Highest Rated Events (only 193 and 304 shown) All AR FE FL
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Detected by gchintzo, Submitted at 2019-03-11T21:26:43
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)
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Detected by gchintzo, Submitted at 2019-03-11T20:38:28
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.
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Detected by halocme, Submitted at 2019-03-05T07:14:28
2019-03-02T01:10:13 --> 2019-03-02T02:45:01
The eruption followed slow rising motions of closed loops. As a result, a post-eruption arcade formed underneath the eruption and tgemporary dimming was seen in the area to the east.
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Detected by halocme, Submitted at 2019-03-05T07:02:44
2019-03-01T01:15:01 --> 2019-03-01T02:21:01
The eruption started from an inverse-S-shaped structure, much smaller than typical active region sigmoids. It affected areas west and southeastern to its origin.
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Detected by halocme, Submitted at 2019-03-05T06:51:49
2019-02-28T01:50:25 --> 2019-02-28T04:50:25
The weak eruption appears to be suppressed by an overlying large-scale coronal structure.
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Detected by halocme, Submitted at 2019-03-05T05:08:32
2019-02-28T00:10:13 --> 2019-02-28T01:00:37
An eruption from a bright region, which was not large enough to be an active region. A small filament was involved. This had no coronagraphic consequences.
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Detected by halocme, Submitted at 2019-03-05T04:56:57
2019-02-27T15:50:25 --> 2019-02-27T20:00:25
This filament eruption occurred in a quiescent region. It is not clear what triggered it. But the CME-like closed loop structure was seen to move outward in two steps, more clearly in 171 A than 211 A. The related CME is http://spaceweather.gmu.edu/seeds/mkmovie_ql.php?cme=20190227.174807.w023.v0340.p260&frame=12.
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Detected by halocme, Submitted at 2019-03-05T01:40:48
2019-02-26T22:10:13 --> 2019-02-26T23:10:13
It is possible to find at least some jet-like collimated eruptions in polar coronal holes within, say, 10 minutes of time-lapse images, but this one was quite obvious. It is accompanied by the ejection of cool material and also followed by a smaller jet at a higher latitude.
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Detected by halocme, Submitted at 2019-03-05T01:20:52
2019-02-25T18:30:01 --> 2019-02-25T19:40:49
This is a very small eruption that only temporarily shows dimming (in 211 A) and elongated two-ribbon brightening.
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Detected by gchintzo, Submitted at 2019-02-18T23:23:53
2019-02-17T09:50:09 --> 2019-02-18T05:50:09
A filament in between the two dispersed magnetic polarities of a decaying active region. The filament is visible as a dark lane between the green and red patches (positive and negative magnetic polarities).
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Detected by gchintzo, Submitted at 2019-02-15T00:39:12
2019-02-12T12:00:09 --> 2019-02-13T16:40:09
An emerging flux region (unnamed by NOAA) near the southwest limb of the sun.
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Detected by gchintzo, Submitted at 2019-02-14T00:06:05
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.
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Detected by halocme, Submitted at 2019-02-08T01:39:00
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.
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Detected by halocme, Submitted at 2019-02-08T00:43:12
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).
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Detected by halocme, Submitted at 2019-02-08T00:25:13
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.
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Detected by halocme, Submitted at 2019-02-08T00:16:06
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.
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Detected by halocme, Submitted at 2019-02-07T03:39:10
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.
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Detected by halocme, Submitted at 2019-02-07T03:21:44
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.
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Detected by halocme, Submitted at 2019-02-07T03:17:02
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.
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Detected by halocme, Submitted at 2019-02-07T03:11:05
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.
