LMSAL >> Sungate >> Heliophysics Events Knowledgebase

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

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by asainz, Submitted at 2011-08-01T22:41:13
2011-07-29T15:20:04 --> 2011-07-31T07:00:04
Some interesting flares in and between ARs. I found very interesting the jet-like flare at the end of the meovie from the left-handed AR to the right-handed one.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by schryver, Submitted at 2011-03-23T22:08:18
2011-03-14T19:20:11 --> 2011-03-14T21:20:11
Fast eruptive event, with the ejection propagating towards the SW in a direction apparently strongly inclined relative to the vertical.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by schryver, Submitted at 2011-02-15T22:50:40
2011-02-15T01:35:34 --> 2011-02-15T06:21:46
X2 flare, associated with surges and filament eruptions. The first eruption/surge moves towards a region northward of the AR, but then deflects towards the east. The second, larger event, has a synchronous counterpart in an AR in the NE towards the limb, with a large filament-like structure in two parts almost connecting these two region in an eruption towards the SE.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by juanms, Submitted at 2010-07-29T20:28:39
2010-07-28T03:17:22 --> 2010-07-28T05:17:00
Small flare with a jet in a small active region which finish with a another flare at the end of the jet life.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by cheung, Submitted at 2010-06-14T16:09:04
2010-06-12T00:08:10 --> 2010-06-12T01:58:22
An M-class (GOES) flare exhibits itself as an flare and EUV wave in AIA.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by Annotator, Submitted at 2010-05-06T22:40:36
2010-05-05T16:00:02 --> 2010-05-05T17:58:37
Nice M class flare with good loop oscillations and diffraction spikes showing flare kernel structure.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2021-03-25T23:47:33
2021-03-22T00:00:09 --> 2021-03-22T02:30:09
This flare developed slowly, and perhaps lacked strong non-thermal emission. But a post-eruption arcade formed, and was associated with a decent CME appearing in northwest (https://cdaw.gsfc.nasa.gov/movie/make_javamovie.php?img1=lasc2rdf&img2=goesx&stime=20210322_0000&etime=20210322_0700). The CME coming from southeast is a separate event.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-02-07T03:21:44
2019-01-30T05:40:14 --> 2019-01-30T06:59:26
The biggest flare from AR 12733. Like others in the series, the flare was not eruptive despite violent motions in the vicinity of the central flare area.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-02-07T03:17:02
2019-01-29T21:00:30 --> 2019-01-29T22:50:54
Violent motions were observed after the flare brightening, but not associated with a CME, a similar pattern to the previous C1.9 flare also from AR 12733.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-02-07T03:11:05
2019-01-29T09:50:26 --> 2019-01-29T11:00:02
Flare in AR 12733. Surge-like motions are noted, just after the flare brightening, but there was no indication that the ejected material reached the coronagraphic heights, such as ~2 Rs.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-02-06T22:52:21
2019-01-26T13:00:02 --> 2019-01-26T14:00:02
The largest X-ray flare since 2018 Feb 7. It was non-eruptive, even though signatures were seen that are often thought of as being related to eruptions, such as rising loops and high-temperature regions just above nthe bright flare loops. Flares in AR 12733 were generally non-eruptive.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-01-05T22:54:28
2019-01-04T10:50:26 --> 2019-01-04T12:50:26
This flare, in AR 12732, showed eruptive signatures such as outward motions and cusp-like post-flare loops. But the large-scale effects were limited. The active region was already tired.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-01-05T22:25:51
2019-01-03T16:20:25 --> 2019-01-03T18:40:25
The region was ~5 degrees behind the limb, which arrived in Earth view only as a plage region. The eruptive motion was largely toward north, hardly contributing to a CME.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2018-10-10T22:04:28
2018-10-02T04:35:25 --> 2018-10-02T05:21:01
The first B-class flare in three weeks, which occurred in the western periphery of AR 12723. It was ejective, producing a weak coronal wave.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2018-03-03T01:52:03
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.

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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.

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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.

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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.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2018-02-07T03:53:06
2018-02-05T18:10:13 --> 2018-02-05T18:59:25
This flare occurred in AR 12699 as it developed. Multiple small-scale eruptions were seen, suggesting multiple footpoints and complex topology. Overall, this flare was not eruptive (no CME).

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2018-02-07T02:58:05
2018-01-30T17:15:01 --> 2018-01-30T18:00:37
This flare in AR 12697 looks like a confined eruption.

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