Highest Rated Events (only 193 and 304 shown) All AR FE FL
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5.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-05-14T22:22:50
2012-05-11T19:04:08 --> 2012-05-12T04:32:08
Coupled eruptions in two adjacent ARs (one strong, one quite small) with an apparent null point in between.
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Detected by anny, Submitted at 2012-05-10T03:37:31
2012-05-05T13:10:04 --> 2012-05-05T20:10:04
A large-scale filament erupts from the NE limb. Note that a minor flux rope in a nearby AR on the disk erupts, too - in the beginning of the large eruption.
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5.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2012-05-08T06:41:26
2012-05-02T04:05:04 --> 2012-05-02T15:10:04
An example of a disturbance which spans over the entire N half of the disk. A small slow eruption at the top left corner of the FOV is followed by a liftoff of a filament at the middle right. Its leftmost footpoint appears to get disconnected from the AR in the middle of the disk. Remnants of the filament (right middle) fall backwards, which is immediately followed by a flare and an eruption at the W imb (right edge of the FOV).
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Num Ratings:1
Detected by cheung, Submitted at 2012-04-24T01:22:08
2012-04-23T13:00:04 --> 2012-04-23T17:30:04
In this region of cross-equatorial reconnection, there seems to be an abundance of coronal condensation in locations that may act as favorable sites of reconnection between different domains of connectivity. Perhaps turbulent reconnection creates plasmoids which trap material and facilitate coronal condensation?
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5.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2012-04-24T01:22:08
2012-04-23T13:00:04 --> 2012-04-23T17:30:04
In this region of cross-equatorial reconnection, there seems to be an abundance of coronal condensation in locations that may act as favorable sites of reconnection between different domains of connectivity. Perhaps turbulent reconnection creates plasmoids which trap material and facilitate coronal condensation?
Rating:
5.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2012-04-24T01:07:32
2012-04-20T13:20:04 --> 2012-04-23T03:20:04
Some event from behind the limb seems to inject a large quantity of mass into the region that forms a quiescent filament. The filamentary material is clearly visible in 304 (red/orange). The morphology in the 171 channel (yellow) indicates a coronal cavity above the filament. This cavity+filament system is eventually destablized and launches off.
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5.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2012-04-24T01:07:31
2012-04-20T13:20:04 --> 2012-04-23T03:20:04
Some event from behind the limb seems to inject a large quantity of mass into the region that forms a quiescent filament. The filamentary material is clearly visible in 304 (red/orange). The morphology in the 171 channel (yellow) indicates a coronal cavity above the filament. This cavity+filament system is eventually destablized and launches off.
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5.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2012-04-20T21:18:02
2012-04-19T10:40:04 --> 2012-04-19T18:40:04
After one goes off, the other is destabilized and also lifts off.
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Num Ratings:1
Detected by cheung, Submitted at 2012-04-20T21:07:41
2012-04-16T21:20:04 --> 2012-04-17T08:50:04
More like a gentle lifting off than an eruption.
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Num Ratings:1
Detected by schryver, Submitted at 2012-04-17T20:05:15
2012-04-17T05:12:04 --> 2012-04-17T13:28:04
An eruption from an AR near the NE limb (at least the 3rd from this AR), showing a clear signature of a cusp-like structure, with oscillations along one side of the structure.
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Num Ratings:1
Detected by schryver, Submitted at 2012-04-17T20:05:13
2012-04-17T05:12:04 --> 2012-04-17T13:28:04
An eruption from an AR near the NE limb (at least the 3rd from this AR), showing a clear signature of a cusp-like structure, with oscillations along one side of the structure.
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Num Ratings:1
Detected by schryver, Submitted at 2012-04-17T19:56:44
2012-04-16T06:52:04 --> 2012-04-16T18:32:04
QS filament eruption, with a post-eruption arcade forming underneath the location of the dark erupted filament.
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Num Ratings:1
Detected by schryver, Submitted at 2012-04-16T22:52:26
2012-04-16T17:18:28 --> 2012-04-16T19:00:04
Filament eruption from the E limb, with much of the material later falling back. South of the erupting filament, a wedge-like structure appears (reminiscent of the event on 2010/04/30 22:00UT seen on disk). Note also the 'sympathetic' brightenings in the region south of the erupting/flaring region.
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Num Ratings:1
Detected by cheung, Submitted at 2012-04-14T00:48:53
2012-04-05T11:00:04 --> 2012-04-05T19:40:04
This filament eruption occurs with hours of the filament eruption from behind the western limb.
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Num Ratings:1
Detected by cheung, Submitted at 2012-04-14T00:46:05
2012-04-05T08:10:04 --> 2012-04-05T20:20:04
The high latitude and absence of AR loops suggests this is a quiescent filament eruption.
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Num Ratings:1
Detected by cheung, Submitted at 2012-04-13T22:36:05
2012-04-09T15:30:04 --> 2012-04-09T19:50:04
Seems to be some overexpansion in the transverse directions (i.e perpendicular to radial and plane of sky).
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Num Ratings:1
Detected by cheung, Submitted at 2012-04-13T22:25:54
2012-04-09T05:00:04 --> 2012-04-11T18:50:04
Loops from the AR (in the north) seem to be sucked into the interacting region.
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Num Ratings:1
Detected by cheung, Submitted at 2012-04-13T22:20:16
2012-04-09T01:10:04 --> 2012-04-09T02:50:04
Filamentary material get slingshot into a magnetic arcade and triggers some MHD oscillations.
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5.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2012-04-13T22:20:16
2012-04-09T01:10:04 --> 2012-04-09T02:50:04
Filamentary material get slingshot into a magnetic arcade and triggers some MHD oscillations.
Rating:
5.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2012-04-13T22:08:45
2012-04-09T09:00:04 --> 2012-04-09T17:20:04
This filament eruption occurs shortly before the filament eruption from behind the east limb at a comparable latitude.