-07T13:50:04 --> 2012-04-07T22:15:04

This filament is clearly oscillating before it is ejected from the corona.

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

Detected by cheung, Submitted at 2014-02-10T02:14:26

2012-10-12T00:10:03 --> 2012-10-12T01:50:03

The lack of on-disk footpoint brightenings following the gravitational descent of material along the legs of the filament implies that the footpoints are anchored on the far side of the Sun.

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

Detected by cheung, Submitted at 2014-02-10T02:14:26

2012-05-29T20:20:04 --> 2012-05-30T03:50:04

This filament eruption occurs simultaneously with the one in the northeastern limb.

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

Detected by cheung, Submitted at 2014-02-10T02:14:25

2012-05-29T20:20:04 --> 2012-05-30T03:50:04

This filament eruption occurs simultaneously with the one in the northwestern limb.

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

Detected by cheung, Submitted at 2014-02-10T02:14:25

2012-04-24T06:50:04 --> 2012-04-24T09:20:04

THIS is a tornado In this filament eruption, the filament being launched is seen to expand and unwind over Alfvenic time scales. This event is visually reminiscent of magnetically driven jets in MHD simulations of accretion disks.

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

Detected by cheung, Submitted at 2014-02-10T02:14:24

2012-04-07T13:50:04 --> 2012-04-07T22:15:04

This filament is clearly oscillating before it is ejected from the corona.

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

Detected by anny, Submitted at 2014-02-05T02:26:26

2014-01-30T13:14:03 --> 2014-01-30T17:18:03

The Earth transit has clearly caused the large filament to erupt producing an EUV wave. The preceding M6.6 flare is purely coincidental.

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

Detected by anny, Submitted at 2014-02-05T02:02:20

2014-01-29T00:00:03 --> 2014-01-29T03:08:03

An explosive activity in one filament is immediately followed by eruption of a nearby larger filament.

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

Detected by anny, Submitted at 2014-02-01T02:57:56

2014-01-27T00:00:03 --> 2014-01-27T00:57:03

I'd like to call it an EUV wave, except for (a) it's at the S limb, (b) it shows in 304A but not in 171A and 211A. Perhaps, remnants of some erupted flux rope passed by?

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

Detected by cheung, Submitted at 2014-01-17T02:09:43

2014-01-16T11:30:03 --> 2014-01-16T14:15:03

Filament eruption from the southwest limb

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

Detected by cheung, Submitted at 2014-01-17T02:01:59

2014-01-13T06:15:03 --> 2014-01-13T12:30:03

This off-limb filament follows the launch of two other filament eruptions (one on-disk and another from the east limb).

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

Detected by cheung, Submitted at 2014-01-17T01:58:42

2014-01-13T04:30:03 --> 2014-01-13T06:50:03

This off-limb filament lifts off at around the same time as the on-disk filament. Thereafter, another filament in the northwestern limb lifts off.

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

Detected by cheung, Submitted at 2014-01-17T01:55:37

2014-01-13T04:30:03 --> 2014-01-13T09:45:03

This on disk filament seems to lift off at the same time as a smaller filament on the east limb. Thereafter, another filament in the northwestern limb lifts off.

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

Detected by halocme, Submitted at 2014-01-09T08:56:58

2014-01-07T17:50:23 --> 2014-01-07T19:50:23

This is a major eruption with a very fast (>2000 km/s) CME. The LCPF is faster than 1000 km/s as measured laterally. It interacted with quiescent regions near the south pole after the CME passed beyond the limb.