Highest Rated Events (only 193 and 304 shown) All AR FE FL
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T16:58:00
2012-03-09T03:15:36 --> 2012-03-09T04:45:36
The propagating front is obvious in intensity images at all of the three wavelengths (211A, 193A and 171A). It seems that the southward front is blocked by two active regions before reaching the coronal hole. How about the northward front? Let's discuss it privately.
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3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T16:32:58
2012-03-08T21:15:00 --> 2012-03-08T22:15:00
The prominence eruption in 304 A images looks confined, but material is seen moving out in a narrow channel in coronal channels.
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3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T16:24:38
2012-03-08T19:20:24 --> 2012-03-08T21:00:24
This is again likely to be from a region behind the limb. It is not clear if this is a separate from the previous event. The associated CME is more bullet-like (narrow) than loop-like. The loops in the northern part of the movie seem to be post-eruption loops, meaning that the region was part of the previous eruption. The cusp-like dark region over these loops is mostly in 171 A images, meaning high temperatures.
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3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T16:01:33
2012-03-08T14:30:00 --> 2012-03-08T18:32:00
The prominence standing over the limb is seen to gradually rise. It is not clear if a small eruption in the disk region has to do with triggering the eruption of the prominence. The southern part is more clearly opened up, throwing material northward, hence the appearance of the associated CME in LASCO data that is extended to north.
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3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T15:19:37
2012-03-08T09:50:24 --> 2012-03-08T12:20:24
Two filament eruptions are seen around the same time near central meridian and on the west limb.
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3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T07:55:40
2012-03-08T03:00:00 --> 2012-03-08T04:32:00
As a prominence moves out untwisted the overlying corona appears to dim (at 171 A and 211 A).
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3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T07:28:39
2012-03-06T00:00:04 --> 2012-03-08T00:00:04
This movie gives an impression that the cavity becomes clearer as the prominence material starts to stay at certain heights.
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3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T07:12:05
2012-03-07T20:40:12 --> 2012-03-07T21:40:12
This is a minor jet. Jets tend to recur, but this one does not seem to . It is seen primarily at 193 A (not clear at 211 A or 171 A).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T06:54:59
2012-03-07T08:50:24 --> 2012-03-07T10:30:24
The eruption is clear in 211 A images, but its relation with motions of the prominence at 304 A is not clear.
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3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T06:44:53
2012-03-07T00:00:04 --> 2012-03-07T02:00:04
Very spectacular event. STEREO-B data show that the propagation is more pronounced in latitudinal than in longitudinal directions. Note that the X5.4 flare was followed by a X1.3 flare, which was also associated with a coronal wave, mostly in the soutwestward direction.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-15T06:10:25
2012-03-06T12:20:25 --> 2012-03-06T13:40:13
Small-scale motions are seen, but they do not make this flare eruptive - no CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-13T01:20:32
2012-03-05T21:40:12 --> 2012-03-05T22:40:12
This jet seems to start around the end of a filament (or loop) as it goes down. But their relation is not clear.
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3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-13T01:09:14
2012-03-05T18:00:05 --> 2012-03-05T20:00:05
This movie contains three flares (one C-class and two M-class), but none of them is eruptive although they show motions clong closed loops.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-13T00:55:53
2012-03-05T09:30:00 --> 2012-03-05T12:00:00
The eruption of the filament material is well traced in the three channels, but the 211 A images do not clearly show a front. The associated CME is narrow and not spectacular.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-12T23:35:45
2012-03-04T19:00:04 --> 2012-03-04T22:00:04
The LASCO C2 difference image of 21:24-20:36 shows a bright CME with irregular shape on the NE limb, but the next frames are left with an unimpressive outflow which may not qualify as a CME. This movie again shows that only the 211 A channel (out of the 304-211-171 combination) indicates large-scale eruptions, possibly corresponding to the CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-12T22:50:05
2012-03-04T17:10:13 --> 2012-03-04T18:19:49
Associated with a C3.2 flare, this does not seem to be a full-blown eruption. Indeed no CME is associated.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-07T22:40:48
2012-03-04T10:00:05 --> 2012-03-04T12:00:05
A clear EUV wave even in intensity images. But full-disk running difference images show propagating disturbances both over the limb and on disk. This event was a partial halo CME. The movie shown here nicely captures post-eruption high-temperature regions including current sheets.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2012-03-07T20:56:53
2012-03-04T02:45:00 --> 2012-03-04T03:46:12
No flare obviously associated with this eruption. It is too minor to lead to a CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2012-03-06T01:30:44
2012-03-03T17:00:04 --> 2012-03-04T05:00:04
Eruption and small flare just inside the NE limb, with a very unusual (and pretty) set of post-event loops: sharply-cusped loops towards the N and a strongly-inclinded glowing arcade towards the S (over a region where a smallish eruption seems to have started the sequence).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by berger, Submitted at 2012-02-28T22:21:23
2012-02-24T10:24:04 --> 2012-02-24T13:54:04
Small/moderate sized prominence bubble propagates through quiescent prominence on SW limb.