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

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-08-19T00:04:15

2014-08-14T17:00:03 --> 2014-08-14T22:00:03

In H-alpha movies a filament was seen to disappear during this time frame. However, none of the AIA channels clearly show an eruption. Moreover the ribbon-like brightening seems to be absent. Therefore the filament may have not erupted.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-08-14T00:40:29

2014-07-21T16:57:03 --> 2014-07-21T21:45:03

A very bright spray surge on the E limb, in what seems to be an active region. The surge is bright enough to make diffraction pattern visible in 304A channel. There is no evidence of an associated eruption. However, this surge is immediately followed by a dimmer surge nearby, suggesting a magnetic connectivity between the two sites.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-08-14T00:40:29

2014-07-22T17:00:03 --> 2014-07-23T05:09:03

Following the filament eruption annotated earlier, one of the footpoints of the flux rope persists for a short time, spinning around, wiggling, and eventually falling apart (that's what it literally looks like), with its remnants spread on both sides of the limb.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-08-14T00:40:27

2014-07-22T22:39:03 --> 2014-07-23T16:54:03

A small tornadoe-shape prominence on the E limb quickly forms, quickly falls back down as a coronal rain, but gets reborn almost right away.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-08-04T20:03:02

2014-07-30T16:40:03 --> 2014-07-30T18:50:03

This confined eruption has an intersting morphology. There is a set of closed loops threaded with filamentary material. Adjacent to these closed loops are a set of predominantly radial loops. It almost looks like a giant jet in this regard.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-08-04T20:03:02

2014-07-30T02:50:03 --> 2014-07-30T08:50:03

A long-winding quiescent filament is released, leading to a pair of long, convoluted ribbons.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-08-04T20:03:01

2014-07-29T23:50:03 --> 2014-07-30T01:20:03

This jet-like episode seems to be accompanied by collapsing field lines following reconnection.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-08-04T20:03:01

2014-07-29T09:40:35 --> 2014-07-29T11:30:35

This filament eruption originates from AR 12121

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-08-04T20:03:01

2014-07-28T02:50:35 --> 2014-07-28T03:40:35

This filament was sitting above a polarity inversion line between some network flux, likely from decayed ARs.Even though its an 'quiescent' filament eruption, there is still a post-eruption arcade.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-08-04T20:02:59

2014-07-16T22:30:03 --> 2014-07-17T01:30:03

Some filamentary material is injected into loops and then falls back down the other side.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-08-04T20:02:59

2014-07-28T08:10:35 --> 2014-07-28T09:40:35

The dense absorbing plasma is seens to swirl around and then drain back to the footpoints.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-08-04T20:02:57

2014-07-30T16:40:03 --> 2014-07-30T18:50:03

This confined eruption has an intersting morphology. There is a set of closed loops threaded with filamentary material. Adjacent to these closed loops are a set of predominantly radial loops. It almost looks like a giant jet in this regard.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-08-04T20:02:57

2014-07-29T23:50:03 --> 2014-07-30T01:20:03

This jet-like episode seems to be accompanied by collapsing field lines following reconnection.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by derosa, Submitted at 2014-08-04T20:02:55

2014-07-04T05:00:03 --> 2014-07-04T09:00:03

A small eruption occurs in AR12106, and as the effects of the eruption travel north, oscillations in the nearby coronal cells are affected. Curiously, some intervening loop structures seem to be unaffected.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by derosa, Submitted at 2014-08-04T20:02:54

2014-07-24T00:00:03 --> 2014-07-25T15:00:03

This emerging flux region on the limb causes some nice loop dynamics, visible here for more than a day. Additionally, the activity associated with the chromospheric material in the foreground makes these dynamics even more cool (double meaning intended). A prominence south of the emerging flux region is also fairly active.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by derosa, Submitted at 2014-08-04T20:02:54

2014-07-24T00:00:03 --> 2014-07-25T15:00:03

This prominence stays active for at least 36h. AR12121 (which produced a couple of C flares) is also in the ROI.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by derosa, Submitted at 2014-08-04T20:02:53

2014-07-25T18:00:03 --> 2014-07-25T23:00:03

A small filament within an active region erupts, and then gets trapped by overlying magnetic fields, at which point the cool filamentary material is then observed to stream back down.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by derosa, Submitted at 2014-08-04T20:02:52

2014-07-24T00:00:03 --> 2014-07-25T15:00:03

This emerging flux region on the limb causes some nice loop dynamics, visible here for more than a day. Additionally, the activity associated with the chromospheric material in the foreground makes these dynamics even more cool (double meaning intended). A prominence south of the emerging flux region is also fairly active.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-08-04T20:02:51

2014-07-09T10:02:03 --> 2014-07-09T11:06:03

A rapid brightening at the footpoint is followed by the formation of a spray surge. At first emitting in 304A, it quickly stretches rather far off its footpoint and becomes optically thick in the same channel.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-08-04T20:02:47

2014-07-09T17:06:03 --> 2014-07-09T18:38:03

A large filament erupts close to the disk center and heads eastwards. It obviously carries enough momentum to destabilize the entire Sun Or maybe that is due to an AIA pointing adjustment. Who knows.