Recent Events Reported by Observers
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Detected by halocme, Submitted at 2017-08-28T05:14:35
2017-08-21T15:00:09 --> 2017-08-21T19:00:09
Around the time of Eclipse2017, there was actually an unimpressive CME (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170821.160010.w037.v0191.p096&frame=17&r). STEREO-A EUVI images show a slow filament eruption behind the east limb. AIA images seem to marginally capture the post eruption arcade.
Detected by halocme, Submitted at 2017-08-28T05:41:36
2017-08-24T00:25:13 --> 2017-08-24T01:10:49
A minor eruption that accompanied the C3.0 flare in AR 12671 went primarily westward, whereas the coronal wave propagated southward. A secondary wave from the interaction of the eruption with the adjacent structure is seen off the limb. No CME was associated with this event.
Detected by halocme, Submitted at 2017-08-28T05:41:20
2017-08-24T00:25:13 --> 2017-08-24T01:10:49
A minor eruption that accompanied the C3.0 flare in AR 12671 went primarily westward, whereas the coronal wave propagated southward. A secondary wave from the interaction of the eruption with the adjacent structure is seen off the limb. No CME was associated with this event.
Detected by halocme, Submitted at 2017-08-28T00:44:37
2017-08-20T19:00:09 --> 2017-08-20T21:00:09
Another flare in AR 12672, which was similar to the earlier M1.1 event, in the sense that its eruptive action, mostly radial, left the loops above the AR oscillating.
Detected by halocme, Submitted at 2017-08-28T00:44:36
2017-08-20T19:00:09 --> 2017-08-20T21:00:09
Another flare in AR 12672, which was similar to the earlier M1.1 event, in the sense that its eruptive action, mostly radial, left the loops above the AR oscillating.
Detected by halocme, Submitted at 2017-08-28T00:35:41
2017-08-20T01:20:25 --> 2017-08-20T02:45:37
The flare occurred as AR 12672 rotated on to the visible disk. Its associated eruption was more radial than lateral (i.e. only a weak EUV wave). The loop osciollation was a notable feature of this flare.
Detected by halocme, Submitted at 2017-08-28T00:35:40
2017-08-20T01:20:25 --> 2017-08-20T02:45:37
The flare occurred as AR 12672 rotated on to the visible disk. Its associated eruption was more radial than lateral (i.e. only a weak EUV wave). The loop osciollation was a notable feature of this flare.
Detected by halocme, Submitted at 2017-08-28T00:41:17
2017-08-19T21:10:13 --> 2017-08-19T22:51:01
The flare in AR 12671 seemed to be triggered by a filament eruption toward north. The wave front formed as a result of the eruption and was limited to the northern direction.
Detected by halocme, Submitted at 2017-08-28T00:41:09
2017-08-19T21:10:13 --> 2017-08-19T22:51:01
The flare in AR 12671 seemed to be triggered by a filament eruption toward north. The wave front formed as a result of the eruption and was limited to the northern direction.
Detected by Patricia Jibben, Submitted at 2017-08-28T18:14:53
2017-08-21T20:07:41 --> 2017-08-21T20:08:48
IRIS observed two eclipses on 21 August 2017. This is the second one.
Detected by Patricia Jibben, Submitted at 2017-08-23T19:25:51
2017-08-21T16:16:39 --> 2017-08-21T16:17:10
Solar Eclipse.
Detected by Patricia Jibben, Submitted at 2017-08-23T19:14:41
2017-08-19T18:26:04 --> 2017-08-19T18:55:22
Peak of the flare at 18:13 UT.
Detected by Patricia Jibben, Submitted at 2017-08-23T19:02:22
2017-08-18T06:32:17 --> 2017-08-18T06:48:53
The IRIS slit barely touches the edge of this jet.
Detected by Patricia Jibben, Submitted at 2017-08-23T18:50:01
2017-08-18T01:59:07 --> 2017-08-18T02:16:20
This event does not have a corresponding GOES event id.
Detected by Patricia Jibben, Submitted at 2017-08-23T18:38:27
2017-08-17T20:54:04 --> 2017-08-17T21:19:16
This jet doesn't have a corresponding GOES event. The event initially looks like some loops activating but near the end of the event you can see the jet.
Detected by Patricia Jibben, Submitted at 2017-08-23T18:32:03
2017-08-16T21:14:48 --> 2017-08-16T21:33:15
The large number of small spots makes for interesting observations in 2832. But if you ignore the rapid sunspot evolution you'll see couple of other interesting features that appear between some bright plage. There are no spots nearby but a dark diffuse feature appears along with several small bright beads rapidly moving east. This event has corresponding features in the other wavelengths. There is a smaller version of this happening nearby and seems it to be related to this event in the 2832.
Detected by Patricia Jibben, Submitted at 2017-08-23T18:03:44
2017-08-16T19:09:35 --> 2017-08-16T19:48:56
This active region is great for observing small flares and jets because there are several pores surrounding the two and later three main spots. This active region also undergoes rapid sunspot evolution and both flux emergence and flux cancellation are observed in 2832. In this observation sequence there is a B2.4 flare that is in the upper left FOV 19:45-19:54 UT. The slit does not cross this event and IRIS observed the flare for a few frames. A small reoccurring jet sits in the middle of the FOV and the slit crosses the event several times. The start and end times defined for this event are those for the jet and not the flare.
Detected by Patricia Jibben, Submitted at 2017-08-23T17:39:06
2017-08-16T01:33:32 --> 2017-08-16T02:33:11
There are two minor flares observed in 1400 and 1330. First, a B2.8 flare, peak time: 01:43 and then a B3.7 flare, peak time at 02:20 UT. In Mg II 2796, the flares have the bright base but the feature looks more like a surge along the flare trajectory.
Detected by halocme, Submitted at 2017-08-20T23:06:09
2017-08-04T01:20:25 --> 2017-08-04T06:50:25
Without enhancing the contrast, one can hardly see anything, but 171 A images seem to capture a slowly rising and then disconnected flux rope. No CME.
Detected by halocme, Submitted at 2017-08-20T22:58:14
2017-08-03T09:25:13 --> 2017-08-03T10:35:13
The eruption is so diffuse that one can hardly see it in intensity images. Difference images show it more clearly. A brightening suggests that the one leg of the erupting structure was on the visible side.
