LMSAL >> Sungate >> Heliophysics Events Knowledgebase

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

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-02-07T03:06:20
2019-01-28T14:30:01 --> 2019-01-28T15:40:01
The outward motion of cool material, highly non-radial, propagated to high altitudes. It only resulted in a marginal jet. No type III bursts were associated.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-02-07T01:36:29
2019-01-27T15:50:25 --> 2019-01-27T16:50:25
This jet involves helical motions of cool material as seen in 304 A images. No type III radio burst is noted in Wind/WAVES data.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-02-06T23:07:01
2019-01-26T06:00:09 --> 2019-01-26T11:30:09
A diffuse eruption with cool prominence matrial underlying a flux-rope-like outward-moving feature seen only in 171 A images. No CME associated.

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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 gchintzo, Submitted at 2019-02-05T19:14:47
2019-02-04T00:00:09 --> 2019-02-05T15:00:09
A decaying active region of overall bipolar magnetic distribution. This AR is not catalogued by NOAA.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T21:56:16
2018-12-10T00:00:09 --> 2018-12-10T19:05:09
Part of a prominence structure is ejected and its plasma pulled back into the solar surface.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T19:48:07
2018-12-09T00:00:09 --> 2018-12-09T12:40:09
An eruption is seen to occur from the sigmoid-like active region as it passes through the white box marked in the video

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T19:28:59
2018-12-07T00:00:09 --> 2018-12-08T00:00:09
Large filament is seen erupting on the solar disk, expanding out of the marked white box (see video).

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T19:15:47
2018-12-04T00:00:09 --> 2018-12-05T00:00:09
Following the marked active region allows us to observe its development through the course of 24 hours, whose end is marked by a north-bound eruption.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T19:09:23
2018-12-03T21:10:09 --> 2018-12-04T00:00:09
Eruption seen from/near small active region off western limb.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T18:52:39
2018-12-02T00:00:09 --> 2018-12-02T03:05:09
What seems like a coronal jet (perhaps associated with a prominence?) is seen leaving the Sun from the NW limb.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T18:36:55
2018-11-30T00:00:09 --> 2018-11-30T09:05:09
Filament eruption seen in 304 ? passing through the white box identified in the northern hemisphere.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T18:29:49
2018-11-30T00:00:09 --> 2018-11-30T08:40:09
Large filament erupts from the south hemisphere. The region within the white box (see video) denotes the area where the eruption is clearest, and does not represent the extent of the entire filament. Closer analysis shows that the filament extended further westward on the disk, as did its eruption.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T18:07:45
2018-11-28T00:00:09 --> 2018-11-28T14:00:09
Long filament is seen dancing off the limb, and then breaking off from the solar surface. Note that a smaller filament just below it also erupted towards the end of this video.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T17:46:07
2018-11-25T00:00:09 --> 2018-11-25T03:55:09
A small eruption is visible, where filamentary material is seen falling back to the solar surface.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T17:39:16
2018-11-25T00:00:09 --> 2018-11-26T00:00:09
Beautiful large quiescent filament (or perhaps more than one filament) seen in the south-eastern hemisphere of the Sun.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T17:32:47
2018-11-24T00:00:09 --> 2018-11-24T03:55:09
'Activity' visible in this AR, possibly including filament re-organization/eruption (304 ? rdiff images).

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T17:29:10
2018-11-24T00:00:09 --> 2018-11-24T03:55:09
Filamentary material rises and either erupts or drains by towards the solar surface

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T17:21:15
2018-11-23T04:30:09 --> 2018-11-23T08:15:09
As an active region (visible in 171, 211) rotates out of the the field of view, a small eruption occurs, defined by a shock wave and the expulsion of some filamentary material.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by mkocher, Submitted at 2019-01-24T17:06:26
2018-11-22T00:00:09 --> 2018-11-23T00:00:09
Looks like a series of filaments are forming, evolving and perhaps interacting at the NE limb of the Sun through the course of the day.

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