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

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

Detected by cheung, Submitted at 2012-04-05T18:12:10

2012-04-02T00:30:04 --> 2012-04-03T20:30:04

Magnetic field lines from AR 11143 (in the northern hemisphere) appear to be sucked into a coronal null point or spine. Apart from intermittent coronal jets, this type of reconnection results in magnetic lopos that straddle the equator. This is a candidate for direct observational evidence of cross-equatorial magnetic reconnection taking plane in the corona.

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

Detected by cheung, Submitted at 2012-04-05T18:12:09

2012-04-02T00:30:04 --> 2012-04-03T20:30:04

Magnetic field lines from AR 11143 (in the northern hemisphere) appear to be sucked into a coronal null point or spine. Apart from intermittent coronal jets, this type of reconnection results in magnetic lopos that straddle the equator. This is a candidate for direct observational evidence of cross-equatorial magnetic reconnection taking plane in the corona.

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

Detected by anny, Submitted at 2012-04-05T03:26:43

2012-03-30T11:38:04 --> 2012-03-30T19:20:04

One end of a large filament appears to lift up, swirl around, making a cone-like shape in the plane of the sky, and seemingly reconnects to some other part on the disk.

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

Detected by anny, Submitted at 2012-04-03T02:07:22

2012-03-29T09:24:04 --> 2012-03-29T10:40:04

A spray surge is thrown upward by a flare. When it seemingly gets disconnected from the photosphere, a second flare takes place in about the same location on the limb. Then the first blob completely disappears in 60 seconds and as it happens, a second blob appears pointed in a slightly different direction and slightly offset but at about the same height. It is unclear at first sight whether it is an extremely fast transverse motion or an extremely fast decay and appearance of the second surge.

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

Detected by berger, Submitted at 2012-04-02T17:48:46

2012-03-26T18:00:04 --> 2012-03-27T04:00:04

Large eruption and coronal wave from behind East limb. The event generated a Type II burst but is apparently too far behind the limb to contribute a major X-ray signature. Note that there are two subsequent filament eruptions on the disk that appear to take place in response to the coronal wave.

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

Detected by berger, Submitted at 2012-04-02T17:48:45

2012-03-26T18:00:04 --> 2012-03-27T04:00:04

Large eruption and coronal wave from behind East limb. The event generated a Type II burst but is apparently too far behind the limb to contribute a major X-ray signature. Note that there are two subsequent filament eruptions on the disk that appear to take place in response to the coronal wave.

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

Detected by schryver, Submitted at 2012-03-06T01:30:22

2012-03-03T17:00:04 --> 2012-03-04T05:00:04

Eruption and small flare just inside the NE limb, with a very unusual (and pretty) set of post-event loops: sharply-cusped loops towards the N and a strongly-inclinded glowing arcade towards the S (over a region where a smallish eruption seems to have started the sequence).

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

Detected by schryver, Submitted at 2012-03-06T01:21:23

2012-03-02T06:36:04 --> 2012-03-03T00:00:04

Flare in an AR just over the NE limb. Loop systems are seen to reconfigure for hours prior to the flare, and post-eruption loop system shows subsequent continued evolution. A helmet over a pair of arcade-like configurations suggest the presence of a null point above the flaring region.

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

Detected by schryver, Submitted at 2012-02-10T03:19:56

2012-02-09T17:52:04 --> 2012-02-10T00:00:04

Large prominence eruption on NE limb, associated with transient coronal holes, flare ribbons, and what looks like an induced, delayed eruption from an adjacent QS filament. In the distance, a set of weakened ARs exhibits a 'discoloration', i.e. a transient thermal restructuring, potentiall related to the limb eruption.

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

Detected by anny, Submitted at 2012-01-14T03:31:30

2012-01-12T19:22:04 --> 2012-01-13T00:00:04

Large filament takes off northwards; both footpoints appear to have small filaments on their own, which persist after the main eruption.

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

Detected by schryver, Submitted at 2012-01-06T01:19:55

2012-01-03T00:00:04 --> 2012-01-03T19:56:04

Loops extending southward from a small AR, still emerging, reconfigure, possibly reconnecting through a null point, at least sliding past what looks to be a separatrix surface.

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

Detected by schryver, Submitted at 2011-12-29T23:19:09

2011-12-25T01:45:04 --> 2011-12-25T21:50:04

Emerging flux with a series of flares/eruptions.

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

Detected by schryver, Submitted at 2011-12-29T23:12:44

2011-12-25T05:55:04 --> 2011-12-25T11:20:04

A QS filament eruption occurs close in time (within 30 min.) to an over-the-limb eruption, followed (within 30 min.) by a high-C flare with a pronounced 'coronal wave' associated with the eruption.

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

Detected by schryver, Submitted at 2011-12-29T22:54:45

2011-12-24T22:15:04 --> 2011-12-25T02:00:04

QS filament eruption with beuatiful liftoff and formation of eruption ribbons, with later 171A glow at the ends of the apparent flux rope.

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

Detected by asainz, Submitted at 2011-12-20T02:09:58

2011-12-17T10:20:04 --> 2011-12-17T11:50:04

Beautiful CME occurs in the limb, in fact it seems that is taking place in the back of th Sun.

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

Detected by asainz, Submitted at 2011-12-20T01:38:14

2011-12-18T08:20:04 --> 2011-12-18T19:10:04

An interisting filament activation propagates through surroundings. Later, a couple of smalls flares occur in the left part of the image.

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

Detected by cheung, Submitted at 2011-12-16T00:57:35

2011-12-15T23:36:08 --> 2011-12-16T00:04:56

Comet Lovejoy fragments and evaporates while in AIA's field of view.

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

Detected by anny, Submitted at 2011-11-18T21:42:32

2011-11-17T22:14:04 --> 2011-11-18T00:00:04

Spectacular prominence eruption on the W limb. The tip of the erupting plasma is clearly observed. The prominence seems to folow the path of the open field lines above a small dipole, that is, the 'outer' lines in a Y-type current sheet.

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

Detected by anny, Submitted at 2011-11-15T00:55:35

2011-11-14T00:00:04 --> 2011-11-14T21:00:04

A pretty eruption of limb part of a very long filament. One end of the filament, that was a bit elevated before and showed some signs of activity in the previous day, lifted up high and the plasma on its tip has fallen down as coronal rain along two opposite trajectories forming an owl-like shape (called such by Camilla SDO :)). Remainings of the filament sunk down and got re-attached to the surface. It is worth mentioning that some time prior to this event there was a bubble eruption on the W limb which triggered a coronal wave - this filament event seems to take place shortly after the wave would have reached it.

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

Detected by schryver, Submitted at 2011-11-09T19:21:25

2011-11-09T12:51:34 --> 2011-11-09T14:51:04

A compact filament rises, and erupts, likely forming a CME, propagating towards the NE from the NE quadrant.