Recent Events Reported by Observers
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Detected by Paola Testa, Submitted at 2019-04-08T22:39:49
2019-04-04T11:05:09 --> 2019-04-04T11:25:08
Small transition region loops under the slit, providing high temporal resolution spectroscopic observations of the evolution of the loops.
Detected by Paola Testa, Submitted at 2019-04-08T22:37:13
2019-04-04T09:30:04 --> 2019-04-04T09:40:03
A jet in the coronal hole at South Pole is observed by IRIS and the higher portion of the jet is under the slit.
Detected by Paola Testa, Submitted at 2019-04-08T22:30:42
2019-04-04T07:29:14 --> 2019-04-04T08:04:48
Small transition region loops under the slit.
Detected by Paola Testa, Submitted at 2019-04-08T20:46:26
2019-04-02T18:00:16 --> 2019-04-02T18:12:00
Interesting eruption occurring in QS close to North Pole. The eruption is observed in several passbands (both IRIS and AIA).
Detected by Paola Testa, Submitted at 2019-04-08T20:32:26
2019-04-02T14:05:30 --> 2019-04-02T14:27:54
small jet detected in SP CH
Detected by Paola Testa, Submitted at 2019-04-08T20:10:49
2019-04-02T05:17:42 --> 2019-04-02T05:31:17
Peacock tail in trailing sunspot of AR 12737
Detected by gchintzo, Submitted at 2019-04-04T00:47:21
2019-03-30T00:00:09 --> 2019-04-03T14:00:09
The emergence of NOAA AR 12737 captured from its very beginning. This AR appears to be of a simple bipolar nature.
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
