Recent Events Reported by Observers
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Detected by schryver, Submitted at 2011-12-02T01:06:56
2011-11-30T15:40:04 --> 2011-12-01T00:00:04
Prominence activation and eruption
Detected by schryver, Submitted at 2011-12-02T01:04:05
2011-11-30T18:48:04 --> 2011-12-01T00:00:04
Filament eruption
Detected by halocme, Submitted at 2011-12-01T16:43:42
2011-11-29T02:00:04 --> 2011-11-29T04:00:04
This eruption/opening should have been from the back side because of no obvious events on the visible side. The eruption is more easily seen at 211 A/193 A than at 171 A. This did not survive into the LASCO field of view.
Detected by halocme, Submitted at 2011-12-01T06:42:54
2011-11-28T21:15:00 --> 2011-11-28T23:17:00
This is essentially the same phenomenon that was reported as a long-lasting outflow. Now it is clear that the motions were along closed structures.
Detected by halocme, Submitted at 2011-12-01T06:32:21
2011-11-28T15:50:24 --> 2011-11-28T18:20:24
A flux-rope like feature is seen at 171 A and 193 A. The flux rope is probably more east-west oriented than north-south. The prominence seen at 304 A does not seem to participate in the eruption. This event becomes an unimpressive CME seen by LASCO.
Detected by halocme, Submitted at 2011-12-01T06:17:15
2011-11-28T11:30:00 --> 2011-11-28T13:32:00
A jet-like outflow from the same region as the one four hours before. Note how this disturbes a filament.
Detected by halocme, Submitted at 2011-12-01T06:07:38
2011-11-28T07:30:00 --> 2011-11-28T09:30:00
An jet-like outflow is seen for almost two hours. It apparently interacts with filament material.
Detected by halocme, Submitted at 2011-12-01T02:53:12
2011-11-28T04:30:00 --> 2011-11-28T08:00:00
The filament is on the front side, and yet no obvious flare associated. The eruption resuted in an extended CME (not quite a halo).
Detected by halocme, Submitted at 2011-12-01T00:29:16
2011-11-30T18:30:00 --> 2011-11-30T21:00:00
The movie is given in reverse color. The northern leg got loose first. Part of the prominence material is shared in the three wavelengths, but these images indicate a distribution in temperature.
Detected by schryver, Submitted at 2011-11-30T00:48:29
2011-11-29T05:44:04 --> 2011-11-29T09:00:04
Material at the eastern end of a QS filament brightens and moves upward, making an apparent loop, to descend again towards the western end of the filament configuration. Oscillations are excited in the dark filament underneath this rope-like configuration.
Detected by schryver, Submitted at 2011-11-30T00:48:22
2011-11-29T05:44:04 --> 2011-11-29T09:00:04
Material at the eastern end of a QS filament brightens and moves upward, making an apparent loop, to descend again towards the western end of the filament configuration. Oscillations are excited in the dark filament underneath this rope-like configuration.
Detected by derosa, Submitted at 2011-11-30T00:41:24
2011-11-23T12:00:04 --> 2011-11-24T00:00:04
Coronal cavity associated with two bonsai trees in the 211A channel of AIA in the southern hemisphere
Detected by derosa, Submitted at 2011-11-30T00:05:16
2011-11-23T11:00:04 --> 2011-11-23T16:00:04
Failed eruption or surges associated with the C flare in AR11346
Detected by derosa, Submitted at 2011-11-29T23:13:39
2011-11-23T01:00:04 --> 2011-11-23T05:00:04
Surge associated with the C flare from AR11356 that nicely traces out some closed field lines.
Detected by halocme, Submitted at 2011-11-28T22:43:50
2011-11-19T01:00:04 --> 2011-11-19T03:00:04
Should this also be counted as a coronal jet? The source region seems to be slightly behind the limb. The associated flare is barely C-class. The effect on sorruounding structure is best seen at 211 A.
Detected by halocme, Submitted at 2011-11-28T17:39:13
2011-11-25T21:00:36 --> 2011-11-25T23:00:36
The event was associated with a C2.4 flare. The filament material is seen to come back at 304 A.
Detected by halocme, Submitted at 2011-11-28T16:36:11
2011-11-23T08:30:00 --> 2011-11-23T10:00:00
The source region must be on the back side. The filament material is seen on the right, whereas the loop-like ejection (corresponding to the main CME structure) on the left, only at 211 A in this wavelength combination.
Detected by halocme, Submitted at 2011-11-27T22:31:12
2011-11-24T23:00:04 --> 2011-11-25T01:59:28
This event seems to consist of large-scale motions (perhaps closely tracking the CME) followed fast and recurrent waves (notably at 171 A).
Detected by halocme, Submitted at 2011-11-26T20:12:40
2011-11-26T05:30:00 --> 2011-11-26T09:00:00
This event may lack an explosive appearance, but it apparently corresponds to the interplanetary type II burst that has been reported, which seems to be related with a particle event. See the latest event graphics.
Detected by halocme, Submitted at 2011-11-26T19:55:06
2011-10-10T14:30:00 --> 2011-10-10T14:50:24
The C4.5 flare was short-lived (~7 min), but associated with a global wave. The way it propagated is quite interesting. STEREO data suggest that the motion was largely horizontal (i.e., hardly a CME)
