Highest Rated Events (only 193 and 304 shown) All AR FE FL
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-08-31T05:36:21
2012-08-23T04:30:35 --> 2012-08-23T06:30:35
The filament looked already fragmented prior to the eruption. The area underneath the filament brightened, especially around the two legs. By the time the erupted material reached the LASCO field of view, it was deflected to north. The CME was not impressive.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-08-31T05:09:43
2012-08-22T09:15:35 --> 2012-08-22T10:59:35
The off-limb outflow is seen at 211 A and 171 A. This eruption is associated with gradual increase in the GOES 1-8 A X-rays from B1.4 to B2.0. The CME carries a long-lasting internal structure.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-08-31T04:55:07
2012-08-22T00:00:03 --> 2012-08-22T03:00:03
This movie contains two minor eruptions, around 00:10 and 02:10 UT. Only the second one, which occurred slightly to the north of the first one, made it to a (narrow) CME observed by LASCO. The two B-class flares in the same interval do not seem to be in synch with the eruptions.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-08-30T15:41:32
2012-08-29T04:04:03 --> 2012-08-29T14:40:03
Filament activation.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-08-30T15:38:33
2012-08-29T00:00:03 --> 2012-08-29T12:40:03
A coronal reconfiguration adjacent to a near-equatorial small AR occurs synchronously with a filament activation (and subsequent draining/rain) in a distant QS filament.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-08-30T15:38:32
2012-08-29T00:00:03 --> 2012-08-29T12:40:03
A coronal reconfiguration adjacent to a near-equatorial small AR occurs synchronously with a filament activation (and subsequent draining/rain) in a distant QS filament.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-08-30T15:31:37
2012-08-28T00:48:03 --> 2012-08-28T08:20:03
Flux emergence next to (and trailing) a weak, decayed AR leads to the eruption of a small filament. The associated coronal front propagates at least to northward of the northern polar crown filament. Subsequently, a larger eruption occurs in the remains of the AR.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-08-30T15:31:36
2012-08-28T00:48:03 --> 2012-08-28T08:20:03
Flux emergence next to (and trailing) a weak, decayed AR leads to the eruption of a small filament. The associated coronal front propagates at least to northward of the northern polar crown filament. Subsequently, a larger eruption occurs in the remains of the AR.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-08-30T15:31:34
2012-08-28T00:48:03 --> 2012-08-28T08:20:03
Flux emergence next to (and trailing) a weak, decayed AR leads to the eruption of a small filament. The associated coronal front propagates at least to northward of the northern polar crown filament. Subsequently, a larger eruption occurs in the remains of the AR.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by weiliu, Submitted at 2012-08-28T22:20:21
2012-08-27T08:40:03 --> 2012-08-27T11:50:03
A loop-shaped prominence (304, red) erupted on the SW limb, exhibiting unwinding twists; this is immediately followed by another eruption nearby seen at 211 (pale blue).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by weiliu, Submitted at 2012-08-28T22:20:20
2012-08-27T08:40:03 --> 2012-08-27T11:50:03
A loop-shaped prominence (304, red) erupted on the SW limb, exhibiting unwinding twists; this is immediately followed by another eruption nearby seen at 211 (pale blue).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by weiliu, Submitted at 2012-08-28T20:37:19
2012-08-26T17:00:03 --> 2012-08-26T19:30:03
Recurrent surges from an AR on the east limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by weiliu, Submitted at 2012-08-28T20:14:46
2012-08-25T16:00:03 --> 2012-08-26T06:00:03
A large prominence eruption on the east limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by weiliu, Submitted at 2012-08-28T20:07:10
2012-08-25T00:00:03 --> 2012-08-25T13:00:03
A very long, transequatorial filament channel runs across about 3/4 of the solar disk from north-east to south-west.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2012-08-21T22:53:06
2012-08-15T22:35:03 --> 2012-08-16T02:30:03
A filament eruption, presumably from behind the limb, as no signature of the filament could be seen prior to the event.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2012-08-17T01:11:42
2012-08-15T10:00:04 --> 2012-08-15T15:00:04
The filament material that lifts off is rather translucent so but a close look at the movie shows that it's definitely happening.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2012-08-14T00:12:07
2012-08-12T18:15:04 --> 2012-08-13T04:30:04
A filament from behind the limb lifts off.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2012-08-14T00:00:58
2012-08-11T16:00:04 --> 2012-08-11T17:00:04
An eruption channels filamentary material into a magnetic funnel, which itself exhibits transverse oscillations triggered.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2012-08-13T23:36:06
2012-08-10T13:00:04 --> 2012-08-11T01:15:04
This filament gently lifts off from the northeastern limb. It appears that one footpoint of the filament is on the front side while the other is on the far side of the limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-08-10T17:54:49
2012-08-07T00:00:04 --> 2012-08-07T20:00:04
A series of at least seven explosions in a smallish AR, just inside the SE limb, send out perturbation fronts into the surroundings, causing high off-limb loops to oscillate, and with visible couplings to regions at least half a solar radius away.
