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

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

Detected by schryver, Submitted at 2013-05-07T21:42:48

2013-04-30T12:40:03 --> 2013-04-30T23:44:03

A quiet-sun filament activates around 2pm. About 7h later, the corona in that region shows all the signatures of an eruption, but no filament material is seen to be ejected.

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

Detected by schryver, Submitted at 2013-05-07T21:42:43

2013-04-30T12:40:03 --> 2013-04-30T23:44:03

A quiet-sun filament activates around 2pm. About 7h later, the corona in that region shows all the signatures of an eruption, but no filament material is seen to be ejected.

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

Detected by schryver, Submitted at 2013-05-07T16:55:57

2013-04-29T01:52:03 --> 2013-04-29T09:32:03

AR filament eruption towards the SE limb into a SE direction.

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

Detected by schryver, Submitted at 2013-05-07T16:41:31

2013-04-29T19:04:03 --> 2013-04-29T22:28:03

A fast, fairly narrow eruption from a S AR moves out over the SW limb, with a NE propagating perturbation (mainly seen in a fan of cool loops), and a subsequent - potentially coupled - eruption see in high loops over the SW limb.

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

Detected by schryver, Submitted at 2013-05-07T16:41:30

2013-04-29T19:04:03 --> 2013-04-29T22:28:03

A fast, fairly narrow eruption from a S AR moves out over the SW limb, with a NE propagating perturbation (mainly seen in a fan of cool loops), and a subsequent - potentially coupled - eruption see in high loops over the SW limb.

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

Detected by schryver, Submitted at 2013-05-07T16:41:27

2013-04-29T19:04:03 --> 2013-04-29T22:28:03

A fast, fairly narrow eruption from a S AR moves out over the SW limb, with a NE propagating perturbation (mainly seen in a fan of cool loops), and a subsequent - potentially coupled - eruption see in high loops over the SW limb.

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

Detected by anny, Submitted at 2013-05-06T19:53:08

2013-04-28T20:51:03 --> 2013-04-28T23:21:03

This large spray surge is a part of a long sequnce of spray surges at this site. The previous surges in the sequence were, however, much smaller.

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

Detected by anny, Submitted at 2013-05-06T19:48:58

2013-04-28T13:15:03 --> 2013-04-28T19:54:03

A small prominence eruption on the S limb.

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

Detected by anny, Submitted at 2013-05-06T19:40:52

2013-04-27T08:36:03 --> 2013-04-27T14:27:03

A good example of coronal rain on the NE limb.

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

Detected by anny, Submitted at 2013-05-06T19:39:23

2013-04-27T03:39:03 --> 2013-04-27T05:27:03

A very slow lift off of a small isolated blob in 304A on the NW limb.

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

Detected by anny, Submitted at 2013-05-06T19:20:50

2013-04-26T20:03:03 --> 2013-04-27T01:27:03

A C5-class flare produces a beautiful brightening at the top of the two whort loop bundles in 304A on the W limb.

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

Detected by halocme, Submitted at 2013-05-04T17:29:11

2013-05-03T17:14:52 --> 2013-05-03T18:14:52

This flare may be an example in which actions occurring in large-scale or surrounding magnetic field structure triggered the impulsive phase. It appears that changes in the region near the northern leg of the main flare loops (as projected in 2d) weakened the overlying field. There is an indication of the so-called plasmoid ejection. A type II burst is reported. The associated CME shows signatures of a shock wave.

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

Detected by halocme, Submitted at 2013-05-03T19:08:12

2013-05-03T08:50:23 --> 2013-05-03T10:00:23

This is a diffuse event. Although 171 A images show changes only around the western leg, both 193 A and 211 A images also show an outgoing arc that appears to form a loop system. However, it is not clear that this part represents expanding loops or a wave. The front is diffuse, but it can be due to a low S/N.

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

Detected by halocme, Submitted at 2013-05-03T18:27:39

2013-05-03T09:30:00 --> 2013-05-03T11:00:00

These loops attract one's eye. Although 6-8 MK plasma seems to exist inside as seen at 94 A (red), it is not seen at the outer edge nor 195 A secondary signals (for 15-20 MK) in blue. Therefore flare-like reconnection may not be present in loop expansions like this.

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

Detected by halocme, Submitted at 2013-05-03T17:17:33

2013-05-03T04:30:35 --> 2013-05-03T05:30:35

This jet, also seen in 304 A, is similar to but weaker than the one around 2-May -2013 13:20 UT. As well-known, jet activity tends to repeat.

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

Detected by halocme, Submitted at 2013-05-03T07:13:01

2013-05-03T00:50:23 --> 2013-05-03T02:20:23

Several episodes of injections are seen over a one hour interval. The source region seems to be slightly behind the limb.

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

Detected by halocme, Submitted at 2013-05-03T07:06:26

2013-05-02T13:05:23 --> 2013-05-02T13:46:11

The jet is best seen in 211 A and 193 A. In 171 A, only the lower part is seen. In 304 A, the chromospheric material goes up then falls down.

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

Detected by halocme, Submitted at 2013-05-02T23:26:00

2013-05-02T13:20:23 --> 2013-05-02T14:20:23

The CME loop is first seen already above AR loops. It stays in the AIA FOV until 13:55 or so. Even tough we see flare ribbons at 304 A, it is hard ot locate the flare in GOES light curves (with a ~B6 background). A disk region in a coronal hole near central merodian brightened around the time of the eruption, but whether they are related is TBD.

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

Detected by halocme, Submitted at 2013-05-02T18:19:48

2013-05-02T04:57:35 --> 2013-05-02T05:20:23

The eruption is more readily seen over the limb than on disk (i.e., not like a typical "EIT wave"), temporally overlapping with a nice type II burst. From the GOES X-ray light curves alone, it is hard to imagine eruptive behaviors like this. At 171 A, there is an indication of the quasi-peoridic fast propagating waves as reported by Wei Liu, Alan Title et al. for the 1-Aug-2010 event. A narrow filament eruption or surge is involved. The corresponding CME is limited in angular extent as expected from this kind of eruption.

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

Detected by schryver, Submitted at 2013-05-02T17:33:02

2013-04-24T12:00:03 --> 2013-04-24T15:48:03

Eruption from mid-sized AR approaching the W limb, apparently connecting to transequatorial loops over the limb, and with a loop or front propagating off disk.