Recent Events Reported by Observers
Previous Next
Detected by Sean Brannon, Submitted at 2018-03-06T17:24:45
2017-07-07T08:07:22 --> 2017-07-07T09:18:12
Several bright flashes in loops in AR 12665 shortly after it rotated over east limb.
Detected by Sean Brannon, Submitted at 2018-03-06T17:15:57
2017-07-07T05:20:05 --> 2017-07-07T07:39:08
IRIS catches AR 12665 as it rotates over the east limb. Catches several small B-flares, loop brightenings, coronal rain, and a sunspot on the leading side.
Detected by Sean Brannon, Submitted at 2018-03-06T17:10:39
2017-07-06T21:20:51 --> 2017-07-06T22:02:14
Slit just caught a small jet or loop activation.
Detected by Sean Brannon, Submitted at 2018-03-06T17:03:57
2017-07-06T04:20:42 --> 2017-07-06T07:25:14
HOP 269 IRIS only catches a prominence on the west limb for entire observation.
Detected by Sean Brannon, Submitted at 2018-03-06T16:50:45
2017-12-01T18:50:46 --> 2017-12-01T19:11:39
Slit covers bright point in southern coronal hole, one significant brightening during observation may indicate small jet and/or explosive event.
Detected by Sean Brannon, Submitted at 2018-03-06T16:46:23
2017-11-28T17:25:31 --> 2017-11-28T18:02:47
Slit covers bright point in southern coronal hole, several brightenings during observation may indicate small jets and/or explosive events.
Detected by halocme, Submitted at 2018-03-03T01:52:15
2018-03-02T10:20:25 --> 2018-03-02T12:00:01
This one is eruptive, but the global impact may be smaller than the B6.8 flare around 00:30 UT.
Detected by halocme, Submitted at 2018-03-03T01:52:14
2018-03-02T10:20:25 --> 2018-03-02T12:00:01
This one is eruptive, but the global impact may be smaller than the B6.8 flare around 00:30 UT.
Detected by halocme, Submitted at 2018-03-03T01:52:13
2018-03-02T10:20:25 --> 2018-03-02T12:00:01
This one is eruptive, but the global impact may be smaller than the B6.8 flare around 00:30 UT.
Detected by halocme, Submitted at 2018-03-03T01:52:12
2018-03-02T10:20:25 --> 2018-03-02T12:00:01
This one is eruptive, but the global impact may be smaller than the B6.8 flare around 00:30 UT.
Detected by halocme, Submitted at 2018-03-03T01:48:04
2018-03-02T05:00:09 --> 2018-03-02T06:00:09
Looks quite dynamic, but no eruption or other related phenomena.
Detected by halocme, Submitted at 2018-03-03T01:45:01
2018-03-02T00:00:09 --> 2018-03-02T02:00:09
AR 12770 had been dormant until late 1 March 2018, when it started to produce four flares above B1. This one was the most eruptive with relatively long duration soft X-rays. It was accompanied by coronal dimming and global waves.
Detected by halocme, Submitted at 2018-03-03T01:45:02
2018-03-02T00:00:09 --> 2018-03-02T02:00:09
AR 12770 had been dormant until late 1 March 2018, when it started to produce four flares above B1. This one was the most eruptive with relatively long duration soft X-rays. It was accompanied by coronal dimming and global waves.
Detected by halocme, Submitted at 2018-03-03T01:45:00
2018-03-02T00:00:09 --> 2018-03-02T02:00:09
AR 12770 had been dormant until late 1 March 2018, when it started to produce four flares above B1. This one was the most eruptive with relatively long duration soft X-rays. It was accompanied by coronal dimming and global waves.
Detected by halocme, Submitted at 2018-03-03T01:44:59
2018-03-02T00:00:09 --> 2018-03-02T02:00:09
AR 12770 had been dormant until late 1 March 2018, when it started to produce four flares above B1. This one was the most eruptive with relatively long duration soft X-rays. It was accompanied by coronal dimming and global waves.
Detected by halocme, Submitted at 2018-03-02T03:06:43
2018-02-28T14:00:09 --> 2018-02-28T16:00:09
The eruption started in the western part of the active region, producing a long-duration B2.3 flare. It also accomanied twin coronal dimming (typical of a sigmoid eruption) and a large-scale coronal propagating front primarily to the south.
Detected by halocme, Submitted at 2018-03-02T03:06:42
2018-02-28T14:00:09 --> 2018-02-28T16:00:09
The eruption started in the western part of the active region, producing a long-duration B2.3 flare. It also accomanied twin coronal dimming (typical of a sigmoid eruption) and a large-scale coronal propagating front primarily to the south.
Detected by halocme, Submitted at 2018-03-02T03:06:42
2018-02-28T14:00:09 --> 2018-02-28T16:00:09
The eruption started in the western part of the active region, producing a long-duration B2.3 flare. It also accomanied twin coronal dimming (typical of a sigmoid eruption) and a large-scale coronal propagating front primarily to the south.
Detected by halocme, Submitted at 2018-03-02T03:06:41
2018-02-28T14:00:09 --> 2018-02-28T16:00:09
The eruption started in the western part of the active region, producing a long-duration B2.3 flare. It also accomanied twin coronal dimming (typical of a sigmoid eruption) and a large-scale coronal propagating front primarily to the south.
Detected by halocme, Submitted at 2018-03-02T02:56:59
2018-02-25T12:00:09 --> 2018-02-27T12:00:09
This AR got the NOAA number at 27 Feb 2018 00:00 UT. The maximum size was 30 msh on 27 Feb 2018 and the AR decayed immediately to 10 msh on 28 Feb onward. The most intense flare was B3.3 on 26 Feb.
