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 2018-01-05T17:52:54

2018-01-02T22:20:25 --> 2018-01-03T02:20:25

This event looks like a confined eruption in 304 A images alone, but a flux-rope-like structure may be traced to the edge of the AIA field of view, deflected to southwest.

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

Detected by halocme, Submitted at 2018-01-05T17:41:47

2018-01-02T08:15:01 --> 2018-01-02T12:45:01

It appears that an outflow of cool material leads to slow reconfiguration of overlying coronal field as traced in 171 A images (but not 211 A). There was no indication that this structure later erupted.

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

Detected by halocme, Submitted at 2018-01-05T17:20:58

2018-01-01T21:40:13 --> 2018-01-01T23:40:13

This was likely from a region slighly occulted. Cool material fell back but material with coronal temperature seemed to be ejected, producing weak dimming.

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

Detected by halocme, Submitted at 2018-01-05T17:13:34

2018-01-01T16:00:09 --> 2018-01-01T17:50:33

Eruption of cool material seen against hot coronal background. It was likely from backside. The corona at high altitudes slightly dimmed. This eruption may give a false impreession of being stuck. This was due to missing frames in PRGB (all science data are unaffected).

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

Detected by halocme, Submitted at 2017-12-31T22:46:41

2017-12-31T14:30:01 --> 2017-12-31T15:15:37

Miniature sigmoid eruption.

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

Detected by halocme, Submitted at 2017-12-31T22:42:40

2017-12-30T19:20:25 --> 2017-12-30T20:20:25

The eruption was largely horizontal. In difference images, it looks like a jet.

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

Detected by halocme, Submitted at 2017-12-31T22:37:12

2017-12-29T11:30:01 --> 2017-12-29T13:10:01

An eruption, initially looking like a flux rope. This probably became an unimpressive CME (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171229.132545.w025.v0226.p302&frame=10&r)

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

Detected by halocme, Submitted at 2017-12-31T22:28:31

2017-12-28T22:20:25 --> 2017-12-28T23:09:37

The B8.3 flare was an isolated event. The wave propagted along the limb. The associated CME was not impressive (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171228.223607.w029.v0440.p103&frame=10&r).

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

Detected by halocme, Submitted at 2017-12-31T22:23:04

2017-12-27T22:45:01 --> 2017-12-27T23:35:25

A mini filament eruption led first to a jet and then to a more extended but still narrow eruption, to be observed by LASCO (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171228.002407.w011.v0193.p266&frame=3&r).

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

Detected by halocme, Submitted at 2017-12-31T22:16:21

2017-12-27T06:45:01 --> 2017-12-27T07:45:01

A small eruption and post-eruption arcade in a quiescent region.

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

Detected by halocme, Submitted at 2017-12-31T22:12:00

2017-12-27T04:40:13 --> 2017-12-27T05:21:01

Cool material was seen to be ejected horizontally as the jet started. The jet was then deflected to west by adjacent coronal structures. There was contemporaneous smaller jet activity east of this jet.

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

Detected by halocme, Submitted at 2017-12-31T22:06:09

2017-12-26T01:00:09 --> 2017-12-26T01:30:09

It appears that helical motions were involved in the initial stage.

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

Detected by halocme, Submitted at 2017-12-23T10:41:11

2017-12-21T19:30:01 --> 2017-12-21T20:40:49

The eruption occurred in a region that was bright in EUV images but was not given a NOAA AR number because there were no spots. The eruption seems to have hit AR 12692 to the east, also producing dimming regions.

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

Detected by halocme, Submitted at 2017-12-23T10:41:10

2017-12-21T19:30:01 --> 2017-12-21T20:40:49

The eruption occurred in a region that was bright in EUV images but was not given a NOAA AR number because there were no spots. The eruption seems to have hit AR 12692 to the east, also producing dimming regions.

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

Detected by halocme, Submitted at 2017-12-23T10:30:47

2017-12-21T19:00:09 --> 2017-12-21T22:30:09

A minor eruption with traces of helical motions.

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

Detected by halocme, Submitted at 2017-12-23T10:24:45

2017-12-21T04:30:01 --> 2017-12-21T10:00:01

Slow eruption followed by mass falling back. The associated CME may be http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171221.071207.w041.v0309.p273&frame=17&r.

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

Detected by halocme, Submitted at 2017-12-23T10:14:13

2017-12-20T01:20:25 --> 2017-12-20T09:00:25

This slow and diffuse eruption is best seen in 171 A images. A filament in 304 A images disappeared, and its relation to the off-limb motions in 171 A images is not clear.

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

Detected by halocme, Submitted at 2017-12-23T10:02:26

2017-12-17T05:00:09 --> 2017-12-17T12:00:09

Dimming slowly developed at high altitudes in 211 A, and possibly 193 A. This may be better captured by GOES16/SUVI. There was no clear indication of an eruption, and it was not clear how the prominence to the north would have participated in it. A possibly related CME is http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171217.091211.w033.v0152.p083&frame=25&r.

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

Detected by halocme, Submitted at 2017-12-23T09:48:05

2017-12-16T09:45:01 --> 2017-12-16T13:01:01

A coronal volume expanded, following temporary contraction in the inner part. This may signify filament activation, perhaps driven by footpoint motions not seen due to foreshortening. The expansion stopped, not leading to an eruption.

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

Detected by halocme, Submitted at 2017-12-23T01:49:16

2017-12-15T12:00:09 --> 2017-12-15T15:40:09

A filament eruption was seen southeast of a non-numbered region. It led to a striking twin dimming and spreading flare ribbons. The associated CME is http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20171215.170007.w070.v0226.p130&frame=15&r.