Recent Events Reported by Observers
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Detected by halocme, Submitted at 2012-06-02T16:50:18
2012-05-18T12:00:04 --> 2012-05-18T17:00:04
Over this five hour period, the cavity becomes less noticeable. Is this due just to projection effect? Not much action is seen to come from lower down.
Detected by halocme, Submitted at 2012-06-02T16:31:48
2012-05-18T14:20:25 --> 2012-05-18T15:10:25
Although we certainly note outward motions, they are confined. Therefore this C1.3 flare has no global effects and not regarded as eruptive (no CME).
Detected by halocme, Submitted at 2012-06-02T16:24:40
2012-05-18T11:00:04 --> 2012-05-18T12:20:04
This one is again most readily seen at 211 A, but 171 A images do show a mini filament in absorption and a possibly footpoint brightening. Therefore the source region is on the visible side.
Detected by halocme, Submitted at 2012-06-02T16:15:15
2012-05-18T06:50:24 --> 2012-05-18T08:00:24
They perhaps emanate from backside regions. Pronounced in the 211 A channel almost without any signatures at 171 A or 30a A.
Detected by halocme, Submitted at 2012-06-02T16:08:59
2012-05-18T04:40:12 --> 2012-05-18T06:10:12
This event results in dimming south of AR 1482, but the the filament eruption was toward west and north (in the plane of the sky).
Detected by cheung, Submitted at 2014-02-10T02:14:19
2012-05-27T02:00:04 --> 2012-05-27T06:40:04
The tall-standing bright loops disappear after the eruption. Instead, one finds a post-eruption arcade closer to the core of the AR.
Detected by cheung, Submitted at 2014-02-10T02:14:27
2012-05-29T20:20:04 --> 2012-05-30T03:50:04
This filament eruption occurs simultaneously with the one in the northeastern limb.
Detected by cheung, Submitted at 2014-02-10T02:14:27
2012-05-29T20:20:04 --> 2012-05-30T03:50:04
This filament eruption occurs simultaneously with the one in the northwestern limb.
Detected by cheung, Submitted at 2014-02-10T02:14:27
2012-05-30T01:40:04 --> 2012-05-30T03:20:04
The rise of the filament material is halted and the material drains back down to the footpoints of the relaxed magnetic structure.
Detected by cheung, Submitted at 2014-02-10T02:14:22
2012-05-30T01:40:04 --> 2012-05-30T03:20:04
The rise of the filament material is halted and the material drains back down to the footpoints of the relaxed magnetic structure.
Detected by cheung, Submitted at 2014-02-10T02:14:34
2012-05-29T17:00:04 --> 2012-05-29T18:30:04
Much of the material apparently drains back toward the footpoints of the surge.
Detected by cheung, Submitted at 2014-02-10T02:14:22
2012-05-28T14:55:04 --> 2012-05-28T17:27:34
This filament has footpoints behind the limb since there is a lack of footpoint brightening in the EUV images.
Detected by schryver, Submitted at 2012-05-29T20:45:30
2012-05-26T08:36:04 --> 2012-05-26T11:16:04
Eruption from small AR near E limb
Detected by schryver, Submitted at 2012-05-29T20:43:56
2012-05-26T20:16:04 --> 2012-05-26T21:47:04
Over-the-limb eruption with strong loop oscillations excited in another region, of which the base also lies just beyond the W limb.
Detected by schryver, Submitted at 2012-05-29T20:43:57
2012-05-26T20:16:04 --> 2012-05-26T21:47:04
Over-the-limb eruption with strong loop oscillations excited in another region, of which the base also lies just beyond the W limb.
Detected by schryver, Submitted at 2012-05-25T21:12:17
2012-05-24T22:01:16 --> 2012-05-25T02:29:16
Filament eruption
Detected by schryver, Submitted at 2012-05-25T21:09:04
2012-05-24T00:00:04 --> 2012-05-25T00:00:04
A filament eruption on the W limb happens synchronously with an eruption in a smallish AR on the E hemisphere.
Detected by schryver, Submitted at 2012-05-25T21:06:24
2012-05-24T10:16:04 --> 2012-05-24T14:52:04
Filament activation
Detected by schryver, Submitted at 2012-05-25T21:04:45
2012-05-24T16:04:04 --> 2012-05-25T00:00:04
Filament eruption
Detected by anny, Submitted at 2012-05-21T21:48:09
2012-05-17T02:33:04 --> 2012-05-17T05:06:04
As a prominence lifts up and reconnects with the surrounding field, passing through an upside down V-shaped structure, the inner edge of the "V" develops a bright front in 171A.
