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 2013-09-23T21:13:50

2013-09-20T11:30:39 --> 2013-09-20T13:00:39

This is too diffuse to be recognized in intensity images. There are no clear signatures of the trigger or effect on the visible side. It is hard to determine if the vertical structure that is pushed sideways is rooted on this or the other side.

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

Detected by halocme, Submitted at 2013-09-23T17:33:44

2013-09-20T03:05:23 --> 2013-09-20T04:55:23

Only a small part of the filament went off, and most of the material appears to fall back. This event seems to be triggered by energy release down below in the form of heated turbulent motions.

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

Detected by halocme, Submitted at 2013-09-23T17:33:41

2013-09-20T03:05:23 --> 2013-09-20T04:55:23

Only a small part of the filament went off, and most of the material appears to fall back. This event seems to be triggered by energy release down below in the form of heated turbulent motions.

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

Detected by schryver, Submitted at 2013-09-23T15:40:19

2013-09-10T10:44:03 --> 2013-09-10T17:16:03

QS (polar crown?) filament eruption

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

Detected by cheung, Submitted at 2013-09-21T00:16:01

2013-09-17T13:50:03 --> 2013-09-17T15:40:03

In perhaps a confined eruption, a faint filament dissolves into the tenuous corona (some draining also occurs).

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

Detected by cheung, Submitted at 2013-09-19T23:07:34

2013-09-15T12:20:03 --> 2013-09-15T16:10:03

A slowing destabilizing filament seems to dissolve away, possibly due to heating of material out of the 304 passband.

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

Detected by cheung, Submitted at 2013-09-17T00:14:37

2013-09-14T13:20:03 --> 2013-09-14T16:40:03

This arch-shaped filament seems to disappear as it rises. There is some apparent draining motion, but the filament material vanishes out of the 304 passband before reaching the footpoints. This suggests some change in thermodynamic state.

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

Detected by cheung, Submitted at 2013-09-17T00:11:12

2013-09-14T21:50:03 --> 2013-09-15T01:40:03

A portion of a polar crown filament hops behind the limb and disappears. A possible (partial) explanation for the disappearing filament material could be that it was heated out of the 304 passband.

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

Detected by cheung, Submitted at 2013-09-17T00:00:12

2013-09-14T00:10:03 --> 2013-09-14T05:20:03

Quiescent filament eruption from the southeast limb.

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

Detected by halocme, Submitted at 2013-09-15T00:15:17

2013-09-13T23:30:35 --> 2013-09-14T05:30:35

Although very diffuse, some large-scale loops show outward motions, following the eruption (to southeast) of a small prominence in absorption (01:00-01:50 UT). An unimpressive CME is first observed by LASCO around 2 UT.

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

Detected by halocme, Submitted at 2013-09-14T23:35:12

2013-09-11T18:50:23 --> 2013-09-11T20:00:23

A minor jet and associated eruption may be associated with flux emergence that is marginally captured here.

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

Detected by halocme, Submitted at 2013-09-14T23:06:04

2013-09-11T02:30:35 --> 2013-09-11T03:30:35

The eruption involves motions that look like counter-clockwise. Loops to the north are affected by the eruption, leaving temporary dimming notably in 193 A images. No CME is observed by LASCO.

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

Detected by halocme, Submitted at 2013-09-14T22:57:03

2013-09-11T00:00:03 --> 2013-09-11T01:20:03

Looking at part of the areas in the movie, it is possible to be struck as jets. But it appears that a lot of things are going on, such as rising and then horizontal motions of loops in the western part, eruption of a low-lying prominence, opening up of higher structures in the eastern part, etc. No associated CMEs in LASCO data.

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

Detected by halocme, Submitted at 2013-09-14T22:38:03

2013-09-12T21:30:35 --> 2013-09-12T22:30:35

Footpoint brightening suggests that this jet originated on the visible side.

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

Detected by halocme, Submitted at 2013-09-14T21:56:36

2013-09-12T17:30:35 --> 2013-09-12T21:00:35

Although the eruption itself is not clearly captured, there is one because of a two-ribbon brightening. Loops extending over the limb show slight lateral motions, probably signifying that higher structures erupted and observed as a minor CME.

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

Detected by halocme, Submitted at 2013-09-14T21:43:56

2013-09-12T10:50:23 --> 2013-09-12T14:00:23

A minor eruption likely from backside. Its CME association is marginal.

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

Detected by halocme, Submitted at 2013-09-14T18:53:15

2013-09-13T01:00:04 --> 2013-09-13T01:45:40

Another flaring in AR 11839. The background-subtracted peak flux is something like A3. The creation of hot plasma is also seen in the western region (not numbered).

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

Detected by halocme, Submitted at 2013-09-14T18:42:23

2013-09-12T22:50:24 --> 2013-09-12T23:31:12

The peak GOES 1-8 A flux is B1.8, but it is less than B1.0 if background is subtracted. It is interesting to note that the first brightening is seen in AR 11839 (middle), followed by others in the eastern and western regions (without AR numbers).

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

Detected by halocme, Submitted at 2013-09-14T18:15:07

2013-09-12T10:40:12 --> 2013-09-12T12:00:36

This is a major flare of the day. The peak GOES 1-8 A flux is at B2.6, increased from the A9 level. But it is not included in the GOES flare list. Hot plasma is seen to be created in a couple of locations in AR 11841.

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

Detected by halocme, Submitted at 2013-09-14T18:00:31

2013-09-12T02:45:00 --> 2013-09-12T03:25:48

This brightening (causing the GOES 1-8 A channel to increase from B1.2 to B2.0) is in association with turbulent motions in the loop system in the southern extension of AR 11839. The movie at least indicates the generation of 6 MK plasma.