Recent Events Reported by Observers
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Detected by halocme, Submitted at 2018-07-08T00:31:14
2018-06-28T22:00:09 --> 2018-06-28T23:30:09
A marginal eruption seen only in 171 A images.
Detected by halocme, Submitted at 2018-07-08T00:27:39
2018-06-27T22:25:12 --> 2018-06-27T23:35:12
Minor eruption from a quiescent region just on the limb. The overlying coronal structure was slightly impacted.
Detected by halocme, Submitted at 2018-07-01T05:10:58
2018-06-30T16:00:09 --> 2018-06-30T21:00:09
Very diffuse eruption seen in 171 A images, but not in 211 A images. A narrow (23 deg) and slow (121 km/s) CME was found in LASCO C2 data (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20180630.191207.w023.v0121.p082&frame=18&r).
Detected by halocme, Submitted at 2018-07-01T00:21:47
2018-06-17T16:00:09 --> 2018-06-17T21:30:09
A rising prominence appears to interact with overlying field, letting a flux rope move out. This is seen exclusively in 171 A images, suggesting that no heating is brought about by magnetic reconnection.
Detected by halocme, Submitted at 2018-07-01T00:07:47
2018-06-16T08:50:25 --> 2018-06-16T10:00:01
This jet shows spreading footpoints, probably as a result of reconnection of a bipole with open field lines as suggested in a Shibata-type model.
Detected by halocme, Submitted at 2018-06-30T23:58:39
2018-06-14T23:40:13 --> 2018-06-15T01:59:25
In this time interval, each of two regions, east and west, produced two jets.
Detected by halocme, Submitted at 2018-06-30T23:36:48
2018-06-14T13:50:25 --> 2018-06-14T15:10:49
A collimated structure is seen ejected non-radially. The eruption of a small flux-rope-like structure seems to be responsible for the jet.
Detected by halocme, Submitted at 2018-06-30T23:28:23
2018-06-13T10:40:13 --> 2018-06-13T11:30:37
Small jet, but it cam be traced to the edge of the AIA field of view. It contains cool filament material.
Detected by halocme, Submitted at 2018-06-30T23:21:18
2018-06-12T05:30:01 --> 2018-06-12T06:40:49
Minor eruption launched non-radially.
Detected by halocme, Submitted at 2018-06-30T23:15:05
2018-06-13T20:00:09 --> 2018-06-15T02:00:09
A small prominence system slowly got activated with increasing vortex motions. Between 2 and 5 UT on June 14, the first eruption involved cool mass coming back to the southern leg, but the prominence finally took off around 14 UT, followed by a current sheet and a post eruption arcade.
Detected by halocme, Submitted at 2018-06-30T23:15:04
2018-06-13T20:00:09 --> 2018-06-15T02:00:09
A small prominence system slowly got activated with increasing vortex motions. Between 2 and 5 UT on June 14, the first eruption involved cool mass coming back to the southern leg, but the prominence finally took off around 14 UT, followed by a current sheet and a post eruption arcade.
Detected by gchintzo, Submitted at 2018-06-22T23:25:55
2018-06-21T00:00:09 --> 2018-06-21T02:30:09
A small filament eruption that failed (or is too weak) to become a CME in the newborn NOAA AR 12715. Material lifts impulsively but then falls back down as coronal rain.
Detected by Tiago Pereira, Submitted at 2018-06-22T07:25:00
2018-06-15T09:45:04 --> 2018-06-15T09:52:44
Small flare or brightening in AR 12713.
Detected by gchintzo, Submitted at 2018-06-20T18:14:53
2018-06-18T00:00:09 --> 2018-06-18T13:50:09
A high-lying cavity-like structure moving upwards over the course of 3-4 hours. At around that time and for hours afterwards, SOHO/LASCO observed a gradual, slow streamer blowout http://spaceweather.gmu.edu/seeds/dailymkmovie.php?cme=20180619&r
Detected by gchintzo, Submitted at 2018-06-20T17:57:27
2018-06-18T00:00:09 --> 2018-06-19T14:10:09
NOAA AR12713 as it transits the central part of the solar disk. This AR has emerged since it was in the back side of the sun and the decay process has already started, as it can be seen by the dispersed magnetic flux at the surface (red and green patches show negative and positive magnetic flux respectively).
Detected by jinmeng, Submitted at 2018-06-20T17:55:51
2018-06-08T20:20:09 --> 2018-06-09T07:50:09
Large-scale filament eruption near the northern coronal hole.
Detected by gchintzo, Submitted at 2018-06-20T17:51:04
2018-06-18T00:00:09 --> 2018-06-19T18:00:09
Another emerging flux region in the north west quadrant of the solar disk. Note the increasing tilt of this emerging active region's loops towards the north and the south of the neutral line. Also note the dynamics associated with the interaction of the expanding loop systems in the corona.
Detected by jinmeng, Submitted at 2018-06-20T17:48:57
2018-06-11T08:59:45 --> 2018-06-11T15:09:21
Two small eruptions close in time and location were observed. There are also some synchronous activities between the two source regions (e.g., dimmings).
Detected by jinmeng, Submitted at 2018-06-20T17:48:57
2018-06-11T08:59:45 --> 2018-06-11T15:09:21
Two small eruptions close in time and location were observed. There are also some synchronous activities between the two source regions (e.g., dimmings).
Detected by gchintzo, Submitted at 2018-06-20T17:44:17
2018-06-18T00:00:09 --> 2018-06-20T14:00:09
A bipole is seen to emerge in the north hemisphere of the sun. Interesting connectivity develops between the emerging flux and the nearby quiet sun.
