Recent Events Reported by Observers
Previous NextDetected by halocme, Submitted at 2019-11-12T04:02:02
2019-10-30T12:45:01 --> 2019-10-30T13:30:37
Another example of a polar jet that seems to involve cool filament material.
Detected by halocme, Submitted at 2019-11-12T01:43:45
2019-10-29T14:55:13 --> 2019-10-29T15:55:13
This appears to involve a mini-filament.
Detected by halocme, Submitted at 2019-11-12T01:38:01
2019-10-28T03:10:13 --> 2019-10-28T05:00:37
A prominence is seen to erupt, reaching a certain height, but there is no sign at 211 A that the overlying corona is affected. This is likely a confined eruption, and indeed there was no CME.
Detected by halocme, Submitted at 2019-11-12T01:31:15
2019-10-27T18:25:13 --> 2019-10-27T20:06:01
This gives an impression that the eruption started above the bright loops. There was no associated CME.
Detected by halocme, Submitted at 2019-11-12T01:05:44
2019-10-26T11:40:13 --> 2019-10-26T13:10:13
We see two jets. Did the first one lead to the formation of a temporary mini-filament, which triggered the second jet?
Detected by halocme, Submitted at 2019-11-12T00:56:43
2019-10-26T09:30:01 --> 2019-10-26T10:40:49
This started as an ejection of cool material in helical motions and then followed large scale structures around what looked like a flux rope.
Detected by halocme, Submitted at 2019-11-11T22:09:42
2019-10-25T17:15:01 --> 2019-10-25T18:30:37
This event took place in a quiescent region at high latitude. The motion was highly non-radial. 304 A images indicate the presence of a small filament and cool material in the body of the jet.
Detected by halocme, Submitted at 2019-11-11T18:10:41
2019-10-24T15:35:25 --> 2019-10-24T16:45:01
This occurred in a quiescent region (no AR anyway). The trajectory seems to be affected by adjacent coronal structures.
Detected by gchintzo, Submitted at 2019-11-07T01:57:42
2019-11-06T01:40:09 --> 2019-11-06T21:00:09
A cavity on the north west limb expands and moves southward. Note a faint cavity from the same location that exhibits the same behavior.
Detected by gchintzo, Submitted at 2019-11-07T00:52:04
2019-11-02T00:00:09 --> 2019-11-04T19:00:09
This AR exhibits an inverse polarity orientation (as compared to the hemispheric rule). This fact, combined with the high latitude of this AR suggests that Cycle 25 has just started
Detected by Carolina Robustini, Submitted at 2019-10-31T16:14:43
2019-10-28T04:39:52 --> 2019-10-28T07:08:06
Prominence bubble occurring in a late stage prominence.
Detected by Carolina Robustini, Submitted at 2019-10-31T16:03:47
2019-10-28T14:08:48 --> 2019-10-28T17:20:42
Bubbles occurring in a later stage prominence
Detected by Krzysztof Barczynski, Submitted at 2019-10-16T22:54:44
2019-09-24T05:29:26 --> 2019-09-24T07:56:18
The filament is clearly observed in the Mg II h/k raster image. It is not visible in SJI images. The filament is located in the centre part of the raster image.
Detected by gchintzo, Submitted at 2019-10-16T17:38:05
2019-10-15T05:50:09 --> 2019-10-15T19:10:09
A coronal cavity seen rolling from high latitude to low latitude and dissipate in the east limb of the sun
Detected by Krzysztof Barczynski, Submitted at 2019-10-15T23:23:43
2019-09-27T13:34:37 --> 2019-09-27T13:50:41
The filament is clearly observed in the Mg II h/k raster image. It is not visible in SJI images. The filament is located in the centre part of the raster image.
Detected by Krzysztof Barczynski, Submitted at 2019-10-15T20:59:46
2019-09-27T15:05:37 --> 2019-09-27T15:21:41
The filament is clearly observed in the Mg II h/k raster image. It is not visible in SJI images. The filament is located in the centre part of the raster image.
Detected by Krzysztof Barczynski, Submitted at 2019-10-15T19:42:54
2019-09-29T14:09:45 --> 2019-09-29T17:04:11
The fast-evolving prominence is located at the SW limb. The bubble is in the central part of the SJI 2796 image. Several elongated and almost parallel to the limb features are above the bubble. The observation was coordinated with THEMIS.
Detected by Wei Liu, Submitted at 2019-10-13T21:18:54
2019-09-10T04:38:51 --> 2019-09-10T06:40:34
This off-limb prominence exhibits some interesting flow patterns, with tumbling/rotating dynamics.
Detected by Wei Liu, Submitted at 2019-10-13T21:12:04
2019-09-12T04:10:20 --> 2019-09-12T07:20:32
This off-limb prominence appeared and grew significantly in size over hours
Detected by Chunming Zhu, Submitted at 2019-10-13T01:59:32
2019-10-03T19:11:34 --> 2019-10-03T19:38:29
After being "quiet" for weeks, the Sun finally comes with a small active region.