Recent Events Reported by Observers
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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.
Detected by halocme, Submitted at 2017-09-14T08:13:33
2017-09-12T13:45:01 --> 2017-09-12T14:45:01
The eruption from AR 12677 accompanied waves moving into the solar disk.
Detected by halocme, Submitted at 2017-09-14T08:13:33
2017-09-12T13:45:01 --> 2017-09-12T14:45:01
The eruption from AR 12677 accompanied waves moving into the solar disk.
Detected by halocme, Submitted at 2017-09-14T08:06:08
2017-09-12T07:15:01 --> 2017-09-12T08:05:25
The flare occurred in AR 12680. The wave was driven mostly southward.
Detected by halocme, Submitted at 2017-09-14T08:41:24
2017-09-10T15:30:01 --> 2017-09-10T16:50:25
The flare was probably stronger than X8.2 because AR 12673 was slightly behind the limb. The coronal wave appeared to be the widest, covering the entire surface. The associated CME was super fast (3000-3500 km/s), and resulting in quick onset of a big SEP event, possibly a GLE.
Detected by halocme, Submitted at 2017-09-14T08:41:14
2017-09-10T15:30:01 --> 2017-09-10T16:50:25
The flare was probably stronger than X8.2 because AR 12673 was slightly behind the limb. The coronal wave appeared to be the widest, covering the entire surface. The associated CME was super fast (3000-3500 km/s), and resulting in quick onset of a big SEP event, possibly a GLE.
Detected by halocme, Submitted at 2017-09-14T07:47:24
2017-09-09T22:00:09 --> 2017-09-09T23:30:09
The eruption was mostly radial but lateral expansion drove a wave mostly counterclockwise. A fat CME was associated (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170909.233608.w070.v0739.p283&frame=5&r).
Detected by halocme, Submitted at 2017-09-14T07:47:24
2017-09-09T22:00:09 --> 2017-09-09T23:30:09
The eruption was mostly radial but lateral expansion drove a wave mostly counterclockwise. A fat CME was associated (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170909.233608.w070.v0739.p283&frame=5&r).
Detected by halocme, Submitted at 2017-09-14T07:41:27
2017-09-07T17:20:25 --> 2017-09-07T19:10:49
This coronal wave seems to be originated over the limb, not closely related to C-class flares in AR 12673.
Detected by halocme, Submitted at 2017-09-14T07:41:14
2017-09-07T17:20:25 --> 2017-09-07T19:10:49
This coronal wave seems to be originated over the limb, not closely related to C-class flares in AR 12673.
Detected by halocme, Submitted at 2017-09-14T07:41:27
2017-09-07T14:20:25 --> 2017-09-07T15:30:01
An eruption was mostly in the radial direction, and the associated wave on the disk was diffuse. The associated CME was not broad (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170907.153636.w043.v0334.p248&frame=13&r).
Detected by halocme, Submitted at 2017-09-14T07:41:13
2017-09-07T14:20:25 --> 2017-09-07T15:30:01
An eruption was mostly in the radial direction, and the associated wave on the disk was diffuse. The associated CME was not broad (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170907.153636.w043.v0334.p248&frame=13&r).
Detected by halocme, Submitted at 2017-09-14T07:13:24
2017-09-06T08:40:13 --> 2017-09-06T10:30:37
There are some motions related to the flare and even small dimming, but overall it is a non-eruptive event and may the coronalgraph features (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170906.083607.w025.v0224.p260&frame=7&r) may not represent a real CME or related to this flare.
Detected by halocme, Submitted at 2017-09-14T07:08:23
2017-09-06T11:40:17 --> 2017-09-06T13:29:29
This is the largest flare in solar cycle 24. The last flare with a similar magnitude (X9.0) occurred on 5 December 2006. It occurred impulsively in AR 12673, producing global waves. The associated halo CME is fast (maybe too fast to be measured in http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170906.122407.w155.v0582.p243&frame=7&r).
