Recent Events Reported by Observers
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Detected by halocme, Submitted at 2019-02-07T03:21:47
2019-01-30T05:40:14 --> 2019-01-30T06:59:26
The biggest flare from AR 12733. Like others in the series, the flare was not eruptive despite violent motions in the vicinity of the central flare area.
Detected by halocme, Submitted at 2019-02-07T03:17:06
2019-01-29T21:00:30 --> 2019-01-29T22:50:54
Violent motions were observed after the flare brightening, but not associated with a CME, a similar pattern to the previous C1.9 flare also from AR 12733.
Detected by halocme, Submitted at 2019-02-07T03:11:09
2019-01-29T09:50:26 --> 2019-01-29T11:00:02
Flare in AR 12733. Surge-like motions are noted, just after the flare brightening, but there was no indication that the ejected material reached the coronagraphic heights, such as ~2 Rs.
Detected by halocme, Submitted at 2019-02-07T03:06:23
2019-01-28T14:30:01 --> 2019-01-28T15:40:01
The outward motion of cool material, highly non-radial, propagated to high altitudes. It only resulted in a marginal jet. No type III bursts were associated.
Detected by halocme, Submitted at 2019-02-07T01:36:33
2019-01-27T15:50:25 --> 2019-01-27T16:50:25
This jet involves helical motions of cool material as seen in 304 A images. No type III radio burst is noted in Wind/WAVES data.
Detected by halocme, Submitted at 2019-02-06T23:07:05
2019-01-26T06:00:09 --> 2019-01-26T11:30:09
A diffuse eruption with cool prominence matrial underlying a flux-rope-like outward-moving feature seen only in 171 A images. No CME associated.
Detected by halocme, Submitted at 2019-02-06T22:52:24
2019-01-26T13:00:02 --> 2019-01-26T14:00:02
The largest X-ray flare since 2018 Feb 7. It was non-eruptive, even though signatures were seen that are often thought of as being related to eruptions, such as rising loops and high-temperature regions just above nthe bright flare loops. Flares in AR 12733 were generally non-eruptive.
Detected by gchintzo, Submitted at 2019-02-05T19:14:51
2019-02-04T00:00:09 --> 2019-02-05T15:00:09
A decaying active region of overall bipolar magnetic distribution. This AR is not catalogued by NOAA.
Detected by Chad Madsen, Submitted at 2019-01-31T21:04:17
2019-01-28T19:23:25 --> 2019-01-28T20:22:39
A small, thin, straight, stable prominence protruding from the northeast limb.
Detected by Chad Madsen, Submitted at 2019-01-31T21:01:10
2019-01-28T18:12:24 --> 2019-01-28T18:46:03
Running sunspot waves seen in the FUV SJI channels of IRIS. The ripple-like waves spread throughout the umbra and penumbra of the leading sunspot.
Detected by Chad Madsen, Submitted at 2019-01-31T16:20:03
2019-01-28T09:38:33 --> 2019-01-28T10:26:53
Small, compact brightenings indicative of UV bursts largely near the leading sunspot of AR12733. Also, there is a material flow towards the AR from a trailing network patch.
Detected by Chad Madsen, Submitted at 2019-01-31T16:13:38
2019-01-28T01:31:24 --> 2019-01-28T02:19:44
Small, compact brightenings indicative of UV bursts throughout AR12733.
Detected by Chad Madsen, Submitted at 2019-01-29T21:42:29
2019-01-27T20:57:40 --> 2019-01-27T21:14:57
A jet emanating from an oval-shaped brightening in between patches of plage on the right half of the field-of-view. The event begins with an extended phase of high intensity and then quickly dissipates as material appears exit toward the right edge of the field-of-view.
Detected by Chad Madsen, Submitted at 2019-01-29T21:34:54
2019-01-27T17:36:14 --> 2019-01-27T18:24:34
Small, compact brightenings indicative of UV bursts near the polarity inversion line of AR12733.
Detected by Chad Madsen, Submitted at 2019-01-29T21:28:28
2019-01-27T09:17:04 --> 2019-01-27T10:05:24
A small, compact brightening indicative of UV bursts near the polarity inversion line AR12733. There appears to be a small material flow emanating from a location adjacent to the burst.
Detected by Chad Madsen, Submitted at 2019-01-29T21:19:35
2019-01-26T06:04:16 --> 2019-01-26T06:33:34
Two compact brightenings in the network patches of a decayed plage region indicative of explosive events. One is located in the northernmost network patch and the other on the southernmost. The northern event is far brighter, larger, and longer lived than its southern counterpart; however, it does not cross the slit until late in its lifetime.
Detected by Chad Madsen, Submitted at 2019-01-29T20:58:09
2019-01-26T02:25:51 --> 2019-01-26T03:09:17
Small, round, compact brightenings indicative of UV bursts throughout AR12733.
Detected by Chad Madsen, Submitted at 2019-01-29T20:54:36
2019-01-25T21:44:04 --> 2019-01-25T22:32:24
A Non-GOES flare-like event in the leading sunspot cluster of AR12733. The event is accompanied by two dome-shaped eruptions of material.
Detected by Chad Madsen, Submitted at 2019-01-29T20:48:56
2019-01-25T18:18:12 --> 2019-01-25T19:19:30
Compact brightenings indicative of UV bursts throughout AR12733. Many of the potential bursts are coincident with microflares along nearby loops.
Detected by Chad Madsen, Submitted at 2019-01-29T20:44:28
2019-01-25T16:40:46 --> 2019-01-25T17:42:04
Compact brightenings indicative of UV bursts throughout AR12733.
