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 derosa, Submitted at 2012-10-12T22:33:17
2012-10-06T12:00:03 --> 2012-10-07T20:00:03
Liftoff of fairly long polar crown filament, followed by post-eruption ribbons and bright arcades

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Detected by schryver, Submitted at 2012-10-08T17:13:25
2012-10-05T18:40:03 --> 2012-10-06T03:40:03
Rolling motions in an activated polar-crown prominence.

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Detected by halocme, Submitted at 2012-10-08T04:40:32
2012-10-04T21:00:32 --> 2012-10-05T12:00:32
While it is difficult to locate the eruption, we can tell there was one because of the two-ribbon emission and hot (red from 94 A channel) loops between them. They grew slowly. The loops do not appear between the ribbons due to projection effect. A partial halo CME is reported to have been observed during this slow eruption.

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Detected by schryver, Submitted at 2012-10-04T22:49:43
2012-10-04T01:12:12 --> 2012-10-04T03:44:12
Eruption from behind the SE limb

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Detected by weiliu, Submitted at 2012-10-02T22:23:34
2012-10-02T05:40:03 --> 2012-10-02T08:20:03
A large scale surge from an active region near the west limb.

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Detected by weiliu, Submitted at 2012-10-02T22:19:36
2012-10-02T07:45:03 --> 2012-10-02T09:10:03
A surge erupted in an apparently "kinked" trajetory.

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Detected by weiliu, Submitted at 2012-10-02T21:38:19
2012-10-02T07:00:03 --> 2012-10-02T16:30:03
A filament erupts with clear signature of unwinding twist. It spins while rising upward, and some material is ejected toward the east and falls back to the Sun, while some material is pushed to the west and lands near the western limb.

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Detected by weiliu, Submitted at 2012-10-01T20:02:22
2012-09-30T01:55:03 --> 2012-09-30T09:40:03
A sigmoid-shaped surge erupts from an AR.

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Detected by halocme, Submitted at 2012-09-29T16:37:18
2012-09-26T12:00:03 --> 2012-09-26T14:00:03
This may be represent erupting loops but can also dignify waves. It is seen only at 211 A (and possibly at 193 A not included in this movie). It is irresitible to associate it with brightening in the region southwest of it.

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Detected by halocme, Submitted at 2012-09-29T15:55:29
2012-09-26T08:08:03 --> 2012-09-26T11:00:03
It is hard to single out an eruption or brightening, but isn't it possible that the filament eruption in the upper part of these images is driven by changes in the active region complex to south?

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Detected by halocme, Submitted at 2012-09-29T05:54:51
2012-09-24T14:40:11 --> 2012-09-24T22:00:11
Two regions seem to erupt around the same time. Each eruption is not major.

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Detected by halocme, Submitted at 2012-09-29T05:38:44
2012-09-24T15:10:11 --> 2012-09-24T16:40:11
Two loop systems brighten following minor flaring in a small region. No eruption is noted.

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Detected by halocme, Submitted at 2012-09-29T05:32:06
2012-09-24T14:00:04 --> 2012-09-24T15:00:04
This polar jet is seen only at 171, 193 and 211 A. Although the sensitivity is an issue, it appears that not much of high temperature plasma is produced even at the leg to be visible at 335 A or 94 A.

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Detected by halocme, Submitted at 2012-09-29T05:24:29
2012-09-24T09:30:35 --> 2012-09-24T10:16:35
A moving front is seen in a short distance, but this does not seem to be a fully-blown eruption. The front may signify a wave rather than the CME front loops.

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Detected by halocme, Submitted at 2012-09-29T05:06:48
2012-09-24T04:50:23 --> 2012-09-24T06:00:23
This may serve as an example of eruption that starts at relatively high altitudes without much flaring lower down - no flare above the background ~B5 level.

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Detected by halocme, Submitted at 2012-09-29T05:00:36
2012-09-24T02:10:11 --> 2012-09-24T03:10:11
The motion appears to be largely radial.

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Detected by halocme, Submitted at 2012-09-29T00:19:11
2012-09-23T14:00:07 --> 2012-09-24T00:00:07
The eruption itself seems to be not very spectacular (not associated with abig CME), but the post-flare loops are quite perstent. The source region seems to be just over the limb. This temporally follows the big eruption at E110, but their relation is not clear.

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Detected by halocme, Submitted at 2012-09-28T22:59:41
2012-09-23T20:30:35 --> 2012-09-23T21:30:35
This is a small eruption, but it affects the areas not only in the radial direction but also in lateral directions. For example, loops to the west, seen at 171 A in particular, seem to oscillate in association with the eruption, which should be understood in 3-d.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2012-09-28T22:27:33
2012-09-23T02:50:23 --> 2012-09-23T03:40:23
Better viewed in running difference images, a thin structure slightly brightens up for short time. This is probably a jet.

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Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2012-09-28T21:57:48
2012-09-23T03:00:03 --> 2012-09-23T05:00:03
Expanding loops seem to leave mild coronal dimming and ribbons of bright areas as in more energetic eruptions. There is an indication that these expanding loops also affect the larger-scale filament to southweat.

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