Highest Rated Events (only 193 and 304 shown) All AR FE FL
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-24T18:36:53
2015-08-23T03:40:06 --> 2015-08-23T05:40:06
A filament erupts from a small bipolar regions surrounded by very quiet sun and adjacent to a CH channel. The erupting event appears to remain 'collimated' over a large range as the event propagates towards the SE as seen against the disk.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-24T18:34:46
2015-08-23T17:48:06 --> 2015-08-23T23:28:06
Flare/eruption from a moderate AR in the S hemisphere, with signatures of a large eruption, including coronal/thermal restructuring towards the SE over a large patch of QS.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-24T18:34:46
2015-08-23T17:48:06 --> 2015-08-23T23:28:06
Flare/eruption from a moderate AR in the S hemisphere, with signatures of a large eruption, including coronal/thermal restructuring towards the SE over a large patch of QS.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-24T18:06:05
2015-08-22T20:32:10 --> 2015-08-22T23:44:10
Confined flare.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-24T18:04:42
2015-08-22T06:04:10 --> 2015-08-22T09:28:10
A flare from an AR in the S hemisphere leads to reconfiguration and a large-scale clear propagating front reaching to the far N of the N hemisphere, while loop oscillations are seen in the outlying loops of the exploding AR and connections to a small AR towards the N.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-24T18:04:42
2015-08-22T06:04:10 --> 2015-08-22T09:28:10
A flare from an AR in the S hemisphere leads to reconfiguration and a large-scale clear propagating front reaching to the far N of the N hemisphere, while loop oscillations are seen in the outlying loops of the exploding AR and connections to a small AR towards the N.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-24T15:41:05
2015-08-21T11:24:06 --> 2015-08-21T14:44:06
Eruption from trailing end and QS behind a moderate AR.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-24T15:39:17
2015-08-21T09:12:06 --> 2015-08-21T13:08:06
Flare/eruption with pronounced (thermal) distortion of nearby QS (towards NNW) and a propagating front most clearly towards the N regions.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-24T15:34:44
2015-08-21T02:12:06 --> 2015-08-21T05:28:06
Flare with arcade.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-21T16:37:18
2015-08-20T04:24:06 --> 2015-08-20T07:52:06
AR eruption with strong post-eruption arcade, with connections (dimmings) into QS to N and W, and a faint propagating wave signature primarily visible towards the N and NNW.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-21T16:37:17
2015-08-20T04:24:06 --> 2015-08-20T07:52:06
AR eruption with strong post-eruption arcade, with connections (dimmings) into QS to N and W, and a faint propagating wave signature primarily visible towards the N and NNW.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-21T16:24:15
2015-08-19T11:52:06 --> 2015-08-19T17:48:06
An active region and connected QS filament activate, nad are involved in an eruption from the SE limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-19T15:38:51
2015-08-18T21:20:06 --> 2015-08-19T04:00:06
QS filament/prominence activates over the NW limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2015-08-19T15:36:18
2015-08-18T00:00:06 --> 2015-08-18T03:40:06
QS prominence activates over the SE limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-08-17T00:40:22
2015-08-15T12:00:06 --> 2015-08-15T13:09:42
The coronal wave is associated with a C1.6 flare in AR 12401 that followed the collision of a narrow ejection with coronal structures east of the region - this also appears as a small hump in the GOES light curves. Two CME seem to correspond to the narrow ejection and wave, but neither of them is impressive.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-08-17T00:40:21
2015-08-15T12:00:06 --> 2015-08-15T13:09:42
The coronal wave is associated with a C1.6 flare in AR 12401 that followed the collision of a narrow ejection with coronal structures east of the region - this also appears as a small hump in the GOES light curves. Two CME seem to correspond to the narrow ejection and wave, but neither of them is impressive.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-08-17T00:25:04
2015-08-15T11:00:06 --> 2015-08-15T12:39:42
This eruption did not become a big CME, but it showed some interesting features such as dual dimming across the polarity inversion line and loop shrinkage prior to the eruption. This was almost a non-event in 304 A.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-08-17T00:06:12
2015-08-14T16:40:10 --> 2015-08-14T20:00:10
In H-alpha this filament appeared very dark before the eruption, which itself was not extended and resulted in only a minor CME. The ribbon brightenings (below the GOES background level) indicate a multipolar topology of the magnetic field that was involved in the eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-08-16T23:58:47
2015-08-14T07:00:06 --> 2015-08-14T10:30:06
This eruption follows almost two hours of activation in which the filament is seen to rise slowly. The eruption consists of helical motions and resulted in two-ribbon-like brightening below the GOES background level.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-08-16T23:45:36
2015-08-13T00:00:06 --> 2015-08-13T02:30:06
The turbulent motions seem to be between the two legs of the filament, but they may have driven part of the filament to erupt,
