Highest Rated Events (only 193 and 304 shown) All AR FE FL
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2014-08-04T20:02:47
2014-07-09T01:16:03 --> 2014-07-09T03:50:03
Some flows around and above a filament. 304A shows the path of the flows, and 171A shows the location of the footpoints. Note how the end point of the flows "sweeps" from one location to the other.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T05:26:07
2014-07-14T17:35:23 --> 2014-07-14T18:31:23
This may be classified as a jet, even though the motions look mostly horizontal. This appearance probably reflects the field configurations around the region.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T05:21:14
2014-07-14T15:05:23 --> 2014-07-14T16:21:23
This surge-like event is most clearly seen at 304 A, suggesting that the main body is much cooler than the surrounding corona. The adjecent structure seems to be hardly affected.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T05:14:36
2014-07-13T20:10:11 --> 2014-07-13T21:10:11
The subtle change associated with a minor eruption is seen at the edge of a streamer-like structurem only at high altitudes.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T05:07:30
2014-07-13T12:55:11 --> 2014-07-13T15:15:11
This eruption is highly non-radial. It is probably driven on the back side. We see oscillations in the material as it is ejected from the reconnection region.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T05:07:28
2014-07-13T12:55:11 --> 2014-07-13T15:15:11
This eruption is highly non-radial. It is probably driven on the back side. We see oscillations in the material as it is ejected from the reconnection region.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T04:56:47
2014-07-12T20:25:11 --> 2014-07-12T21:35:11
A minor eruption is immediately followed by another one to southeast, suggesting a possible link of the two regions.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T04:56:47
2014-07-12T20:25:11 --> 2014-07-12T21:35:11
A minor eruption is immediately followed by another one to southeast, suggesting a possible link of the two regions.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T04:51:36
2014-07-12T13:15:35 --> 2014-07-12T15:15:35
Large-scale loops standing on the southwest limb are seen to move sideways, indicating an eruptiuon from the far side. The prominence in the 304 A channel seems to belong to a different structure, not affected by the eruptiuon.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T04:42:46
2014-07-12T03:15:35 --> 2014-07-12T04:15:35
This indicates that the jet was driven by reconnection of low-lying loops at their footpoint, another example of Shibata-type jet.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T04:34:48
2014-07-11T23:30:35 --> 2014-07-12T00:20:59
The small eruption associated with a C2.3 flare had global effects. Loop oscillations (three shakes are included in the movie) were seen as the large-scale coronal propagating front was triggered counterclockwise along the limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T04:34:47
2014-07-11T23:30:35 --> 2014-07-12T00:20:59
The small eruption associated with a C2.3 flare had global effects. Loop oscillations (three shakes are included in the movie) were seen as the large-scale coronal propagating front was triggered counterclockwise along the limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-19T04:34:47
2014-07-11T23:30:35 --> 2014-07-12T00:20:59
The small eruption associated with a C2.3 flare had global effects. Loop oscillations (three shakes are included in the movie) were seen as the large-scale coronal propagating front was triggered counterclockwise along the limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-11T05:05:06
2014-07-08T16:00:03 --> 2014-07-08T18:20:03
This flare was associated with the eruption of a bright and irregular-shaped prominence and a fast (~900 km s{-1}) partial halo CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-11T05:05:05
2014-07-08T16:00:03 --> 2014-07-08T18:20:03
This flare was associated with the eruption of a bright and irregular-shaped prominence and a fast (~900 km s{-1}) partial halo CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-11T04:47:34
2014-07-09T00:00:03 --> 2014-07-09T01:10:03
This flare, in AR 2113, was less eruptive than the earlier M6.5 flare from the same region. But we see clear loop oscillations, suggiestive of shock waves. There is some indication of a large-scale coronal propagating front (LCPF).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-11T04:47:33
2014-07-09T00:00:03 --> 2014-07-09T01:10:03
This flare, in AR 2113, was less eruptive than the earlier M6.5 flare from the same region. But we see clear loop oscillations, suggiestive of shock waves. There is some indication of a large-scale coronal propagating front (LCPF).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-11T04:39:48
2014-07-08T08:40:12 --> 2014-07-08T10:10:12
This shares some characteristics of eruptive flares (e.g., formation of an arcade with a hot cusp) , but the eruption is limited to north.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-11T04:39:48
2014-07-08T08:40:12 --> 2014-07-08T10:10:12
This shares some characteristics of eruptive flares (e.g., formation of an arcade with a hot cusp) , but the eruption is limited to north.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-11T04:24:01
2014-07-08T06:30:35 --> 2014-07-08T07:50:35
This looks like a compact and narrow ejection, but it may be quite powerful, given the oscillations of the overlying structures. Perhaps shock waves were launched.
