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 2018-03-03T01:52:01
2018-03-02T10:20:25 --> 2018-03-02T12:00:01
This one is eruptive, but the global impact may be smaller than the B6.8 flare around 00:30 UT.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-03T01:52:00
2018-03-02T10:20:25 --> 2018-03-02T12:00:01
This one is eruptive, but the global impact may be smaller than the B6.8 flare around 00:30 UT.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-03T01:47:59
2018-03-02T05:00:09 --> 2018-03-02T06:00:09
Looks quite dynamic, but no eruption or other related phenomena.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-03T01:44:51
2018-03-02T00:00:09 --> 2018-03-02T02:00:09
AR 12770 had been dormant until late 1 March 2018, when it started to produce four flares above B1. This one was the most eruptive with relatively long duration soft X-rays. It was accompanied by coronal dimming and global waves.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-03T01:44:50
2018-03-02T00:00:09 --> 2018-03-02T02:00:09
AR 12770 had been dormant until late 1 March 2018, when it started to produce four flares above B1. This one was the most eruptive with relatively long duration soft X-rays. It was accompanied by coronal dimming and global waves.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-03T01:44:48
2018-03-02T00:00:09 --> 2018-03-02T02:00:09
AR 12770 had been dormant until late 1 March 2018, when it started to produce four flares above B1. This one was the most eruptive with relatively long duration soft X-rays. It was accompanied by coronal dimming and global waves.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T03:06:33
2018-02-28T14:00:09 --> 2018-02-28T16:00:09
The eruption started in the western part of the active region, producing a long-duration B2.3 flare. It also accomanied twin coronal dimming (typical of a sigmoid eruption) and a large-scale coronal propagating front primarily to the south.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T03:06:31
2018-02-28T14:00:09 --> 2018-02-28T16:00:09
The eruption started in the western part of the active region, producing a long-duration B2.3 flare. It also accomanied twin coronal dimming (typical of a sigmoid eruption) and a large-scale coronal propagating front primarily to the south.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T03:06:30
2018-02-28T14:00:09 --> 2018-02-28T16:00:09
The eruption started in the western part of the active region, producing a long-duration B2.3 flare. It also accomanied twin coronal dimming (typical of a sigmoid eruption) and a large-scale coronal propagating front primarily to the south.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T03:06:28
2018-02-28T14:00:09 --> 2018-02-28T16:00:09
The eruption started in the western part of the active region, producing a long-duration B2.3 flare. It also accomanied twin coronal dimming (typical of a sigmoid eruption) and a large-scale coronal propagating front primarily to the south.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T02:56:49
2018-02-25T12:00:09 --> 2018-02-27T12:00:09
This AR got the NOAA number at 27 Feb 2018 00:00 UT. The maximum size was 30 msh on 27 Feb 2018 and the AR decayed immediately to 10 msh on 28 Feb onward. The most intense flare was B3.3 on 26 Feb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T02:44:26
2018-02-26T17:00:09 --> 2018-02-26T18:39:45
An eruption occurred in a spotless region adjacent to AR 12700. It looked like a confined eruption. It affected the western part of AR 12700, but not significantly.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T02:37:01
2018-02-25T14:00:09 --> 2018-02-25T19:00:09
A large scale structure is seen to open up from the northern leg that resides a prominence being activated. This opening is best seen in 171 A images.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T02:28:38
2018-02-24T18:45:01 --> 2018-02-24T20:00:37
A mild eruption or outflow started on the slightly backside with the associated footpoint brightening hardly visible. South of this eruption, the adjacent structure was seen to shrink.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T02:12:26
2018-02-24T00:00:09 --> 2018-02-24T01:00:09
The mini filament erupted with untwisting motions that horiozntally shifted the jet. This horizontal shift stopped when the filament reconnected with the last set of open field lines.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T02:00:18
2018-02-24T00:30:01 --> 2018-02-24T01:30:01
It is hard to idntify a filament before the eruption. It may have formed during the eruption. It looks like a fragmented structure that is reflected in post-eruption signatures.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T01:50:29
2018-02-23T05:40:13 --> 2018-02-23T06:25:49
There were at least three (unrelated) jets in this region and in this interval. The eastmost one involved the ejection of a cool material as seen in 304 A images, blurring the distinction from a mini filament eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T01:36:59
2018-02-22T22:30:01 --> 2018-02-22T23:36:01
This is so diffuse that we need difference images to offset background emisson.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T01:25:37
2018-02-22T11:15:01 --> 2018-02-22T12:29:25
This is a very diffuse event. The jet was non-radial, toward the adjacent darker (lower-density) region.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2018-03-02T01:17:29
2018-02-21T16:10:13 --> 2018-02-21T17:10:13
The filament itself was hard to identify, but its eruption resulted in a two-ribbon flare that decayed quickly. The eruption looked like a jet, but it was not as narrow or collimated.
