Recent Events Reported by Observers
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Detected by halocme, Submitted at 2019-03-30T07:31:25
2019-03-29T14:00:09 --> 2019-03-29T15:09:45
Fast and narrow, but not so collimated, eruption from the backside. A low-lying prominence is seen to be disturbed, so the source region may not be too far behind the limb. A narrow but bright CME is associated (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20190329.162526.w031.v0489.p272&frame=10&r).
Detected by halocme, Submitted at 2019-03-30T07:20:36
2019-03-28T00:00:09 --> 2019-03-28T08:00:09
This gives an eruption that turbulent motions of a prominence system slowly let go the overlying structure seen in 171 A images. It is not clear what happened to the outward motions at greater heights - no CME.
Detected by halocme, Submitted at 2019-03-30T06:56:51
2019-03-27T01:30:01 --> 2019-03-27T06:00:01
This diffuse eruption started slowly without explosive behavior or producing clear post-eruption arcades. 171 A is the best wavelength to observe it at a greated distance, suggestive of the lack of hot material. The possibly associated CME is http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20190327.041207.w027.v0276.p251&frame=16&r.
Detected by halocme, Submitted at 2019-03-30T06:42:53
2019-03-26T13:15:01 --> 2019-03-26T15:01:01
Even though turbulent motions of a prominence preceded the eruption, it was probably triggered in a region slightly behind the limb. The associated CME is http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20190326.151211.w017.v0441.p282&frame=7&r.
Detected by halocme, Submitted at 2019-03-30T06:08:04
2019-03-25T13:20:25 --> 2019-03-25T14:40:49
This jet involves a cool helical structure seen in 304 A that delineates untwisting motions.
Detected by halocme, Submitted at 2019-03-30T06:02:33
2019-03-25T05:30:01 --> 2019-03-25T06:39:37
The eruption seems to trace a large-scale closed structure.
Detected by halocme, Submitted at 2019-03-30T05:51:27
2019-03-25T02:45:01 --> 2019-03-25T03:45:01
This jet seems to contain a closed structure and flux rope. The ejection is non-radial.
Detected by halocme, Submitted at 2019-03-30T04:40:21
2019-03-24T11:55:13 --> 2019-03-24T12:39:37
This looks like a typical jet. No magnetic field elements are found near the footpoint in HMI Blos data. Adjacent areas also show contemporaneous jet-like activities, which is not too common.
Detected by halocme, Submitted at 2019-03-30T04:33:43
2019-03-24T11:55:13 --> 2019-03-24T12:39:37
test. delete this.
Detected by Tiago Pereira, Submitted at 2019-03-27T16:48:08
2019-03-22T07:57:12 --> 2019-03-22T08:46:22
C2.8 flare on AR 12736
Detected by Tiago Pereira, Submitted at 2019-03-27T16:43:20
2019-03-22T05:06:17 --> 2019-03-22T05:35:26
C4.8 flare on AR 12736, or a sympathetic flare at the same time.
Detected by Tiago Pereira, Submitted at 2019-03-27T16:36:16
2019-03-22T10:14:18 --> 2019-03-22T10:22:29
Some parts of flare may be covered by the slit -- unclear because with the different exposures times between cameras, but some spectra appear very enhanced.
Detected by Tiago Pereira, Submitted at 2019-03-27T16:31:55
2019-03-22T01:56:40 --> 2019-03-22T02:30:55
B6.7 flare on AR 12736
Detected by Tiago Pereira, Submitted at 2019-05-14T14:29:30
2019-03-21T19:54:51 --> 2019-03-21T20:02:11
B8.8 flare on AR 12736
Detected by Tiago Pereira, Submitted at 2019-05-09T22:51:04
2019-03-21T17:13:46 --> 2019-03-21T17:35:58
Sympathetic flare, probably to the C2.6 flare that took place in the same AR 12737, more to the West.
Detected by Jakub Prchlik, Submitted at 2019-03-20T19:44:47
2019-03-16T04:49:23 --> 2019-03-16T06:13:19
IRIS tracked this northern QS filament for a few days prior. Previously, the filament was only visible in Mg II raster movies; however, now that the filament is on the limb one can see it in the 2796 SJI. You can also now clearly see dynamic north/south motions, which were hinted at in the raster observations.
Detected by Jakub Prchlik, Submitted at 2019-03-20T19:35:02
2019-03-13T00:13:38 --> 2019-03-13T00:55:14
IRIS observes an eruption just south of an extended and wispy prominence.
Detected by gchintzo, Submitted at 2019-03-11T21:32:18
2019-03-05T08:10:09 --> 2019-03-06T18:00:09
A decaying AR (unnamed by NOAA) in the south hemisphere of the sun. No significant activity (flares or CMEs) was produced by this region.
Detected by gchintzo, Submitted at 2019-03-11T21:26:48
2019-03-08T00:10:09 --> 2019-03-08T12:50:09
The moment of eruption in AR12734. A slow CME was launched (250 km/s; http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20190308.042816.w048.v0251.p289&frame=10&r)
Detected by gchintzo, Submitted at 2019-03-11T20:38:33
2019-03-04T16:20:09 --> 2019-03-07T06:40:09
An emerging flux region catalogued by NOAA as AR12734. Activity is seen in the east side of the emerging AR early on March 6 (no clear indication of ejection is seen in LASCO observations : http://spaceweather.gmu.edu/seeds/dailymkmovie.php?cme=20190306&r). At the end of the movie the moon is seen obstructing the field of view.
