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 jinmeng, Submitted at 2016-12-17T00:32:31
2016-12-15T02:50:06 --> 2016-12-16T00:00:06
Possible sympathetic filament erutpions were observed with sepeartion about 8-10 hours.

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Detected by jinmeng, Submitted at 2016-12-17T00:21:33
2016-12-15T18:57:06 --> 2016-12-16T00:00:06
A filament went unstable and erupted at last. Most of the filament material seems fall back to the Sun and lead to brightenings. The large-scale field might be changed due to the eruption that leads to a fast shrink of a coronal hole east of the source region. Moreover, there are synchronous activities from an active region at the west limb.

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Detected by jinmeng, Submitted at 2016-12-17T00:05:27
2016-12-14T18:16:06 --> 2016-12-14T18:46:42
a coronal jet was observed in the northern coronal hole with mini-filament eruption. The brightening after eruption showed an S-shape.

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Detected by jinmeng, Submitted at 2016-12-16T23:51:34
2016-12-13T02:30:06 --> 2016-12-13T09:10:06
A filament eruption was observed in the southern hemisphere.

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Detected by jinmeng, Submitted at 2016-12-13T19:57:23
2016-12-11T10:00:06 --> 2016-12-12T05:30:06
An emerging flux region was observed within the on-disk coronal hole. After the emerging phase, the region showed multiple activities with enhanced EUV emission.

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Detected by jinmeng, Submitted at 2016-12-13T19:50:34
2016-12-10T15:20:06 --> 2016-12-10T21:50:06
An eruption at the west limb. The eruption disturbed coronal loops. The EUV emission reached maximum after the eruption onset.

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Detected by jinmeng, Submitted at 2016-12-13T19:42:55
2016-12-10T01:00:06 --> 2016-12-10T04:20:06
A coronal jet from an on-disk coronal hole. It is a mini-filament eruption.

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Detected by gchintzo, Submitted at 2016-12-08T19:54:38
2016-12-05T23:00:06 --> 2016-12-07T15:10:06
Filament Eruption on the North East limb of the sun. A nearby emerging flux region (shows up at the north of the filament) potentially played a role in destabilizing the long filament. This event is the source region of a slow CME (230 km/sec; http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161207.110007.w073.v0230.p067&frame=20&r)

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Detected by gchintzo, Submitted at 2016-12-07T19:30:38
2016-12-05T05:30:06 --> 2016-12-05T13:20:06
Large scale faint connectivity in 171 (light blue) is seen to slowly move radially outwards above the East limb of the sun. At least close to the limb around the equator, this connectivity shows emmision in 304 (red). This is possibly a back-sided large filament eruption. This activity is likely the source region of a very slow CME (122 km/sec) observed by LASCO (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161205.162406.w063.v0122.p108&frame=30&r)

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Detected by gchintzo, Submitted at 2016-12-07T19:09:21
2016-12-04T13:10:06 --> 2016-12-04T15:49:28
An Active Region filament erupts and breaks into dark radial "threads", possibly due to reconnection of the structure with the ambient field. Some of the filament material falls back down as coronal "rain". This is the source region of a jet-like (small angular size) CME observed by LASCO C2 (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161204.142406.w027.v0418.p298&frame=11&r)

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Detected by gchintzo, Submitted at 2016-12-07T19:06:06
2016-12-04T13:10:06 --> 2016-12-04T15:49:28
An Active Region filament erupts and breaks into radial "threads", possibly due to reconnection of the structure with the ambient field. This is the source region of a jet-like (small angular size) CME observed by LASCO C2 (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20161204.142406.w027.v0418.p298&frame=11&r)

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Detected by jinmeng, Submitted at 2016-12-06T00:39:15
2016-11-25T02:20:06 --> 2016-11-28T00:00:06
Flux emergence and formation of a small active region was observed.

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Detected by jinmeng, Submitted at 2016-12-05T21:48:20
2016-11-25T23:50:06 --> 2016-11-26T12:20:06
A Quiet-Sun filament eruption. The filament channel showed brightenings during the eruption.

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Detected by jinmeng, Submitted at 2016-12-05T21:36:08
2016-11-24T15:00:06 --> 2016-11-25T00:00:06
A filament near the West limb showed activities and eventually became a failed eruption. During the activation process, reconnection may occur which leaded to a "double ribbon" structure.

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Detected by halocme, Submitted at 2016-12-05T05:47:13
2016-12-03T21:15:34 --> 2016-12-03T22:25:34
This is a period in which more jets are seen than at other time.

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Detected by halocme, Submitted at 2016-12-05T05:42:46
2016-12-02T15:30:34 --> 2016-12-02T17:16:34
The ejection started in AR 12615 toward north. It went nearly horizontally, disturbing low-lying loops.

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Detected by halocme, Submitted at 2016-12-05T05:35:02
2016-12-01T18:45:34 --> 2016-12-01T20:25:34
This looks like a filament eruption with the three-part structure. However, its coronagraph presence is quite disappointing (http://cdaw.gsfc.nasa.gov/images/soho/lasco_ql/2016/12/01/20161201_204248_lasc2rdf_ql.png).

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Detected by halocme, Submitted at 2016-12-05T05:35:02
2016-12-01T18:45:34 --> 2016-12-01T20:25:34
This looks like a filament eruption with the three-part structure. However, its coronagraph presence is quite disappointing (http://cdaw.gsfc.nasa.gov/images/soho/lasco_ql/2016/12/01/20161201_204248_lasc2rdf_ql.png).

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2016-12-05T05:28:58
2016-12-01T08:40:10 --> 2016-12-01T09:40:10
This was seen in a quiescent region. There was a short-lived chromospheric brightening while the eruption was in progress. There is an indicaiton of a jet toward southwest.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2016-12-05T05:18:03
2016-12-01T06:00:06 --> 2016-12-01T07:50:06
A jet is seen on the limb, accompanying the ejection of cool material (seen in 304 A). This may have triggered another jet to the north.

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