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 schryver, Submitted at 2011-06-08T14:47:07
2011-06-05T18:31:56 --> 2011-06-05T23:03:56
A filament activation (extending from AR to far-away QS, not showing chromospheric extinction) is followed by what appears to be a confined eruption and reconfiguration of the ARs magnetic field.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by schryver, Submitted at 2011-06-08T14:47:05
2011-06-05T18:31:56 --> 2011-06-05T23:03:56
A filament activation (extending from AR to far-away QS, not showing chromospheric extinction) is followed by what appears to be a confined eruption and reconfiguration of the ARs magnetic field.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by schryver, Submitted at 2011-06-08T14:43:43
2011-06-05T05:39:56 --> 2011-06-05T18:15:56
Two subsequent filament activations (likely constrained eruptions) with subsequent thermal evolution of the north-westers extremes of the AR.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by schryver, Submitted at 2011-06-08T14:40:50
2011-06-04T23:59:56 --> 2011-06-05T18:15:56
A prominence and an adjacent over-the-limb loop system interact (perhaps reconnect), followed by 1-2MK coronal evolutions.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by schryver, Submitted at 2011-06-08T14:30:36
2011-06-05T01:55:56 --> 2011-06-05T12:35:56
QS filament, north of smallish AR, erupts, followed by the evolution of post-eruption loop systems.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by cheung, Submitted at 2011-06-06T16:08:53
2011-06-04T22:19:56 --> 2011-06-04T22:42:26
This eruption from behind the limb is likely associated with the limb-only coronal wave occuring at around the same time.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by cheung, Submitted at 2011-06-06T16:03:39
2011-06-04T21:09:56 --> 2011-06-04T23:59:56
Off limb coronal loops are momentarily disturbed by what appears to be a coronal wave propropagating through the back side of the Sun. At the time the wave is observed, an eruption is also seen at a position angle of 280 deg.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-06T05:36:34
2011-06-05T01:59:56 --> 2011-06-05T07:59:56
This eruption may account for a slow proton event. There is no trace of this event in GOES X-ray light curves.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-05T05:21:16
2011-06-04T19:59:56 --> 2011-06-04T23:29:56
This must be a big CME that occurred on the backside. The corona in the northwestern quadrant is seen disturbed and the ejecta to the west (seen in 304 A) may be part of the CME. I cannot include this event under the CME category because I do not know its parameters (obtained in whitelight data).

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T08:29:17
2011-06-02T06:09:58 --> 2011-06-02T09:09:58
Like the previous events since May 29, 2011, this one shows the wave reflected or broken on its contact with northern regions and also fast recurrent pulses.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T08:16:30
2011-06-02T05:30:31 --> 2011-06-02T06:57:31
The 3d trajectory may be studied when STEREO data become available.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T08:03:25
2011-06-02T01:59:57 --> 2011-06-02T03:29:57
A confined flare in the eruptive region AR 11226.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T07:44:38
2011-05-31T21:20:06 --> 2011-05-31T22:00:18
Seems to be an isolated event.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T07:40:39
2011-05-31T21:20:02 --> 2011-05-31T22:00:14
A jet in a quiescent region

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T07:32:56
2011-05-31T14:00:02 --> 2011-05-31T16:48:02
Probably a confined ejection. Note a subsequent beightening in the region to southwest.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T06:55:26
2011-05-31T12:00:02 --> 2011-05-31T13:56:26
Although a filament eruption is not clearly seen, this eruption results in brightening in wide areas.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T02:14:22
2011-05-30T18:59:56 --> 2011-05-30T20:59:56
As expected, a narrow CME is seen shortly after.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T02:03:44
2011-05-30T09:59:56 --> 2011-05-30T12:29:56
Another example of the multiple fronts seen in a snapshot, typically at 171 A. Later frames show reflection of the wave at a northern region,

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T01:54:23
2011-05-30T08:00:02 --> 2011-05-30T12:30:02
The filament on this side of the limb seems to be intact.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-06-04T01:38:10
2011-05-30T04:29:57 --> 2011-05-30T06:59:21
It seems that the large-scale structures moves up first, followed by a compact flare at AR 11226, from which material is ejected to overlying loops --> modest CME

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