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 2011-05-30T22:19:07
2011-05-28T09:30:02 --> 2011-05-28T17:00:02
Hard to see, and only in 304 A images, probably related to the narrow CME observed by LASCO (starting 17:46 UT at PA of ~340 deg).

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-05-30T05:27:44
2011-05-29T20:29:57 --> 2011-05-29T22:29:57
The propagation is primarily northward. In 94 A, the trajectory is not clearly seen, but only when the wave hit the northern region.

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Detected by halocme, Submitted at 2011-05-30T05:08:04
2011-05-27T12:50:00 --> 2011-05-27T13:00:12
This may be called a jet, but an interesting thing is that a tiny eruption is also seen to the west. The two phoneomena may be someow connected.

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Detected by halocme, Submitted at 2011-05-30T04:35:56
2011-05-27T21:40:29 --> 2011-05-27T23:59:41
Similar to the previous event between 07:40 and 10:40 UT except that this one appears dark in 171 A and 211 A.

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Detected by halocme, Submitted at 2011-05-30T04:25:50
2011-05-27T07:40:18 --> 2011-05-27T10:40:18
In 304 A, some of these jets appear to come back down.

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Detected by halocme, Submitted at 2011-05-30T04:17:50
2011-05-27T00:49:45 --> 2011-05-27T05:01:45
Likely to be a failed eruption -- no obv ious CME in LASCO.

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Detected by halocme, Submitted at 2011-05-30T04:09:44
2011-05-29T09:49:45 --> 2011-05-29T10:59:57
This is associated with a CME observed by LASCO, but I put it in the eruption category because I cannot enter the CME information now.

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Detected by halocme, Submitted at 2011-05-29T23:05:45
2011-05-26T18:00:02 --> 2011-05-26T19:59:26
Two regions are seen that produced jets. They are likely to propagate into LASCO FOV.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2011-05-29T16:56:18
2011-05-27T22:24:55 --> 2011-05-27T22:59:07
Around the time of the C1.2 flare in AR 11226 (on the limb), a few areas on disk also brightened, accompanying minor eruptions. How are they connected?

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by derosa, Submitted at 2011-05-28T01:19:52
2011-05-25T06:01:59 --> 2011-05-25T23:59:59
A coronal cavity associated iwth a polar crown filament.

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Detected by derosa, Submitted at 2011-05-28T01:15:33
2011-05-25T06:01:59 --> 2011-05-25T23:59:59
A loop fan plane, on the edge of a coronal hole, that shows continual upward streaming in all directions. Can this be a source of the solar wind (e.g., as in Sakao et al. 2007)?

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by derosa, Submitted at 2011-05-28T00:56:24
2011-05-25T00:01:59 --> 2011-05-25T19:59:59
A double eruption from AR11218.

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Detected by derosa, Submitted at 2011-05-27T18:05:15
2011-05-24T07:02:18 --> 2011-05-24T23:59:18
Eruption observed in both the 211 and 304 channels of AIA (the latter includes prominence material) on or behind the limb

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Detected by seguin, Submitted at 2011-05-26T21:49:55
2011-05-25T09:59:56 --> 2011-05-26T09:59:56
Flux is seen to upwell in the middle of a region of opposite polarity, followed shortly by a series of small eruptions and a slightly larger, but still compact eruption. The eruptions all look to be confined. Look at the magnetogram to view the flux emergence, although it is also apparent from the EUV channels.

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Detected by seguin, Submitted at 2011-05-26T21:49:48
2011-05-25T09:59:56 --> 2011-05-26T09:59:56
Flux is seen to upwell in the middle of a region of opposite polarity, followed shortly by a series of small eruptions and a slightly larger, but still compact eruption. The eruptions all look to be confined. Look at the magnetogram to view the flux emergence, although it is also apparent from the EUV channels.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by berger, Submitted at 2011-05-26T21:12:06
2011-05-24T00:02:18 --> 2011-05-25T11:02:18
Coronal cavity and associated quiescent prominence on SW limb. Prominence activates in response to nearby eruption and material is seen moving into cavity center.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by anny, Submitted at 2011-05-24T21:33:12
2011-05-20T00:45:53 --> 2011-05-20T21:05:53
A large filament on the SE disk makes swirling motions, slowly lifts off one end and produces coronal rain.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by anny, Submitted at 2011-05-24T21:25:35
2011-05-19T23:45:53 --> 2011-05-20T03:25:53
Large-scale coronal rain or possibly a small eruption.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by weiliu, Submitted at 2011-05-23T22:36:22
2011-05-23T00:00:12 --> 2011-05-23T06:45:12
Recurrent surges on the southwest limb, including one episode seen first at 304 and then at 211 along a loop.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by weiliu, Submitted at 2011-05-23T21:46:52
2011-05-23T00:00:12 --> 2011-05-23T06:45:12
A sigmoid-shaped filament erupts, unwraps itself (see the dark 304 features with twists), and leads to flaring (see the separating flare ribbons seen at 211).

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