LMSAL >> Sungate >> Heliophysics Events Knowledgebase

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

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Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by schryver, Submitted at 2010-06-22T15:52:12
2010-06-21T16:13:28 --> 2010-06-21T22:42:50
Rapid coronal reconfiguration associated possibly with an eruption: interaction of a compact active region with an adjacent long-lived QS filament results in a series of coronal changes.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by juanms, Submitted at 2015-08-14T21:52:40
2015-08-10T05:10:06 --> 2015-08-10T15:30:06
Within the active region there are a few spots with recurrent jets continously for several hours with different intensities and sizes.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by schryver, Submitted at 2011-03-30T22:12:59
2011-02-10T00:00:04 --> 2011-02-15T06:00:04
Active region emergence from start to past X2.2 flare (4.25d interval).

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by asainz, Submitted at 2010-12-11T07:29:28
2010-12-08T01:45:01 --> 2010-12-09T23:57:50
Two ARs showing nice coronal loops. HMI magnetogram is overlaid in green/red.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-12-26T08:16:32
2019-12-23T12:00:09 --> 2019-12-25T16:00:09
This is AR 12754.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2019-12-26T08:08:16
2019-12-22T18:00:09 --> 2019-12-25T16:00:09
This is AR 12753.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by gchintzo, Submitted at 2019-11-07T00:51:59
2019-11-02T00:00:09 --> 2019-11-04T19:00:09
This AR exhibits an inverse polarity orientation (as compared to the hemispheric rule). This fact, combined with the high latitude of this AR suggests that Cycle 25 has just started

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by gchintzo, Submitted at 2019-03-11T21:32:12
2019-03-05T08:10:09 --> 2019-03-06T18:00:09
A decaying AR (unnamed by NOAA) in the south hemisphere of the sun. No significant activity (flares or CMEs) was produced by this region.

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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 2019-01-24T19:15:47
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 2019-01-24T17:32:47
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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Detected by halocme, Submitted at 2018-11-27T06:35:31
2018-11-17T12:00:09 --> 2018-11-19T12:00:09
Emerged around N26, this region had solar cycle 25 polarity. But it failed to become a NOAA active region because the marginal dark areas appeared in continuum images only for limited times and not continuous.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by gchintzo, Submitted at 2018-08-21T23:18:29
2018-08-18T17:40:09 --> 2018-08-19T10:20:09
Eruption from the decaying active region NOAA AR12718. It most likely was a failed eruption since no indication of a CME was seen in LASCO images.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by gchintzo, Submitted at 2018-08-07T22:27:06
2018-08-02T00:00:09 --> 2018-08-05T00:00:09
NOAA AR12717 transiting the solar disk. No sunspots are visible in this Active Region due to the incoherence of its magnetic flux concentrations (green positive, red negative)

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by tiwari, Submitted at 2018-07-20T21:17:35
2018-07-19T06:50:09 --> 2018-07-20T18:00:09
Evolving active region loops on limb.

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Detected by tiwari, Submitted at 2018-07-18T18:14:05
2018-07-16T05:20:09 --> 2018-07-18T10:30:09
A slowly evolving quiet active region with numerous hot loops.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by tiwari, Submitted at 2018-07-16T17:57:55
2018-07-13T00:30:09 --> 2018-07-14T17:40:09
A nice young evolving active region with bright coronal loops.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by tiwari, Submitted at 2018-07-09T20:13:21
2018-07-06T20:10:09 --> 2018-07-08T23:50:09
Dynamic AR loops on the East limb; several small bursts can be noticed.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by gchintzo, Submitted at 2018-06-20T17:57:23
2018-06-18T00:00:09 --> 2018-06-19T14:10:09
NOAA AR12713 as it transits the central part of the solar disk. This AR has emerged since it was in the back side of the sun and the decay process has already started, as it can be seen by the dispersed magnetic flux at the surface (red and green patches show negative and positive magnetic flux respectively).

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by jinmeng, Submitted at 2018-06-01T00:51:54
2018-05-22T13:10:09 --> 2018-05-24T21:30:09
Flux emergence and forming of AR 12711. During the process, there is another smaller-scale flux emergence region to the NE of the major one. The two flux emerging regions developed connections during the evolution. But due to flux cancellation, the smaller flux emerging region disappearred later.

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