Recent Events Reported by Observers

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.

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.

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.

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.

Detected by anny, Submitted at 2013-05-06T19:05:57

2013-04-26T00:00:03 --> 2013-04-26T09:30:03

A "V"-shaped cusp in 171A slowly lifts off. It lies above and in between of two dark domes in 171A which are in turn conined between two large prominences.

Detected by anny, Submitted at 2013-05-06T19:01:39

2013-04-26T20:15:03 --> 2013-04-27T00:00:03

A rapid relatively large-scale eruption is visible iin 211A and 171A on the W limb. I do not see any 304A erupting structure, nor an erupting cavity,

Detected by anny, Submitted at 2013-05-06T18:58:25

2013-04-26T10:25:03 --> 2013-04-26T21:50:03

A VERY large filament, spanning to a good third of the disk, takes off, likely our direction.

Detected by halocme, Submitted at 2013-05-04T17:29:16

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.

Detected by halocme, Submitted at 2013-05-03T19:08:16

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.

Detected by halocme, Submitted at 2013-05-03T18:27:45

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.

Detected by halocme, Submitted at 2013-05-03T17:51:01

2013-05-03T06:20:23 --> 2013-05-03T07:20:23

This movie shows how the twisted core field gets ejected, perhaps in reference to numerical simulations. The CME front appears to form only when the ejection reaches a certain height.

Detected by halocme, Submitted at 2013-05-03T17:17:37

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.

Detected by halocme, Submitted at 2013-05-03T07:13:06

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.

Detected by halocme, Submitted at 2013-05-03T07:06:30

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.

Detected by halocme, Submitted at 2013-05-02T23:26:04

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.

Detected by halocme, Submitted at 2013-05-02T18:19:52

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.

Detected by schryver, Submitted at 2013-05-02T17:33:06

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.

Detected by schryver, Submitted at 2013-05-02T17:30:54

2013-04-24T02:48:03 --> 2013-04-24T14:00:03

Long-range connections appear between an emerging ER and a distant AR.

Detected by schryver, Submitted at 2013-05-02T17:26:18

2013-04-24T11:54:03 --> 2013-04-24T12:38:27

Coronal jet from ER

Detected by schryver, Submitted at 2013-05-02T17:19:34

2013-04-24T08:12:03 --> 2013-04-24T10:44:03

A QS filament, connecting to a very small bipolar region, activates and reconfigures with motions extending into two diametrically opposed directions.