Recent Events Reported by Observers
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Detected by Roy Smart, Submitted at 2019-05-28T02:17:01
2019-01-16T10:33:18 --> 2019-01-16T10:40:55
Possible explosive event where slit crosses event
Detected by Roy Smart, Submitted at 2019-05-28T02:08:43
2019-01-16T04:24:31 --> 2019-01-16T04:40:51
A good candidate for an explosive event, a small region of enhanced intensity inside a plage/bright point region.
Detected by Roy Smart, Submitted at 2019-05-28T01:58:20
2019-01-15T21:24:14 --> 2019-01-15T21:36:48
Tiny loop brightening of flux system
Detected by Roy Smart, Submitted at 2019-05-28T01:41:48
2019-01-15T17:48:25 --> 2019-01-15T18:44:57
Small eruption associated with magnetic reconfiguration of bright point.
Detected by Roy Smart, Submitted at 2019-05-28T01:38:23
2019-01-15T16:10:59 --> 2019-01-15T17:15:54
Small peacock tail from bright point
Detected by Roy Smart, Submitted at 2019-05-28T01:36:05
2019-01-15T15:18:30 --> 2019-01-15T15:33:10
Short bright point eruption
Detected by Bart De Pontieu, Submitted at 2019-05-21T19:46:10
2019-05-18T03:11:34 --> 2019-05-18T03:17:38
Only caught the beginning
Detected by Bart De Pontieu, Submitted at 2019-05-21T19:21:36
2019-05-17T13:21:25 --> 2019-05-17T13:34:52
Extended eruption (?)
Detected by gchintzo, Submitted at 2019-05-18T00:34:13
2019-05-14T06:50:09 --> 2019-05-14T20:10:09
It appears that this eruption comes from the north part of the internal PIL of AR12740.
Detected by Bart De Pontieu, Submitted at 2019-05-17T19:02:03
2019-05-16T14:30:44 --> 2019-05-16T15:18:49
Nice evolution
Detected by Bart De Pontieu, Submitted at 2019-05-17T18:38:40
2019-05-16T07:03:41 --> 2019-05-16T07:11:32
in super penumbra
Detected by Bart De Pontieu, Submitted at 2019-05-17T18:29:21
2019-05-15T19:16:03 --> 2019-05-15T19:43:31
C2 flare
Detected by Bart De Pontieu, Submitted at 2019-05-17T18:25:39
2019-05-15T18:43:54 --> 2019-05-15T18:51:48
Coronal jet
Detected by Bart De Pontieu, Submitted at 2019-05-17T18:22:28
2019-05-15T16:28:15 --> 2019-05-15T17:30:13
B2 flare
Detected by Bart De Pontieu, Submitted at 2019-05-17T18:08:57
2019-05-14T17:54:03 --> 2019-05-14T18:20:21
Partial view of magnetic field reconfiguration that appears similar to a coronal jet
Detected by gchintzo, Submitted at 2019-05-14T18:48:13
2019-05-13T13:20:09 --> 2019-05-13T19:10:09
A non radial eruption in the neutral line between AR12741 and AR12740. A CME was observed by LASCO (253 km s-1 ; http://spaceweather.gmu.edu/seeds/mkmovie_ql.php?cme=20190513.171207.w012.v0253.p096&frame=14)
Detected by gchintzo, Submitted at 2019-05-14T18:43:12
2019-05-12T17:40:09 --> 2019-05-13T00:00:09
Eruption from external Polarity Inversion Line of AR12741 and AR12740. This was associated with a halo CME seen in LASCO observations (375 km s-1; http://spaceweather.gmu.edu/seeds/monthly.php?a=2019&b=05)
Detected by gchintzo, Submitted at 2019-05-14T18:35:34
2019-05-10T17:30:09 --> 2019-05-11T05:00:09
A failed eruption in the core of AR12740 and a successful eruption coming from a much wider area off the north of AR12740. A slow faint halo CME was seen in LASCO data (174 km s-1; http://spaceweather.gmu.edu/seeds/mkmovie_ql.php?cme=20190511.034807.w021.v0174.p293&frame=15)
Detected by gchintzo, Submitted at 2019-05-14T18:27:03
2019-05-09T04:00:09 --> 2019-05-09T09:30:09
A confined eruption in the core of AR12740. A shock bubble is seen following the eruption. No ejection was seen in LASCO coronagraphic observations.
Detected by gchintzo, Submitted at 2019-05-13T18:24:03
2019-05-08T00:00:09 --> 2019-05-08T06:00:09
A non-radial eruption in the south part of NOAA AR12741. Plane of the sky CME speed in LASCO is 968 km s-1 (http://spaceweather.gmu.edu/seeds/mkmovie_ql.php?cme=20190508.043607.w055.v0968.p098&frame=4)
