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

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

Detected by anny, Submitted at 2013-03-19T20:59:26

2013-03-16T13:45:03 --> 2013-03-16T14:25:03

A close-up of the initial phase of the previously annotated eruption. Note that the erupting structure "consists" of thin dark semi-circularly shaped strand and a bright fringe around it. The fringe has uneven "outer" edge, and this edge is the brightest part of the whole structure.

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

Detected by anny, Submitted at 2013-03-19T20:53:40

2013-03-16T11:58:03 --> 2013-03-16T19:14:03

A large-scale, beautiful filament eruption on the NW disk. Note that the ejected material bright in 304A floats around in the corona like a "cloud" for long time after the eruption. Note also beautiful post-eruption arcade. In the beginning phase the footpoints are bright enough to cause the diffraction pattern in 304A, however there is no GOES flare associated with this event. On the still image in this annotation, note several dark thin smoothly-shaped strands in the core of the erupting structure.

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

Detected by cheung, Submitted at 2013-03-15T18:13:15

2013-03-12T10:07:33 --> 2013-03-12T11:30:03

This filament looks like a result of flux cancellation between decayed active region. The ejection of material appears (in projection) to be predominantly northward.

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Detected by schryver, Submitted at 2013-03-12T00:01:06

2013-03-08T15:32:03 --> 2013-03-08T21:52:03

Eruption of what looks like a blowout through a pseudo-streamer base

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Detected by schryver, Submitted at 2013-03-11T23:48:14

2013-02-19T02:56:03 --> 2013-02-19T22:52:03

QS filament activation

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Detected by schryver, Submitted at 2013-03-11T23:39:05

2013-02-17T00:00:03 --> 2013-02-18T04:00:03

An emerging flux region flares repeatedly. Towards the end of the day, the surrounding corona shofts in temperature (towards 171A/blue), which could be indicative of separatrix formation.

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

Detected by schryver, Submitted at 2013-02-19T23:34:57

2013-02-02T00:00:03 --> 2013-02-03T00:00:03

Compact flux emergence into a pre-existing monopolar region leading to many small-scale, short-lived brightenings.

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Detected by cheung, Submitted at 2013-02-15T17:11:24

2013-02-13T05:50:03 --> 2013-02-13T11:30:03

The concave morphology of the quiescent filament roof-top suggests the existence of a magnetic flux rope above the filament.

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

Detected by cheung, Submitted at 2013-02-15T17:07:14

2013-02-12T20:20:03 --> 2013-02-13T06:50:03

The first eruption leads to the appearance of a post-eruption arcade. As the arcade loops start to fade, another filament from the region is launched. It is difficult to establish a direct causal connection between the first eruption and the destabilization of the second.

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

Detected by cheung, Submitted at 2013-02-13T00:33:34

2013-02-11T18:50:03 --> 2013-02-11T20:10:03

This filament eruiption injects material into an open flux region. While some material (as signal in the 304 channel) escapes the AIA field-of-view, the remainder seems to be temporarily suspended in the corona before a sunward descent and/or in-situ disappearance.

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

Detected by cheung, Submitted at 2013-02-13T00:33:31

2013-02-11T18:50:03 --> 2013-02-11T20:10:03

This filament eruiption injects material into an open flux region. While some material (as signal in the 304 channel) escapes the AIA field-of-view, the remainder seems to be temporarily suspended in the corona before a sunward descent and/or in-situ disappearance.

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

Detected by anny, Submitted at 2013-02-07T23:55:56

2013-02-06T00:00:03 --> 2013-02-06T01:12:03

This is a high-cadence view on the beginning on the major eruption annotated earlier.

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

Detected by anny, Submitted at 2013-02-07T23:25:08

2013-02-06T00:00:03 --> 2013-02-06T04:36:03

A C-class flare produced this enormous eruption on the N disk.

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

Detected by schryver, Submitted at 2013-01-29T00:31:32

2013-01-26T20:32:03 --> 2013-01-27T00:00:03

A region between four relatively small active regions reconfigures suddenly, with (at 22:48UT) a structure that briefly looks a lot like a classicale current sheet with V-shaped endings, but there a much los confusion in this rapidly evolving pattern.

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

Detected by schryver, Submitted at 2013-01-28T18:30:53

2013-01-25T14:04:03 --> 2013-01-25T21:24:03

A quiet-Sun filament erupts towards the NE limb, with a beautiful cusp over the retracting loops.

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

Detected by cheung, Submitted at 2013-01-23T18:28:28

2013-01-23T00:30:03 --> 2013-01-23T05:50:03

This filament started to launch just about 20-24 hours after a neighboring lifted off. With such a long time delay, could these two events still be sympathetic eruptions (i.e. causally connected).

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

Detected by cheung, Submitted at 2013-01-23T18:21:34

2013-01-22T00:10:03 --> 2013-01-22T07:20:03

After this filament has lifted off, a neighboring one closer to the southern polar cap also launches. Are these sympathetic eruptions?

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

Detected by schryver, Submitted at 2013-01-03T00:45:11

2012-12-24T00:00:03 --> 2012-12-24T09:08:03

Two filaments (apparently unconnected but evolving jointly) near the polar crown activate. The largest, trailing one appears to straighten up vertically and subsequently drain and vanish as an absorbing body. The leading one is faint at all times, never really connects to the trailing one, but appears to lean towards it as that one moves towards a vertical orientation.

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

Detected by schryver, Submitted at 2012-12-12T23:19:10

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

Within the 24h period of 2012/12/11, at least five activations are seen involving the leading end of a filament/prominence configuration in the NE. The leading segment of the filament brightens, and then reveals an EUV extension arching high above the trailing end of the configuration, which is clearly affected (with oscillatory components) by the repeated activation.

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

Detected by cheung, Submitted at 2012-12-10T21:31:04

2012-12-07T21:00:03 --> 2012-12-07T22:30:03

The connection between this third eruption (from either AR 11623 or AR 11625) with the preceding two seems more tenuous than the connection between the first and second events.