Recent Events Reported by Observers
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Detected by jinmeng, Submitted at 2016-05-11T18:03:24
2016-05-10T12:30:06 --> 2016-05-11T00:00:06
An eruption near the east limb. The loop oscillation due to the eruption is evident.
Detected by Hans Courrier, Submitted at 2016-05-11T18:02:18
2016-05-09T17:25:47 --> 2016-05-09T18:00:35
Mercury transit 9
Detected by Hans Courrier, Submitted at 2016-05-11T17:59:14
2016-05-09T18:20:27 --> 2016-05-09T18:43:33
Mercury transit 10
Detected by jinmeng, Submitted at 2016-05-11T17:59:41
2016-05-09T20:00:06 --> 2016-05-10T06:30:06
Sympathetic activities across the Sun, involving AR 12542, 12543, a filament eruption near the north pole, and a flux-emerging region SE of AR 12543.
Detected by jinmeng, Submitted at 2016-05-10T22:22:14
2016-05-09T10:10:06 --> 2016-05-09T20:10:06
Mecury Transit
Detected by jinmeng, Submitted at 2016-05-11T17:42:17
2016-05-09T03:00:06 --> 2016-05-09T10:10:06
An eruption from AR 12542.
Detected by Hans Courrier, Submitted at 2016-05-10T21:58:25
2016-05-05T09:32:23 --> 2016-05-05T09:38:31
Small bi-directional explosive event at edge of AR12541.
Detected by jinmeng, Submitted at 2016-05-10T21:33:41
2016-05-08T12:30:06 --> 2016-05-09T10:20:06
A filamant formation process observed near the north pole.
Detected by Nicole Schanche, Submitted at 2016-05-10T18:42:55
2016-03-27T16:32:48 --> 2016-03-27T16:58:34
This small B4.8 flare occurred as AR12524 approached the west limb. Material appears to be ejected and may have had a small CME associated with it. The slit misses the main flare event, but passes over the region immediately after.
Detected by Nicole Schanche, Submitted at 2016-07-05T18:38:23
2016-03-27T15:00:16 --> 2016-03-27T15:13:33
A small jet occurs just north of the sunspot of AR12524. The jet material moves non-radially and shows curvature as it extends outward. Toward the end, the material becomes more diffuse and no longer follows a linear path.
Detected by Nicole Schanche, Submitted at 2016-05-10T18:23:45
2016-03-22T19:24:13 --> 2016-03-22T22:07:32
There is a thin light bridge seen in both 1400 and 2796. This was from the trailing spot of AR12524. The slit misses the main light bridge, but does catch the top where the light bridge joins the penumbra.
Detected by halocme, Submitted at 2016-05-08T01:18:49
2016-05-07T15:20:22 --> 2016-05-07T18:00:22
It started to the northwest of AR 12542, producing brightenings at low altitudes (as seen in 304 A channel). The eruption was mostly toward north, perhaps channeled by the coronal hole sitting near disk center. See also https://twitter.com/halocme/status/729115888348102656.
Detected by halocme, Submitted at 2016-05-07T23:11:06
2016-05-07T13:50:22 --> 2016-05-07T14:40:22
There seem to be no changes on the visible disk, but coronal structures sticking out on the west limb seem to be dimmed or displaced, indicating an eruption on the backside. The associated CME was marginal, however.
Detected by halocme, Submitted at 2016-05-07T22:00:02
2016-05-07T12:35:22 --> 2016-05-07T13:55:22
A small loop system turned into an eruption. We hardly see the eruption in 304 A images, likely related to the only diffuse CME that resulted from the eruption. The waves associated with the eruption propagated preferentially northward (counterclockwise), leaving the adjacent prominence to oscillate.
Detected by halocme, Submitted at 2016-05-07T22:00:02
2016-05-07T12:35:22 --> 2016-05-07T13:55:22
A small loop system turned into an eruption. We hardly see the eruption in 304 A images, likely related to the only diffuse CME that resulted from the eruption. The waves associated with the eruption propagated preferentially northward (counterclockwise), leaving the adjacent prominence to oscillate.
Detected by halocme, Submitted at 2016-05-07T21:20:21
2016-05-06T15:10:10 --> 2016-05-06T16:30:10
There is slight indication of dimming due to a minor eruption on the backside. A very diffuse outflow is seen in LASCO images which may or may not be a CME.
Detected by halocme, Submitted at 2016-05-07T20:04:51
2016-05-05T20:20:22 --> 2016-05-05T22:50:22
The filament was sitting to the east of AR 12535, where the magnetic field was probably weak. Emission from both the flare ribbon and post-eruption arcade was waek. No clear CME was associated.
Detected by halocme, Submitted at 2016-05-07T19:42:32
2016-05-05T08:50:22 --> 2016-05-05T10:16:22
Although we hardly recognize an eruption, the presence of a marginal CME at a right time (http://cdaw.gsfc.nasa.gov/images/soho/lasco_ql/2016/05/05/20160505_103605_lasc2rdf_ql.png) may indicate that the opening up of the coronal structure around AR 12539 may represent an eruption. As we approach solar minimum, we may see more of these unimpressive and subtle eruptions.
Detected by halocme, Submitted at 2016-05-07T01:22:35
2016-05-04T22:40:10 --> 2016-05-04T23:40:10
The eruption itself does not look like reaching coronagraph heights, but it appears to impact adjacent structures probably underlying streamers. A LASCO frame that shows the associated CME is http://cdaw.gsfc.nasa.gov/images/soho/lasco_ql/2016/05/05/20160505_000005_lasc2rdf_ql.png.
Detected by halocme, Submitted at 2016-05-07T01:15:37
2016-05-04T18:35:22 --> 2016-05-04T20:59:22
This is a weak filament eruption, but post-eruption loops are clearly seen in EUV images (not reaching the GOES detection threshold).
