Recent Events Reported by Observers
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Detected by Chunming Zhu, Submitted at 2019-02-14T00:34:53
2019-02-09T07:16:00 --> 2019-02-09T08:12:14
There is a bubble located at the base of the prominence. Interestingly, a second bubble appears beside the previous one, and rises up into the prominence, and finally breaks.
Detected by Chunming Zhu, Submitted at 2019-02-14T00:24:21
2019-02-09T20:25:16 --> 2019-02-09T20:34:16
Part of the prominence appears to be twisting/untwisting, as suggested by the relative motions of the prominence materials. A slit of IRIS happens to scan that region and may provide more detailed information about the motions of the materials there.
Detected by Chunming Zhu, Submitted at 2019-02-14T00:12:37
2019-02-09T22:25:30 --> 2019-02-09T23:02:22
A dense and thick prominence extends high up into the solar corona. Based on the tracking of this prominence, what is shown here likely corresponds to the eastern leg of a large prominence.
Detected by gchintzo, Submitted at 2019-02-14T00:06:07
2019-02-08T00:00:09 --> 2019-02-09T16:30:09
A prominence bubble developing under a prominence seen in the northeast limb of the sun.
Detected by gchintzo, Submitted at 2019-02-14T00:03:20
2019-02-10T09:30:09 --> 2019-02-12T00:00:09
A coronal cavity in the northwest limb of the sun exhibiting rotational motions in its interior. It appears that material rises from lower heights and as it moves upwards within the cavity a sense of counterclockwise rotation occurs wirhin the cavity.
Detected by Chunming Zhu, Submitted at 2019-02-13T23:48:02
2019-02-07T03:28:40 --> 2019-02-07T03:57:57
Prominence is a bunch of dense and relatively cool ionized gases suspended in the solar corona. The video shown here is from IRIS observation. It displays both horizontal and vertical flows inside the prominence, implying the ongoing dynamic and complex processes there.
Detected by Chunming Zhu, Submitted at 2019-02-13T23:45:17
2019-02-07T03:28:40 --> 2019-02-07T03:57:57
Prominence is a bunch of dense and relatively cool ionized gases suspended in the solar corona. The video shown here is from IRIS observation. It displays both horizontal and vertical flows inside the prominence, implying the ongoing dynamic and complex processes there.
Detected by gchintzo, Submitted at 2019-02-08T01:59:47
2019-02-07T09:20:09 --> 2019-02-07T22:00:09
An on-disk filament (dark feature) is seen to extend past the solar limb as the sun rotates, essentially becoming a "prominence" (term used for filaments when they are appear to protrude past the solar limb). The filament/prominence is seen along its axis, making it appear as a radial structure. Note the swaying motions of the filament.
Detected by halocme, Submitted at 2019-02-08T01:45:43
2019-02-03T09:00:09 --> 2019-02-03T11:30:09
This was of backside origin. A diffuse but broad front is seen in 211 A images.
Detected by gchintzo, Submitted at 2019-02-08T01:45:31
2019-02-06T18:50:09 --> 2019-02-07T03:20:09
Two consecutive eruptions of minifilaments in the quiet sun from a very small area where magnetic fields cancel.
Detected by halocme, Submitted at 2019-02-08T01:39:05
2019-02-01T06:00:09 --> 2019-02-01T07:20:33
Another example of coronal rain observed by IRIS (e.g. http://www.lmsal.com/solarsoft/irisa/data/level2/2019/02/01/20190201_061304_3610108077/www/l2_20190201_061304_3610108077_SJI_1330_t000_fits_20190201_061304_j.html). This one outlines closed structures, seen in 171 A images in addition to 304 A images.
Detected by halocme, Submitted at 2019-02-08T00:43:18
2019-01-31T10:30:01 --> 2019-01-31T11:40:49
In 304 A images, we see the coronal rain against tall loops in 171 A. This is the same coronal rain observed by IRIS (e.g. http://www.lmsal.com/solarsoft/irisa/data/level2/2019/01/31/20190131_104409_3620108077/www/l2_20190131_104409_3620108077_SJI_1330_t000_fits_20190131_104409_j.html).
Detected by halocme, Submitted at 2019-02-08T00:25:16
2019-02-02T21:05:25 --> 2019-02-02T22:15:25
Three minor eruptions are noted in this movie. The northmost one was probably of backside origin. The associated small-scale brightenings are found on the disk for the other two eruptions.
Detected by halocme, Submitted at 2019-02-08T00:16:10
2019-02-01T06:20:25 --> 2019-02-01T07:30:25
An erupting "mini-filament" can be be traced in the low part of the jet.
Detected by Milan Gosic, Submitted at 2019-02-07T19:47:18
2019-02-03T16:29:53 --> 2019-02-03T17:41:05
QS/CH boundary observed for almost 11 hours on 2019/02/03. This observational sequence should coincide with the slit crossing the QS/CH boundary. There are 3 more observational runs before and after this sequence, covering QS, QS/CH boundary and CH.
Detected by Milan Gosic, Submitted at 2019-02-07T19:44:18
2019-02-02T16:09:00 --> 2019-02-02T17:20:12
QS/CH boundary observed for almost 11 hours. This observational sequence should coincide with the slit crossing the QS/CH boundary. There are 3 more observational runs before and after this sequence, covering QS, QS/CH boundary and CH.
Detected by Milan Gosic, Submitted at 2019-02-07T19:38:09
2019-02-01T06:24:52 --> 2019-02-01T07:01:43
Coronal rain along coronal loops above AR 12733 on the west limb. It happened after a microflare. The event is covered by the slit.
Detected by Milan Gosic, Submitted at 2019-02-07T19:29:32
2019-01-31T10:44:18 --> 2019-01-31T11:32:38
Coronal rain above AR 12733 on the west limb, covered by the slit.
Detected by Milan Gosic, Submitted at 2019-02-07T19:24:45
2019-01-31T09:18:38 --> 2019-01-31T09:54:07
Two spray surges on the west limb, covered by the slit (AR 12733).
Detected by halocme, Submitted at 2019-02-07T03:39:13
2019-01-31T17:45:01 --> 2019-01-31T19:25:01
The eruption started at the southern periphery of a plage region. In STEREO-A EUVI images, the region was near the disk center, and the eruption looked like expanding loops.
