Recent Events Reported by Observers

Detected by Wei Liu, Submitted at 2017-04-03T22:57:42

2017-03-16T02:13:07 --> 2017-03-16T03:43:53

A loop-shaped prominence with shallow angles from the south-east limb, exhibiting dynamic flows along the "loop".

Detected by Wei Liu, Submitted at 2017-04-03T22:51:02

2017-03-15T05:15:35 --> 2017-03-15T12:33:11

An prominence at the southwest limb exhibits interesting morphology, possibly a line-of-sight effect of two loop-shaped prominence crossing each other. Here the boundary between the two phenomena: prominence and coronal rain is very vague. Note an interesting episode of activity with material being thrown upward and falling back down, from about 9:30 to 11:00 UT.

Detected by gchintzo, Submitted at 2017-04-03T21:52:54

2017-04-02T19:00:09 --> 2017-04-03T00:00:09

A sixth eruptive flare (M6) in AR12644

Detected by gchintzo, Submitted at 2017-04-03T21:43:56

2017-04-02T16:10:09 --> 2017-04-02T19:50:09

A fifth eruptive flare (M1) in AR12644.

Detected by gchintzo, Submitted at 2017-04-03T21:39:24

2017-04-02T11:10:09 --> 2017-04-02T15:10:09

A fourth eruptive flare (M1.5) in AR12644.

Detected by gchintzo, Submitted at 2017-04-03T21:27:37

2017-04-01T23:00:09 --> 2017-04-02T09:00:09

A third eruptive flare (M5.4) in AR12644.

Detected by gchintzo, Submitted at 2017-04-03T21:21:54

2017-04-01T20:20:09 --> 2017-04-02T00:00:09

A second eruptive flare (M4.4). In this event, the CME 'bubble' is rather evident in the low corona.

Detected by gchintzo, Submitted at 2017-04-03T21:17:50

2017-04-01T18:20:09 --> 2017-04-01T20:40:09

Eruptive flare C3.7 in AR12644.

Detected by gchintzo, Submitted at 2017-04-03T20:27:41

2017-04-01T16:20:09 --> 2017-04-02T13:30:09

A small parasitic bipole emerges by the following polarity of the large bipolar AR in the south hemisphere of the sun. This sparks some jet-like activity but the most striking feature is two occurences of Coronal Waves emanating from the following polarity (possibly due to the interaction of the two bipoles). The coronal waves seem to bounce off the south coronal hole.

Detected by gchintzo, Submitted at 2017-04-03T20:07:00

2017-03-31T00:00:09 --> 2017-03-31T20:10:09

A large (extending to lower latitudes) coronal hole at the south pole of the sun.

Detected by gchintzo, Submitted at 2017-04-03T20:04:22

2017-03-31T09:25:09 --> 2017-03-31T22:20:09

A large (bipolar) emerging flux region with some subflaring activity (possibly a confined flare towards the end).

Detected by halocme, Submitted at 2017-03-30T22:00:58

2017-03-30T10:30:01 --> 2017-03-30T12:30:01

A jet was launched first closer to the limb, followed by what looks like a dual mini-filament eruption that was more non-radial in the beginning.

Detected by halocme, Submitted at 2017-03-30T22:00:58

2017-03-30T10:30:01 --> 2017-03-30T12:30:01

A jet was launched first closer to the limb, followed by what looks like a dual mini-filament eruption that was more non-radial in the beginning.

Detected by halocme, Submitted at 2017-03-30T21:00:51

2017-03-29T02:30:01 --> 2017-03-29T07:30:01

This occurred in a quiescent region east of AR 12644. The trigger is not identified, but the disturbances ran from southeast to northwest. No clear ecvience that something erupted.

Detected by halocme, Submitted at 2017-03-30T20:30:37

2017-03-28T04:30:01 --> 2017-03-28T06:00:01

Another C-class flare in AR 12645. An eruption coincided with the impulsive phase, but it was probably less powerful than the previous ones in the same region. There was no associated CME.

Detected by halocme, Submitted at 2017-03-30T20:30:37

2017-03-28T04:30:01 --> 2017-03-28T06:00:01

Another C-class flare in AR 12645. An eruption coincided with the impulsive phase, but it was probably less powerful than the previous ones in the same region. There was no associated CME.

Detected by halocme, Submitted at 2017-03-30T20:01:38

2017-03-28T09:00:09 --> 2017-03-28T18:00:09

The prominence eruption was captured first in 304 A images, in which it was hard to trace it to higher altitudes. The eruption at later times was seen better in 171 A images. No obvious CME associated.

Detected by halocme, Submitted at 2017-03-30T17:40:41

2017-03-24T00:00:09 --> 2017-03-30T13:00:09

On 30 March 2017 we see two sunspot active regions, AR 12644 (north) and 12645 (south). AR 12644 already showed bright coronal structures close to the east limb on 24 March. It had the largest growth on 26 March in terms of the region size and transient activity (one C-class and many B-class flares). The emergence of AR 12645 was seen during the second half of 26 March. Its most active period was 27 March. As soon as both of the leading and trailing spots got established, both ARs became less active. They may not produce major events unless they are triggered from outside the ARs.

Detected by halocme, Submitted at 2017-03-30T07:38:40

2017-03-27T16:30:01 --> 2017-03-27T19:30:01

There were three eruptions between 17:00 UT and 18:30 UT. First, large-scale motions seemed to precede the footpoint brightening of the C1.6 flare that peaked at 17:12. Then more violent eruption was seen associated with a B4.1 flare peaking at 17:43 (here it seems that flare=post-eruption arcade) slightly closer to the limb. Finally the footpoint brightening of theC5.1 flare that peaked at 18:20 seemed to precede an eruption, which appeared not as significant as the first two. The SEEDS catalog does not contain LASCO images around these events, but a CME is seen in https://cdaw.gsfc.nasa.gov/movie/make_javamovie.php?img1=lasc2rdf&img2=goesx&stime=20170327_1800&etime=20170327_2359.

Detected by halocme, Submitted at 2017-03-30T07:38:40

2017-03-27T16:30:01 --> 2017-03-27T19:30:01

There were three eruptions between 17:00 UT and 18:30 UT. First, large-scale motions seemed to precede the footpoint brightening of the C1.6 flare that peaked at 17:12. Then more violent eruption was seen associated with a B4.1 flare peaking at 17:43 (here it seems that flare=post-eruption arcade) slightly closer to the limb. Finally the footpoint brightening of theC5.1 flare that peaked at 18:20 seemed to precede an eruption, which appeared not as significant as the first two. The SEEDS catalog does not contain LASCO images around these events, but a CME is seen in https://cdaw.gsfc.nasa.gov/movie/make_javamovie.php?img1=lasc2rdf&img2=goesx&stime=20170327_1800&etime=20170327_2359.