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 schryver, Submitted at 2011-11-23T16:43:51
2011-11-22T14:40:04 --> 2011-11-23T00:00:04
Filament/prominence eruption and hot coronal rain over widely separated footpoints

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Detected by schryver, Submitted at 2011-11-23T16:41:51
2011-11-22T03:36:04 --> 2011-11-22T17:20:04
Field reconfiguration at apparent topological separator

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Detected by schryver, Submitted at 2011-11-23T01:54:51
2011-11-21T04:36:04 --> 2011-11-21T13:12:04
QS filament activation with signs of coronal channels in response to the coronal reconfiguration.

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Detected by schryver, Submitted at 2011-11-23T01:54:37
2011-11-21T04:36:04 --> 2011-11-21T13:12:04
QS filament activation with signs of coronal channels in response to the coronal reconfiguration.

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Detected by schryver, Submitted at 2011-11-23T01:51:36
2011-11-21T09:16:04 --> 2011-11-21T20:28:04
Quiet-Sun polar-crown filament activation with hot coronal rain in relatively distant quiet Sun.

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Detected by anny, Submitted at 2011-11-21T22:40:51
2011-11-19T21:43:04 --> 2011-11-20T00:00:04
A blob of plasma is thrown sidewards at large speed after a flare; it quickly rises up and falls down as coronal rain.

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Detected by anny, Submitted at 2011-11-18T21:44:29
2011-11-17T22:14:04 --> 2011-11-18T00:00:04
Open loops in 171A and a prominence in 304A wiggle being disturbed by the spectacular eruption nearby.

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Detected by anny, Submitted at 2011-11-18T21:22:06
2011-11-17T15:14:04 --> 2011-11-17T17:58:04
Flux rope erupts S-wards from an AR on the SE limb. It isn't clear whether the eruption is somplete or the entire flux rope sinks back in. A large loop could be seen in the last stage of the eruption on the tip of the rope, suggesting kink instability as a trigger.

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Detected by anny, Submitted at 2011-11-18T21:10:37
2011-11-17T11:58:04 --> 2011-11-17T19:04:04
Large filament takes off on the SW disk. Large-scale swirls are seen in its W-most footpoint. This eruption takes place nearly contemporary with a few other eruptive events on the disk. It seems to start at the ame time as a small eruption-like brightening above a tiny dipole on its W-most point.

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Detected by anny, Submitted at 2011-11-16T00:48:35
2011-11-14T20:00:04 --> 2011-11-15T15:24:04
This must be the slowest filament takeoff I have ever seen It isn't clear whether some of this massive structure takes off completely; some definitely falls down in all directions as coronal rain, while some very very slowly lifts off as coronal puff. Close to the lifting footpoint there is later some swirling which yet again slowly rises and takes off as puff or falls down as rain, is hard to tell.

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Detected by anny, Submitted at 2011-11-14T21:20:48
2011-11-13T07:50:04 --> 2011-11-13T09:22:04
Eruption in AR's 11343 and 11344. It brightens up a jet in each AR on the opposite sides of the ARs; this is followed by oscillations in the overlying 211A loops and a blob of plasma emitting in 304A rapidly thrown up and fallen back down.

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Detected by anny, Submitted at 2011-11-14T20:55:17
2011-11-13T00:00:04 --> 2011-11-14T00:00:04
Long filament which starts at the disk and goes over the limb suddenly develops activity in its limb portion. It starts to kink, then rise and swirl, and then it sinks down dragging in some overlying plasma - if to play the last part of the event backwards in time it might look like a slow eruption.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by schryver, Submitted at 2011-11-07T22:22:26
2011-11-04T13:35:04 --> 2011-11-04T22:10:04
Quiet-Sun filament activation

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Detected by anny, Submitted at 2011-11-07T20:16:47
2011-11-01T19:02:04 --> 2011-11-01T19:42:04
Bright blob is thrown upwards presumably after a flare; it sinks back down on the other end of the loop and its well-defined front edge is bright enough to cause diffraction pattern at all points along the trajectory.

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Detected by anny, Submitted at 2011-11-03T00:24:01
2011-10-31T20:44:04 --> 2011-11-01T00:00:04
Coronal rain in 304A forms a clear ring high up in the corona. This ring soon grows horns and tail - a very appropriate structure for Halloween

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by anny, Submitted at 2011-11-03T00:19:31
2011-10-31T13:00:04 --> 2011-11-01T00:00:04
Plama in thin long filament suddenly starts to flow down one of its footpoints along a swirled trajectory; immediately after the entir filament takes off clearly swirling in the same direction. A dark coronal dimming appears in 211A under where the filament was; this dimming slowly crawls SE. The structure of the chromosphere in 304A is clearly different in this dimming from the rest of the quiet disk.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by anny, Submitted at 2011-11-03T00:19:27
2011-10-31T13:00:04 --> 2011-11-01T00:00:04
Plama in thin long filament suddenly starts to flow down one of its footpoints along a swirled trajectory; immediately after the entir filament takes off clearly swirling in the same direction. A dark coronal dimming appears in 211A under where the filament was; this dimming slowly crawls SE. The structure of the chromosphere in 304A is clearly different in this dimming from the rest of the quiet disk.

Movie

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by anny, Submitted at 2011-10-11T21:12:40
2011-10-10T04:10:04 --> 2011-10-10T11:42:04
Plasma flows along the filament channel from one footpoint to the other in the plane of the sky and later seemingly snks in the other footopint along spectacular spiral trajectories seemingly along the line of sight.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by anny, Submitted at 2011-10-11T00:43:29
2011-10-09T13:08:04 --> 2011-10-09T14:08:04
A probably C-class flare - it is hard to tell as it is the 2nd in the sequence in this region. The first flare triggers matter emitting in 304A and 171A to flow along the loop with sharp front visible - but half way through there seems to be another flare - or at least there is a diffraction pattern, most eminent in 304A.

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Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by asainz, Submitted at 2011-10-11T00:00:10
2011-10-07T14:40:16 --> 2011-10-09T00:00:16
Faint CME ande then a small flare.

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