Recent Events Reported by Observers
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Detected by halocme, Submitted at 2014-01-09T06:41:41
2013-12-20T20:00:31 --> 2013-12-21T05:00:31
This is a minor eruption primarily seen in 304 A channel. Like other cases, the prominence erupts with untwisting motions.
Detected by halocme, Submitted at 2014-01-09T06:33:17
2013-12-20T10:30:00 --> 2013-12-20T13:00:00
This flare was preceded by a C2.2 flare. It may have played a role of destabilizing the structure that was erupted in a limited way in the main flare. The eruption appears to be largely confined, although leaving some dimming signatures.
Detected by halocme, Submitted at 2014-01-09T06:33:16
2013-12-20T10:30:00 --> 2013-12-20T13:00:00
This flare was preceded by a C2.2 flare. It may have played a role of destabilizing the structure that was erupted in a limited way in the main flare. The eruption appears to be largely confined, although leaving some dimming signatures.
Detected by halocme, Submitted at 2014-01-09T06:33:16
2013-12-20T10:30:00 --> 2013-12-20T13:00:00
This flare was preceded by a C2.2 flare. It may have played a role of destabilizing the structure that was erupted in a limited way in the main flare. The eruption appears to be largely confined, although leaving some dimming signatures.
Detected by halocme, Submitted at 2015-05-11T20:16:21
2013-12-20T06:30:35 --> 2013-12-20T10:30:35
The filament lay north of AR 11920. The movie captures its slow rise, and the coronal response after the filament reached the cirtain height. Two-ribbon emission is seen, not reaching the GOES background level in X-rays.
Detected by slater, Submitted at 2014-01-09T04:34:50
2014-01-07T17:30:35 --> 2014-01-08T03:30:35
Large eruptive flare from AR 11944. Complex multi-ribbons (at least three). Flare associated with flux system connecting the leading spot of the region with decaying active region flux to the west. Two sets of post flare loops connecting two different flux systems. Blast directed to the southwest.
Detected by slater, Submitted at 2014-01-09T02:37:50
2014-01-07T00:00:03 --> 2014-01-08T00:00:03
Continuing reconnection at quadrupolar magnetic separator between ARs 11944 and 11946 in the 24 hour period leading up to an X flare.
Detected by cheung, Submitted at 2014-01-07T01:25:32
2014-01-06T05:10:03 --> 2014-01-06T07:20:03
Most of the filamentary material (304, orange) from this eruption seems to slide back down toward the lower atmosphere. Nevertheless the temporal change in the off-limb signal in 211 (green) sugguests an irrevocable change in the large-scale coronal field.
Detected by cheung, Submitted at 2014-01-07T01:17:24
2014-01-06T02:30:03 --> 2014-01-06T04:50:03
ARs 11944 and 11946 form a quadrapolar magnetic configuration with loops that straddle across the equatorial plane. The apparent motion of kinked EUV loop tops in this system is suggestive of separator reconnection.
Detected by cheung, Submitted at 2014-01-07T00:55:56
2014-01-05T17:40:03 --> 2014-01-05T18:50:03
Surges are launched in succession at the edge of this emerging flux region.
Detected by cheung, Submitted at 2014-01-07T00:55:55
2014-01-05T17:40:03 --> 2014-01-05T18:50:03
Surges are launched in succession at the edge of this emerging flux region.
Detected by schryver, Submitted at 2014-10-14T22:18:03
2014-01-03T11:44:03 --> 2014-01-03T14:56:03
Flare and field reconfiguration.
Detected by schryver, Submitted at 2014-10-14T22:18:14
2014-01-03T11:44:03 --> 2014-01-03T14:56:03
Flare and field reconfiguration.
Detected by cheung, Submitted at 2014-01-07T00:51:31
2014-01-05T15:56:03 --> 2014-01-05T16:50:03
The two jets occur in succession and both exhibit apparent rotational motion.
Detected by schryver, Submitted at 2014-10-14T22:17:51
2014-01-03T00:40:03 --> 2014-01-03T04:52:03
Prominence eruption
Detected by schryver, Submitted at 2014-10-14T22:17:51
2014-01-03T15:24:03 --> 2014-01-03T19:08:03
QS filament eruption
Detected by cheung, Submitted at 2014-01-07T00:45:42
2014-01-05T02:20:03 --> 2014-01-05T02:50:03
The filamentary material ejected from this eruption seems to experience an abrupt change in flow direction, as if it were reflecting off a stiff barrier in the mid-corona.
Detected by cheung, Submitted at 2014-01-07T00:45:40
2014-01-05T02:20:03 --> 2014-01-05T02:50:03
The filamentary material ejected from this eruption seems to experience an abrupt change in flow direction, as if it were reflecting off a stiff barrier in the mid-corona.
Detected by cheung, Submitted at 2014-01-07T00:35:11
2014-01-04T19:30:03 --> 2014-01-05T01:10:03
This eruption is possibly associated with the GOES M4.0 flare which peaked at 2014-01-04T19:46:00. The post-eruption arcade loops seem to slide past each other in a counter-propagating direction, suggestive of slip-running reconnection.
Detected by cheung, Submitted at 2014-01-07T00:35:11
2014-01-04T19:30:03 --> 2014-01-05T01:10:03
This eruption is possibly associated with the GOES M4.0 flare which peaked at 2014-01-04T19:46:00. The post-eruption arcade loops seem to slide past each other in a counter-propagating direction, suggestive of slip-running reconnection.