Recent Events Reported by Observers
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Detected by Sean Brannon, Submitted at 2019-06-21T20:02:51
2019-05-08T19:03:19 --> 2019-05-08T19:30:30
Spectrograph slit catches eruption from north side of sunspot in AR 12740. Some loop draining (coronal rain) possible.
Detected by Sean Brannon, Submitted at 2019-06-21T19:58:11
2019-05-07T13:03:05 --> 2019-05-07T13:41:59
Spectrograph slit catches eruption on west side of sunspot in AR 12740.
Detected by Sean Brannon, Submitted at 2019-06-21T19:52:33
2019-05-07T07:29:24 --> 2019-05-07T12:04:10
Sunspot waves appear like ripples in a pond in this observation of AR 12740
Detected by Lijia Guo, Submitted at 2019-06-21T00:30:33
2019-06-04T09:43:58 --> 2019-06-04T10:17:24
A few quiet sun jets was captured by IRIS slit, their blue-shifted doppler components are visible in Si IV, C II and Mg II h&k.
Detected by Lijia Guo, Submitted at 2019-06-21T00:15:23
2019-06-04T06:55:42 --> 2019-06-04T07:03:39
A jet was captured by the rastering IRIS slit, both its footprint and part of the jet is covered, as one can see in the Si IV spectra.
Detected by Krzysztof Barczynski, Submitted at 2019-06-19T09:38:05
2019-06-18T04:19:11 --> 2019-06-18T05:23:21
Prominence bubble visible above the North-East limb is partially covered by the slit. IRIS observation presents the prominence in decaying phase. The prominence does not evolve much during the observation.
Detected by Krzysztof Barczynski, Submitted at 2019-06-19T09:33:02
2019-06-18T04:19:11 --> 2019-06-18T05:23:21
Prominence bubble visible above the North-East limb is partially covered by the slit. IRIS observation presents the prominence in decaying phase. The prominence does not evolve much during the observation.
Detected by Jacob Parker, Submitted at 2019-06-14T22:20:42
2019-06-02T00:44:01 --> 2019-06-02T00:58:44
Thanks to STEREO we were able to begin tracking this AR as soon as it came around the east limb. It was tracked via HOP 307 from limb to limb.
Detected by Jacob Parker, Submitted at 2019-06-14T21:59:13
2019-05-30T02:53:50 --> 2019-05-30T03:07:43
Both a prominence off the east limb and part of small filament were captured via a large dense raster. This OBS was run twice, each with a few repeats, throughout the day.
Detected by Jacob Parker, Submitted at 2019-06-14T21:42:21
2019-05-29T05:05:21 --> 2019-05-29T05:13:48
This small region of emerging flux came and went in a couple days and produced multiple explosive events.
Detected by halocme, Submitted at 2019-05-29T07:07:16
2019-05-25T21:15:01 --> 2019-05-25T23:01:01
The eruption occurred in what could be considered a coronal bright point (although it was largish). The area south of the region dimmed temporarily.
Detected by halocme, Submitted at 2019-05-29T07:00:57
2019-05-25T06:45:01 --> 2019-05-25T09:45:01
A slow, plasmoid- or flux-rope-like eruption was seen exclusively in 171 A images. The ejecta was seen to deflected toward the equator.
Detected by halocme, Submitted at 2019-05-29T06:55:34
2019-05-25T05:05:25 --> 2019-05-25T06:45:25
The eruption likely occurred on the backside. It appeared to trigger another one to the north on the visible side.
Detected by halocme, Submitted at 2019-05-29T06:49:16
2019-05-23T06:40:13 --> 2019-05-23T07:30:37
This jet contains cool material initially ejected in helical motions.
Detected by halocme, Submitted at 2019-05-29T06:42:57
2019-05-23T04:20:25 --> 2019-05-24T05:50:25
A bipolar region hosted what looked like a coronal bright point in full-disk images. It lasted a few days. Its appearance traced the evolution of the underlying magnetic field structure.
Detected by halocme, Submitted at 2019-05-29T06:29:45
2019-05-22T12:45:01 --> 2019-05-22T14:01:01
A tiny eruption, causing the overlying structure to slightly dim.
Detected by halocme, Submitted at 2019-05-29T06:24:57
2019-05-22T07:15:01 --> 2019-05-22T11:15:01
This eruption was very diffuse and seen only in 171 A images. An ourflow seemed to precede a more localized filament eruption, which accelerated the eruption of a closed coronal structure. The eruption was deflected clockwise.
Detected by halocme, Submitted at 2019-05-29T06:17:15
2019-05-21T06:45:01 --> 2019-05-21T09:01:01
The coronal structure overlying AR 12741 was seen to gradually open up and dim, even though eruption itself was not clearly seen. This was associated with a CME (http://spaceweather.gmu.edu/seeds/mkmovie_ql.php?cme=20190521.083607.w041.v0323.p248&frame=12).
Detected by halocme, Submitted at 2019-05-29T06:11:01
2019-05-21T04:00:09 --> 2019-05-21T06:10:09
Low-lying filament activity around AR 12741 seemed to cause a minor eruption, which did not go beyond the AIA field of view, hence no CME.
Detected by halocme, Submitted at 2019-05-29T05:58:30
2019-05-20T13:35:25 --> 2019-05-20T14:25:25
This looked like a narrow eruption, different from a flux rope eruption (CME), but it started impulsively, causing the overlying structure to oscillate.
