Recent Events Reported by Observers
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Detected by weiliu, Submitted at 2014-03-07T23:30:11
2014-03-06T12:00:03 --> 2014-03-07T03:10:03
A filament eruption reported yesterday triggered a two-ribbon flare, after which another minor flare went off in the nearby region - sympathy?
Detected by weiliu, Submitted at 2014-03-07T23:30:10
2014-03-06T12:00:03 --> 2014-03-07T03:10:03
A filament eruption reported yesterday triggered a two-ribbon flare, after which another minor flare went off in the nearby region - sympathy?
Detected by weiliu, Submitted at 2014-03-07T23:25:28
2014-03-06T12:00:03 --> 2014-03-07T20:00:03
Rain in both active regions near the equator on the west limb.
Detected by weiliu, Submitted at 2014-03-07T23:19:38
2014-03-06T12:00:03 --> 2014-03-07T20:00:03
The top portion of a prominence gradually lifts off and disappears, suggestive of some sort of heating.
Detected by weiliu, Submitted at 2014-03-07T21:01:26
2014-03-05T20:40:03 --> 2014-03-06T00:00:03
Rapid mass flows (toward the east) in a filament, likely generated by a minor flare at its end toward the west (right-hand side), evidently bifurcate (toward the north and south) when they arrive at a location, indicative of a separator.
Detected by weiliu, Submitted at 2014-03-07T21:01:25
2014-03-05T20:40:03 --> 2014-03-06T00:00:03
Rapid mass flows (toward the east) in a filament, likely generated by a minor flare at its end toward the west (right-hand side), evidently bifurcate (toward the north and south) when they arrive at a location, indicative of a separator.
Detected by halocme, Submitted at 2015-05-11T20:16:36
2014-03-03T15:30:35 --> 2014-03-03T16:29:59
This M1.2 flare consists mainly of a pair of ribbons, but a much wider area seems to change or brighten well before the GOES X-ray flux starts to increase. This event may account for a slow wimpy CME seen in NW around 22 UT.
Detected by halocme, Submitted at 2015-05-11T20:16:00
2014-03-03T15:30:35 --> 2014-03-03T16:29:59
This M1.2 flare consists mainly of a pair of ribbons, but a much wider area seems to change or brighten well before the GOES X-ray flux starts to increase. This event may account for a slow wimpy CME seen in NW around 22 UT.
Detected by halocme, Submitted at 2015-05-11T20:15:45
2014-03-05T13:10:11 --> 2014-03-05T14:40:11
Same as before. On a second day.
Detected by halocme, Submitted at 2015-05-11T20:13:40
2014-03-04T18:00:03 --> 2014-03-04T20:00:03
The wave is seen to propagate over the north pole.
Detected by halocme, Submitted at 2015-05-11T20:16:52
2014-03-04T23:00:03 --> 2014-03-05T03:00:03
The limb region repeatedly emitted material in narrow channels. The neighboring region also started similar activity, although it is not clear whether it was triggered by the limb region.
Detected by halocme, Submitted at 2015-05-11T20:16:24
2014-03-04T20:35:23 --> 2014-03-04T22:25:47
This eruption starts at a region without spots, but it produces two-ribbon emission and a post-eruption arcade.
Detected by halocme, Submitted at 2015-05-11T20:16:00
2014-03-04T20:08:23 --> 2014-03-04T21:50:23
The outflow over the limb signify an eruption from the far side that was contemporaneous with another eruption on the east limb.
Detected by halocme, Submitted at 2015-05-11T20:16:36
2014-03-04T17:35:23 --> 2014-03-04T19:16:11
This eruption seems to preceded by downflows in the surrouding area. The expansion of the core field is seen in all the three channels in this movie. The event is associated with a gradual C5.5 flare.
Detected by halocme, Submitted at 2015-05-11T20:15:59
2014-03-04T17:35:23 --> 2014-03-04T19:16:11
This eruption seems to preceded by downflows in the surrouding area. The expansion of the core field is seen in all the three channels in this movie. The event is associated with a gradual C5.5 flare.
Detected by halocme, Submitted at 2015-05-11T20:13:33
2014-03-04T10:50:23 --> 2014-03-04T12:20:23
This appears to be triggered by foot-point dynamics possibly flux emergence, reminiscent of the prevalent model of coronal jets. But the coronal response seems to be broader than what is considered to be a jet.
Detected by halocme, Submitted at 2015-05-11T20:15:59
2014-03-04T03:10:11 --> 2014-03-04T04:10:11
This outflow or eruption is very diffuse, but it is seen to follow a cusp-like structure.
Detected by halocme, Submitted at 2015-05-11T20:15:58
2014-03-03T23:50:23 --> 2014-03-04T01:20:23
The ejection is seen in 304 A, 211 A and 171 A images in emission. The source region is likely to be occulted, and the closed structure on the limb is not affected by this ejection.
Detected by halocme, Submitted at 2015-05-11T20:13:32
2014-03-03T18:20:23 --> 2014-03-03T20:20:23
Collimated eruptions are seen for more than two hours. It is hard to know exactly when and how this activity started.
Detected by halocme, Submitted at 2015-05-11T20:16:48
2014-03-03T11:00:03 --> 2014-03-03T13:30:03
Coronal loops over an active region are seen to expand in a sequence. We note four steps in this movie. They do not reflect in GOES X-ray light curves.
