Recent Events Reported by Observers
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Detected by schryver, Submitted at 2012-08-30T15:31:42
2012-08-28T00:48:03 --> 2012-08-28T08:20:03
Flux emergence next to (and trailing) a weak, decayed AR leads to the eruption of a small filament. The associated coronal front propagates at least to northward of the northern polar crown filament. Subsequently, a larger eruption occurs in the remains of the AR.
Detected by schryver, Submitted at 2012-08-30T15:31:41
2012-08-28T00:48:03 --> 2012-08-28T08:20:03
Flux emergence next to (and trailing) a weak, decayed AR leads to the eruption of a small filament. The associated coronal front propagates at least to northward of the northern polar crown filament. Subsequently, a larger eruption occurs in the remains of the AR.
Detected by weiliu, Submitted at 2012-08-28T23:21:25
2012-08-27T14:50:03 --> 2012-08-27T15:40:03
Small flare with ribbons.
Detected by weiliu, Submitted at 2012-08-28T22:20:25
2012-08-27T08:40:03 --> 2012-08-27T11:50:03
A loop-shaped prominence (304, red) erupted on the SW limb, exhibiting unwinding twists; this is immediately followed by another eruption nearby seen at 211 (pale blue).
Detected by weiliu, Submitted at 2012-08-28T22:20:25
2012-08-27T08:40:03 --> 2012-08-27T11:50:03
A loop-shaped prominence (304, red) erupted on the SW limb, exhibiting unwinding twists; this is immediately followed by another eruption nearby seen at 211 (pale blue).
Detected by weiliu, Submitted at 2012-08-28T21:45:35
2012-08-25T22:40:03 --> 2012-08-26T01:00:03
A small flare occured in this AR, producing double (or more) ribbons.
Detected by weiliu, Submitted at 2012-08-28T20:42:30
2012-08-26T18:12:03 --> 2012-08-26T18:56:03
Loop-shaped, small-scale mini-prominence eruption.
Detected by weiliu, Submitted at 2012-08-28T20:39:27
2012-08-26T17:00:03 --> 2012-08-26T19:30:03
Another cloud prominence over west limb.
Detected by weiliu, Submitted at 2012-08-28T20:37:19
2012-08-26T17:00:03 --> 2012-08-26T19:30:03
Recurrent surges from an AR on the east limb.
Detected by weiliu, Submitted at 2012-08-28T20:30:27
2012-08-25T16:00:03 --> 2012-08-25T17:30:03
A small scale condensation of cool 304 material constantly drains mass, in a so-called "cloud prominence" (Tandberg-Hanssen 1995; S. Martin) configuration, see Liu, Berger, Low (2012, http://adsabs.harvard.edu/abs/2012ApJ...745L..21L) and references there-in; this could be similar to coronal rain in loops (see e.g., Antolin et al. 2012; http://adsabs.harvard.edu/doi/10.1007/s11207-012-9979-7).
Detected by weiliu, Submitted at 2012-08-28T20:20:47
2012-08-25T16:00:03 --> 2012-08-25T17:30:03
A loop-shaped prominence eruption on SW limb, likely from the far side of the visible disk.
Detected by weiliu, Submitted at 2012-08-28T20:14:46
2012-08-25T16:00:03 --> 2012-08-26T06:00:03
A large prominence eruption on the east limb.
Detected by weiliu, Submitted at 2012-08-28T20:10:04
2012-08-25T01:30:03 --> 2012-08-25T02:50:03
A small scale eruption occurred on the east limb, likely originating from the far side of the Sun.
Detected by weiliu, Submitted at 2012-08-28T20:07:10
2012-08-25T00:00:03 --> 2012-08-25T13:00:03
A very long, transequatorial filament channel runs across about 3/4 of the solar disk from north-east to south-west.
Detected by anny, Submitted at 2012-08-22T01:10:06
2012-08-17T20:15:03 --> 2012-08-18T02:40:03
A close-up view on the site of the filament eruption. Despite quite spectacular foorpoint brightening, little of the flux rope is seen erupting until the later stages when it takes off from the field of view (dark feature travelling towards the top left corner).
Detected by anny, Submitted at 2012-08-22T01:00:51
2012-08-17T20:25:03 --> 2012-08-18T09:00:03
The filament itself is not visible well until the last stages of the eruption, hovewer, the post-eruption brightening is quite spectacular in all channels.
Detected by anny, Submitted at 2012-08-21T23:29:17
2012-08-17T20:30:03 --> 2012-08-18T09:00:03
Spray surges seem to be repetitively happening in the same location. What is going on there?
Detected by anny, Submitted at 2012-08-21T23:15:03
2012-08-16T11:15:03 --> 2012-08-16T16:50:03
A coronal dimming is associated with a post-flare arcade and arcade signature in 304A, however there is no evidence of an erupting filament.
Detected by anny, Submitted at 2012-08-21T23:15:02
2012-08-16T11:15:03 --> 2012-08-16T16:50:03
A coronal dimming is associated with a post-flare arcade and arcade signature in 304A, however there is no evidence of an erupting filament.
Detected by anny, Submitted at 2012-08-21T23:08:27
2012-08-16T17:25:03 --> 2012-08-16T19:45:03
The overlying structure which shows in 304 (but not in 211 or 171) is suggestive of that the erupting structure is much thicker than the filament itself, and that the filament resides at its bottom. The cavity does not appear like a sphere, more like a thicker "shell" around the erupting flux rope. It is an interesting observation as I do not recall observing the signature of the top of the cavity that clearly in 304A and not in other channels.
