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 halocme, Submitted at 2011-09-27T05:59:10
2011-09-08T15:20:24 --> 2011-09-08T16:20:24
Agai, the northern part seems to be the eruption itself.

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Detected by halocme, Submitted at 2011-09-27T05:54:50
2011-09-07T22:20:24 --> 2011-09-07T23:20:24
Certainly part of these disturbances should be CME loops ahead of the erupting filament, about which a separate annotation is needed.

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Detected by halocme, Submitted at 2011-09-27T05:48:56
2011-09-06T22:00:05 --> 2011-09-06T23:14:29
The northern portion of the disturbances looks like CME loops, but other portions are.... probably a wave.

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Detected by halocme, Submitted at 2011-09-27T05:40:51
2011-09-04T04:30:00 --> 2011-09-04T05:31:12
The source region is ~18 degrees behind the limb.

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Detected by halocme, Submitted at 2011-09-27T01:52:14
2011-09-22T09:40:13 --> 2011-09-22T11:40:13
A big event near the east limb.

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Detected by halocme, Submitted at 2011-09-27T01:41:57
2011-09-23T21:50:24 --> 2011-09-23T22:31:12
Have we seen something like this before?

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Detected by halocme, Submitted at 2011-09-27T01:33:17
2011-09-23T12:00:04 --> 2011-09-23T13:00:04
The wave-like disturbances appear to follow the CME. Primarily northward.

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Detected by halocme, Submitted at 2011-09-27T01:16:53
2011-09-26T14:30:00 --> 2011-09-26T15:20:24
Compared with previous ones from the same region (AR 11302), this one is very weak.

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Detected by halocme, Submitted at 2011-09-27T00:52:31
2011-09-25T15:20:24 --> 2011-09-25T16:50:24
The wave-like disturbances are limited to a relatively small area to the south of the flare. The associated filament eruption is more spectacular, which should be annotated separately.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-09-27T00:44:05
2011-09-25T09:20:24 --> 2011-09-25T10:10:48
From AR 11303. In addition to the CME-driven wave, recurrent pulses are seen in the wake of the CME.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-09-27T00:09:20
2011-09-25T04:20:25 --> 2011-09-25T05:20:25
This is again from AR 11302, and its propagation is mostly southward.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-09-26T23:59:24
2011-09-25T01:45:00 --> 2011-09-25T03:25:48
This was associated with a M4.4 flare in AR 1303 (though the NOAA report shows AR 1302), like the previous two events. In comparison, this one seems to be more aligned with the CME loops.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-09-26T23:44:09
2011-09-24T23:20:24 --> 2011-09-25T00:40:48
Similar to the previous event associated with a M1.2 flare. The wave is minor, but the CME loops seem to be even more compact.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-09-26T23:36:48
2011-09-24T21:00:37 --> 2011-09-24T21:59:25
This is a minor event in AR 1303.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-09-26T22:35:47
2011-09-24T19:00:05 --> 2011-09-24T22:00:05
This one was primarily toward north, different from the previous two events from the same region. Interestingly, the large-scale disturbances were associated with the M3.0 flare starting 19:09, and the following M5.8 flare starting 20:29 at an area slightly to the east was quite confined.

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Detected by halocme, Submitted at 2011-09-26T22:19:55
2011-09-24T11:50:25 --> 2011-09-24T14:50:25
The signature is marginal in this version of 94 A movies, but this channel is included for future references. Compared with the previous one at 09:21 (with the X1.9 flare), the CME loops are clearly seen in this event. The X-ray time profiles are more gradual.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-09-26T22:09:07
2011-09-24T09:00:05 --> 2011-09-24T11:00:05
The wave signatures get less global at higher temperatures.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by anny, Submitted at 2011-09-22T19:23:09
2011-09-20T04:50:04 --> 2011-09-20T06:08:04
A spray surge following a flare in the active region that produced a lot of flares already. Note the conteporary coronal jet to the W of it and the contemporary surge on the W limb.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by anny, Submitted at 2011-09-22T02:34:49
2011-09-19T20:18:04 --> 2011-09-20T00:00:04
Large-scale structure in 171A and 304A bends and wiggles in responce to a nearby faint eruption.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by anny, Submitted at 2011-09-22T02:21:16
2011-09-19T10:28:04 --> 2011-09-19T17:04:04
A spray surge directed towards a null point is followed by appearance of bright 211A and 171A (latter not shown) loops overlying the null. Thin features emitting in 304A and seemingly optically thick in 211A later reappear above the null and sink down to the footpoints - if coronal rain could be observed at disk center, it could have looked exactly like that.

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