Recent Events Reported by Observers
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Detected by cheung, Submitted at 2015-06-26T22:58:23
2015-06-22T18:03:15 --> 2015-06-22T18:34:27
The fast mode wave is driven by the eruption that caused the M6.5 flare.
Detected by cheung, Submitted at 2015-06-26T22:58:22
2015-06-22T18:03:15 --> 2015-06-22T18:34:27
The fast mode wave is driven by the eruption that caused the M6.5 flare.
Detected by cheung, Submitted at 2015-06-26T22:28:51
2015-06-26T00:00:03 --> 2015-06-26T19:10:03
Coronal rain persistently condenses at a boundary layer that may represent a QSL between magnetic flux domains.
Detected by cheung, Submitted at 2015-06-26T22:28:50
2015-06-26T00:00:03 --> 2015-06-26T19:10:03
Coronal rain persistently condenses at a boundary layer that may represent a QSL between magnetic flux domains.
Detected by weiliu, Submitted at 2015-06-22T23:44:32
2015-06-22T17:00:03 --> 2015-06-22T19:30:03
An M6.5 flare today was associated with a halo CME and global EUV wave.
Detected by weiliu, Submitted at 2015-06-22T23:44:32
2015-06-22T17:00:03 --> 2015-06-22T19:30:03
An M6.5 flare today was associated with a halo CME and global EUV wave.
Detected by halocme, Submitted at 2015-06-19T17:04:26
2015-06-19T03:00:03 --> 2015-06-19T09:00:03
The eruption took place without a clear filament, which is often seen as a marker, or a flare in GOES X-ray curves. This type of eruption would be very hard to forecast, even though it can be geo-effective (let's see what happens on June 21-22).
Detected by halocme, Submitted at 2015-06-19T06:34:47
2015-06-18T16:30:35 --> 2015-06-18T17:40:11
Although the GOES X-ray light curves have a data gap in the early phase, this event seems to have a relatively weak impulsive phase and the usual large-scale coronal propagating front due to lateral expansion is weak. But the eruption itself is powerful, resulting in a full halo CME. Moreover, oscillatory behavior is extensively seen, including the pattern that is reminiscent of fast wave trains.
Detected by halocme, Submitted at 2015-06-19T06:34:47
2015-06-18T16:30:35 --> 2015-06-18T17:40:11
Although the GOES X-ray light curves have a data gap in the early phase, this event seems to have a relatively weak impulsive phase and the usual large-scale coronal propagating front due to lateral expansion is weak. But the eruption itself is powerful, resulting in a full halo CME. Moreover, oscillatory behavior is extensively seen, including the pattern that is reminiscent of fast wave trains.
Detected by halocme, Submitted at 2015-06-19T06:34:46
2015-06-18T16:30:35 --> 2015-06-18T17:40:11
Although the GOES X-ray light curves have a data gap in the early phase, this event seems to have a relatively weak impulsive phase and the usual large-scale coronal propagating front due to lateral expansion is weak. But the eruption itself is powerful, resulting in a full halo CME. Moreover, oscillatory behavior is extensively seen, including the pattern that is reminiscent of fast wave trains.
Detected by halocme, Submitted at 2015-06-19T06:05:59
2015-06-18T00:10:11 --> 2015-06-18T01:59:23
Beautiful eruption showing helical motions in two steps. From above, the mtion appears to be clockwise. At higher temperatures, there was a supra arcade dwonflow (SAD).
Detected by halocme, Submitted at 2015-06-19T05:53:47
2015-06-17T12:40:11 --> 2015-06-17T16:01:11
The corona above AR 12371 dynamically transforms, including the prominence barely seen in 304 A channel. At this stage the system still stays unerupted.
Detected by schryver, Submitted at 2015-06-16T23:23:01
2015-06-16T00:00:03 --> 2015-06-16T20:00:03
Flux (continuing to) emerge near the E limb reaches into a largely unipolar area of QS leading the region, causing a daisy-like loop ensemble. Pretty and quite unusual.
Detected by schryver, Submitted at 2015-06-16T23:17:19
2015-06-15T00:00:03 --> 2015-06-15T13:48:03
Emerging flux just behind the E limb, giving an excellent side multithermal view of evolving loops, including some flaring.
Detected by schryver, Submitted at 2015-06-16T23:07:59
2015-06-14T04:48:03 --> 2015-06-14T11:08:03
A QS filament, extending to over the NE limb, rises, first over the limb, then 'unzipping' on the disk, followed by material flowing down and brightening (heating?) as it impacts the lower atmosphere, with late fleeting brightenings in the outer parts of the field configuration.
Detected by schryver, Submitted at 2015-06-16T23:00:13
2015-06-14T00:00:03 --> 2015-06-14T08:20:03
Eruption from a magnetically complex region, with 'ribbons', and interaction with a QS filament towards the south
Detected by halocme, Submitted at 2015-06-08T05:41:14
2015-06-05T17:15:00 --> 2015-06-05T17:55:00
This C3.5 flare was the largest during 5-7 June 2015. Some dynamic processes appear to be at work, but they may not contribute to an eruption due largely to the strong overlying field.
Detected by halocme, Submitted at 2015-06-08T05:34:10
2015-06-07T06:00:03 --> 2015-06-07T07:00:03
See only in 304 A and marginally in 171 A images. Not clear how far behind the limb the source region was.
Detected by halocme, Submitted at 2015-06-08T05:28:16
2015-06-07T10:00:03 --> 2015-06-07T11:40:03
This minor eruption was seen between the domains of loops connecting within AR 12360 and of those connecting AR 12360 and 12361.
Detected by halocme, Submitted at 2015-06-08T05:19:42
2015-06-06T22:20:23 --> 2015-06-06T23:20:23
Compact C2.2 flare in AR 12364 impacting the overlying corona.
