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

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

Detected by anny, Submitted at 2012-11-14T02:15:32

2012-11-12T00:00:03 --> 2012-11-13T00:00:03

A day-long sequence of flares from otherwise unremarkable ethemeral region on the disk.

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

Detected by anny, Submitted at 2012-11-14T02:13:23

2012-11-12T09:12:03 --> 2012-11-12T10:57:03

A flare and contemporary brightening in the quiet sun happen first, then a jet could be seen taking off from the flare site followed by brightening in the filament between the flare site and the brightening in the quiet sun.

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

Detected by anny, Submitted at 2012-11-14T02:05:05

2012-11-12T03:03:03 --> 2012-11-12T08:06:03

Small filament erupts on the disk; an associated cavity in 211A shows up right before the eruption and takes off, too.

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

Detected by anny, Submitted at 2012-11-12T20:51:03

2012-11-11T12:27:03 --> 2012-11-11T17:33:03

Coronal dimming on the disk with no erupting structures visible. There is, however, a post-eruption-like arcade in 211A with appropriate footpoint brightening in 304A

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

Detected by schryver, Submitted at 2012-11-09T00:57:32

2012-11-07T02:32:03 --> 2012-11-07T07:20:03

A moderately-sized AR near central meridian erupts, leading to a dimming phenomenon no larger than about 0.1 Rsun, propagating northward from the AR.

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

Detected by schryver, Submitted at 2012-11-09T00:57:31

2012-11-07T02:32:03 --> 2012-11-07T07:20:03

A moderately-sized AR near central meridian erupts, leading to a dimming phenomenon no larger than about 0.1 Rsun, propagating northward from the AR.

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

Detected by schryver, Submitted at 2012-11-09T00:45:28

2012-11-06T06:52:03 --> 2012-11-06T12:48:03

Above a small AR at the W limb, a field configuration appears to 'roll' as it moves upward, with emission first dropping, then recovering.

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

Detected by schryver, Submitted at 2012-11-09T00:42:53

2012-11-06T00:00:03 --> 2012-11-06T02:16:03

Strong eruption from small bipole, with assiated 'dimming' and field oscillations.

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

Detected by derosa, Submitted at 2012-10-31T01:45:02

2012-10-29T12:00:03 --> 2012-10-29T21:00:03

A prominent prominence forms on the west limb when material is drawn into an omega-shaped feature that includes some twist.

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

Detected by derosa, Submitted at 2012-10-30T01:21:25

2012-10-28T05:00:03 --> 2012-10-28T17:00:03

Eruption of AR11594 on the west limb, showing a reasonably nice bubble and vortical motions.

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

Detected by halocme, Submitted at 2012-10-25T05:57:52

2012-10-21T19:20:23 --> 2012-10-21T23:20:23

This flare does not seem to be eruptive (incidentally, the X1.8 flare on 2012-10-23 from the same region was also confined), but LASCO saw a CME at first at 21:12 UT and it became quite bright at 21:36 UT. Then what is the origin of this CME? This is not clearly answered even with STB. One possibility may be the region about 30 degrees behind the limb.

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

Detected by halocme, Submitted at 2012-10-25T05:10:42

2012-10-20T22:10:11 --> 2012-10-20T23:40:11

This one, which looks broader, was seen 24 hours after the previous one.

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

Detected by halocme, Submitted at 2012-10-25T05:03:44

2012-10-19T22:10:11 --> 2012-10-19T23:40:11

This is a diffuse jet, but the movie clearly captures the associated footpoint brightening.

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

Detected by halocme, Submitted at 2012-10-25T04:55:58

2012-10-19T17:00:03 --> 2012-10-19T20:00:03

This eruption is similar to the previous event associated with a C3.6 flare, namely the main eruption is a collimated rather than loop-like structure. The oscillation is seen when another bright erupting structure hits the loops.

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

Detected by halocme, Submitted at 2012-10-25T04:37:17

2012-10-19T20:40:11 --> 2012-10-19T21:50:59

This is an eruption that involves surge-like motions. The CME resulting from this erution initially appears circular, perhaps indicating a shock wave, but it decays rapidly. Loop oscillations associated with the eruption may be more outstanding.

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

Detected by halocme, Submitted at 2012-10-25T01:40:59

2012-10-19T05:30:35 --> 2012-10-19T09:30:35

This eruption starts as a rising motion almost radially, at which stage a very narrow CME is seen. It changes to encompass a wider area and thus resulting in a wider CME. It is not clear how the downward motions are related with the onset of the CME.

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

Detected by halocme, Submitted at 2012-10-24T18:15:48

2012-10-19T01:40:11 --> 2012-10-19T03:00:11

The eruption is seen only at the tops of tall loops. 304 A images show mass injections at the legs of these loops around the time of the eruption.

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

Detected by anny, Submitted at 2012-10-17T00:45:59

2012-10-15T13:05:03 --> 2012-10-15T20:40:03

Despite its large size, this filament eruption is barely seen even in 304A channel.

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

Detected by derosa, Submitted at 2012-10-12T23:52:34

2012-10-08T09:00:03 --> 2012-10-09T06:00:03

Double eruption from the same active region about to rotate onto the disk. The first eruption is a quickie, and the second eruption is more of a full-fledged blowout.

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

Detected by derosa, Submitted at 2012-10-12T23:04:03

2012-10-07T18:00:04 --> 2012-10-08T15:00:04

A series of off-limb eruptions seen in 131 and 193 channels of AIA. The 131 emission [in red] is high both during the onset of the eruptions as well as when the post-eruption arcades are cooling, due to the fact that the response function for the AIA 131 channel has peaks both near 10 MK and 1 MK.