Recent Events Reported by Observers
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Detected by Gregal Vissers, Submitted at 2017-09-14T18:36:09
2017-08-31T08:02:57 --> 2017-08-31T09:13:55
Flare and (failed) eruption in leading part of AR12672, partly covered by the rastering slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T18:30:48
2017-08-31T15:08:50 --> 2017-08-31T15:57:36
Small flare in AR12674, partly sampled by the rastering slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T18:29:03
2017-08-31T06:56:25 --> 2017-08-31T07:21:55
Small flare ribbon lighting up twice in trailing part of AR12672, not covered by the slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T18:25:14
2017-08-31T06:09:51 --> 2017-08-31T10:52:37
UV bursts and flaring fibrils in trailing part of AR12672. The slit rasters across the sub-FOV multiple times catching several events.
Detected by Gregal Vissers, Submitted at 2017-09-14T18:14:40
2017-08-30T23:46:38 --> 2017-08-31T03:30:50
UV bursts and flaring fibrils in AR12674, some sampled multiple times by the rastering slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T18:11:49
2017-08-30T21:23:27 --> 2017-08-30T22:59:47
Several large (coronal) jets in the trailing part of AR12672, not sampled by the slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:59:52
2017-08-30T18:08:51 --> 2017-08-30T18:20:51
Coronal jet in AR12672, outside the range of the raster.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:56:05
2017-08-30T17:54:41 --> 2017-08-30T18:27:24
UV bursts and flaring fibrils in AR12672, outside the range of the raster.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:53:30
2017-08-30T16:03:41 --> 2017-08-30T16:49:09
Small flare in leading part of AR12672 (probably B-class; not highlighted on SolarMonitor), just outside the raster range.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:45:27
2017-08-30T13:17:21 --> 2017-08-30T16:49:09
Flaring fibrils and UV bursts in trailing part of AR12672, scanned several times by the rastering slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:42:04
2017-08-30T04:19:53 --> 2017-08-30T05:10:53
Flaring fibrils in trailing part of AR12672. The slit rasters across the fibrils as the brightenings extend from one footpoint to the other.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:39:37
2017-08-30T04:19:53 --> 2017-08-30T05:23:05
Coronal jet in trailing part of AR12672, not sampled by slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:29:53
2017-08-29T18:03:27 --> 2017-08-29T22:56:44
UV bursts in emerging flux near disc center, not covered by sit-and-stare slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:26:50
2017-08-29T05:36:25 --> 2017-08-29T05:36:25
Coronal jet-like eruption in AR12673 sampled once by the scanning slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:13:32
2017-08-29T12:00:41 --> 2017-08-29T12:58:21
Several UV bursts in trailing part of AR12672 sampled once by the scanning slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:12:12
2017-08-29T12:26:11 --> 2017-08-29T12:58:21
Several UV bursts in AR12672 just outside the reach of the slit.
Detected by Gregal Vissers, Submitted at 2017-09-14T17:10:36
2017-08-29T12:00:41 --> 2017-08-29T12:58:21
Several repetitive coronal jets in AR12672, two of which are sampled once by the scanning slit.
Detected by halocme, Submitted at 2017-09-14T08:41:15
2017-09-12T19:00:09 --> 2017-09-12T20:00:09
The flare was again in AR 12680, and there seemed two eruptions, producing a wave that moved mostly southward.
Detected by halocme, Submitted at 2017-09-14T08:41:25
2017-09-12T15:15:01 --> 2017-09-12T16:30:37
A B3.5 flare in AR 12680 was associated with an eruption moving northward, and as it hit coronal structures, it produced a wave, which is more diffuse than normal large-scale coronal propagating fronts.
Detected by halocme, Submitted at 2017-09-14T08:41:14
2017-09-12T15:15:01 --> 2017-09-12T16:30:37
A B3.5 flare in AR 12680 was associated with an eruption moving northward, and as it hit coronal structures, it produced a wave, which is more diffuse than normal large-scale coronal propagating fronts.