Recent Events Reported by Observers
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Detected by halocme, Submitted at 2015-05-11T20:16:44
2014-06-11T20:30:35 --> 2014-06-11T21:40:11
Like the previous X2.2, M3.1 and X1.0 flares (not the X1.5, which was special in terms of a powerful eruption), this flare was associated with a minor eruption and loop oscillations at higher altitudes. The eruption looks falling back, but at least an unimpressive CME has resulted from it.
Detected by halocme, Submitted at 2015-05-11T20:16:02
2014-06-11T20:30:35 --> 2014-06-11T21:40:11
Like the previous X2.2, M3.1 and X1.0 flares (not the X1.5, which was special in terms of a powerful eruption), this flare was associated with a minor eruption and loop oscillations at higher altitudes. The eruption looks falling back, but at least an unimpressive CME has resulted from it.
Detected by halocme, Submitted at 2015-05-11T20:16:39
2014-06-11T20:30:35 --> 2014-06-11T21:40:11
Like the previous X2.2, M3.1 and X1.0 flares (not the X1.5, which was special in terms of a powerful eruption), this flare was associated with a minor eruption and loop oscillations at higher altitudes. The eruption looks falling back, but at least an unimpressive CME has resulted from it.
Detected by halocme, Submitted at 2015-05-11T20:16:44
2014-06-11T07:50:23 --> 2014-06-11T09:59:59
Like the previous day's successive flares (X2.2 then X1.5), the first one showed a compact ejection. But unlike the previous day's events, the second flare, although more intense in X-rays, was not more dramatic than the first one. Both flares accompanied loop oscillations.
Detected by halocme, Submitted at 2015-05-11T20:16:38
2014-06-11T07:50:23 --> 2014-06-11T09:59:59
Like the previous day's successive flares (X2.2 then X1.5), the first one showed a compact ejection. But unlike the previous day's events, the second flare, although more intense in X-rays, was not more dramatic than the first one. Both flares accompanied loop oscillations.
Detected by halocme, Submitted at 2015-05-11T20:16:02
2014-06-11T07:50:23 --> 2014-06-11T09:59:59
Like the previous day's successive flares (X2.2 then X1.5), the first one showed a compact ejection. But unlike the previous day's events, the second flare, although more intense in X-rays, was not more dramatic than the first one. Both flares accompanied loop oscillations.
Detected by halocme, Submitted at 2015-05-11T20:16:49
2014-06-11T08:55:11 --> 2014-06-11T10:15:35
NW first then NE and SW.
Detected by halocme, Submitted at 2015-05-11T20:15:46
2014-06-10T12:30:35 --> 2014-06-10T13:59:23
The front is seen primarily along the limb, both clockwise and counterclockwise. Computation of coronal toplogical objects may tell us why the front is hardly seen on the disk.
Detected by halocme, Submitted at 2014-06-16T06:16:24
2014-06-10T13:30:27 --> 2014-06-10T17:30:27
For a few hours after the X1.5 flare the east limb was still in a disturbed state with continued outflows.
Detected by halocme, Submitted at 2015-05-11T20:16:38
2014-06-10T11:30:35 --> 2014-06-10T13:59:23
The first flare, at X2.2, showed a compact ejection. The second flare, at X1.5, was much more eruptive, associated with large-scale disturbances. Close to the flare region, coronal dimming and loop oscillations associated with the X1.5 flare are clear even in intensity images.
Detected by halocme, Submitted at 2015-05-11T20:16:43
2014-06-10T11:30:35 --> 2014-06-10T13:59:23
The first flare, at X2.2, showed a compact ejection. The second flare, at X1.5, was much more eruptive, associated with large-scale disturbances. Close to the flare region, coronal dimming and loop oscillations associated with the X1.5 flare are clear even in intensity images.
Detected by halocme, Submitted at 2015-05-11T20:16:02
2014-06-10T11:30:35 --> 2014-06-10T13:59:23
The first flare, at X2.2, showed a compact ejection. The second flare, at X1.5, was much more eruptive, associated with large-scale disturbances. Close to the flare region, coronal dimming and loop oscillations associated with the X1.5 flare are clear even in intensity images.
Detected by halocme, Submitted at 2015-05-11T20:13:30
2014-06-10T11:30:35 --> 2014-06-10T13:59:23
The first flare, at X2.2, showed a compact ejection. The second flare, at X1.5, was much more eruptive, associated with large-scale disturbances. Close to the flare region, coronal dimming and loop oscillations associated with the X1.5 flare are clear even in intensity images.
Detected by halocme, Submitted at 2015-05-11T20:16:01
2014-06-10T10:55:11 --> 2014-06-10T11:55:11
We often see the erupted material fall back in 304 A, but not at coronal temperatures like this.
Detected by halocme, Submitted at 2015-05-11T20:13:33
2014-06-10T05:00:03 --> 2014-06-10T05:45:39
This jet started at the western periphery of an active region. It seems that the reconnection processes involved field lines into the umbra (to northeast).
Detected by halocme, Submitted at 2015-05-11T20:16:43
2014-06-09T17:00:03 --> 2014-06-09T17:39:39
This flare at AR 10287 looks spiky in GOES X-ray light curves. But it was responsible for loop oscillations and a slow eruption. As a result, a narrow CME was seen in LASCO data.
Detected by halocme, Submitted at 2015-05-11T20:16:38
2014-06-09T17:00:03 --> 2014-06-09T17:39:39
This flare at AR 10287 looks spiky in GOES X-ray light curves. But it was responsible for loop oscillations and a slow eruption. As a result, a narrow CME was seen in LASCO data.
Detected by halocme, Submitted at 2015-05-11T20:16:52
2014-06-09T07:10:12 --> 2014-06-09T07:40:12
This flare in AR 12080 accompanied a surge-like ejection toward southwest. Note that the remote area in that direction brightened. It is not clear the brightening in the loop structure to the east was induced by the flare.
Detected by halocme, Submitted at 2015-05-11T20:16:37
2014-06-09T07:10:12 --> 2014-06-09T07:40:12
This flare in AR 12080 accompanied a surge-like ejection toward southwest. Note that the remote area in that direction brightened. It is not clear the brightening in the loop structure to the east was induced by the flare.
Detected by halocme, Submitted at 2015-05-11T20:16:28
2014-05-30T23:30:35 --> 2014-05-31T04:00:35
This eruption suggests out of the plane-of-the-sky motions, which also contain untwisting. A narrow CME seems to be associated with this eruption.
