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 cheung, Submitted at 2014-05-23T22:40:24
2014-05-10T22:50:03 --> 2014-05-11T01:30:03
This filament stops rising in the mid corona.

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Detected by cheung, Submitted at 2014-05-23T22:40:23
2014-05-12T06:27:03 --> 2014-05-12T07:17:03
The activation causes oscillations of loops in a neighboring filament channel.

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Detected by cheung, Submitted at 2014-05-23T22:40:22
2014-05-12T10:40:03 --> 2014-05-12T17:30:03
This region previously spawned two giant helical surges. This eruption seems to also have arcade loops.

Movie

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Detected by cheung, Submitted at 2014-05-23T22:40:21
2014-05-12T10:40:03 --> 2014-05-12T17:30:03
This region previously spawned two giant helical surges. This eruption seems to also have arcade loops.

Movie

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Detected by cheung, Submitted at 2014-05-23T22:40:20
2014-05-10T10:10:03 --> 2014-05-10T10:40:03
The apparent helical motion of the jet suggests the field lines are untwisting.

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Detected by cheung, Submitted at 2014-05-23T21:40:19
2014-05-09T23:10:03 --> 2014-05-10T05:10:03
The coronal loops seem to open up during this faint eruption.

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Detected by cheung, Submitted at 2014-05-23T21:40:18
2014-05-09T23:10:03 --> 2014-05-10T05:10:03
The coronal loops seem to open up during this faint eruption.

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Detected by halocme, Submitted at 2014-05-22T05:52:10
2014-05-21T00:45:35 --> 2014-05-21T03:09:35
In this eruption, the flux rope structure is seen at 304 A. The northern parts seems to reconnect with the surrounding corona, while the southern part expands radially. This eruption became the most decent CME during 19-21 May.

Movie

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Detected by halocme, Submitted at 2014-05-22T05:52:09
2014-05-21T00:45:35 --> 2014-05-21T03:09:35
In this eruption, the flux rope structure is seen at 304 A. The northern parts seems to reconnect with the surrounding corona, while the southern part expands radially. This eruption became the most decent CME during 19-21 May.

Movie

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2014-05-22T05:37:21
2014-05-21T11:30:35 --> 2014-05-21T14:00:35
A filament encompassing the whole active region seems to erupt first, inducing the spiraling jet from the northern part of the region. The filament itself is hardly visible.

Movie

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Detected by halocme, Submitted at 2014-05-22T05:37:20
2014-05-21T11:30:35 --> 2014-05-21T14:00:35
A filament encompassing the whole active region seems to erupt first, inducing the spiraling jet from the northern part of the region. The filament itself is hardly visible.

Movie

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2014-05-22T05:29:09
2014-05-21T10:00:03 --> 2014-05-21T11:30:03
This is more than a flow along long closed loops. Adjacent areas are affected including dimming.

Movie

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2014-05-22T05:22:11
2014-05-20T18:00:03 --> 2014-05-20T20:00:03
The northwest limb stands out for prominence activities. The material falling down in the southern leg pops up from nowhere. It is not clear whether these motions follow an eruption or belong to filament activation.

Movie

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2014-05-22T05:12:48
2014-05-20T11:50:23 --> 2014-05-20T17:00:23
A diffuse front is seen to move northward, followed by the formation of a two-ribbon brightening and post flare loops between the ribbons. However, it is difficult to determine how this eruption slowly developed. This eruption may be partially Earth-directed, given the appearance of the associated CME.

Movie

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2014-05-22T05:00:49
2014-05-20T03:50:23 --> 2014-05-20T06:00:23
This eruption has a characteristic right-hand screw pattern (from the bottom). Part of it is seen in emission in 171 A images. The complex structure is reflected in the later CME.

Movie

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2014-05-22T04:52:58
2014-05-19T20:10:11 --> 2014-05-19T22:10:11
The driver of the eruption is probably located behind the limb, but sideway motions of dark filament material get intensified with the eruption. Following the eruption, we see dimming, loop oscillations and post-flare loops.

Movie

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2014-05-22T04:52:57
2014-05-19T20:10:11 --> 2014-05-19T22:10:11
The driver of the eruption is probably located behind the limb, but sideway motions of dark filament material get intensified with the eruption. Following the eruption, we see dimming, loop oscillations and post-flare loops.

Movie

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2014-05-22T04:52:57
2014-05-19T20:10:11 --> 2014-05-19T22:10:11
The driver of the eruption is probably located behind the limb, but sideway motions of dark filament material get intensified with the eruption. Following the eruption, we see dimming, loop oscillations and post-flare loops.

Movie

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by halocme, Submitted at 2014-05-22T04:44:14
2014-05-19T05:40:11 --> 2014-05-19T08:40:11
This filament eruption may look simple, but it is more complex than the lifting of a linear structure between what becomes a two-ribbon flare. For example, the eruption completes when the southern part leaves the Sun, but without a 3D reconstruction it is not clear whether that part developed later or just represented a projection of the upper structure.

Movie

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1
Detected by derosa, Submitted at 2014-05-10T23:40:23
2014-05-09T01:00:03 --> 2014-05-09T05:00:03
A filament ejects upward from the west limb

Movie

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