Recent Events Reported by Observers
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Detected by halocme, Submitted at 2018-03-02T01:37:05
2018-02-22T22:30:01 --> 2018-02-22T23:36:01
This is so diffuse that we need difference images to offset background emisson.
Detected by halocme, Submitted at 2018-03-02T01:25:44
2018-02-22T11:15:01 --> 2018-02-22T12:29:25
This is a very diffuse event. The jet was non-radial, toward the adjacent darker (lower-density) region.
Detected by halocme, Submitted at 2018-03-02T01:17:36
2018-02-21T16:10:13 --> 2018-02-21T17:10:13
The filament itself was hard to identify, but its eruption resulted in a two-ribbon flare that decayed quickly. The eruption looked like a jet, but it was not as narrow or collimated.
Detected by halocme, Submitted at 2018-03-02T01:05:22
2018-02-20T02:00:09 --> 2018-02-20T03:20:33
At least three jets are seen in this area and in thie interval. They are probably not connected.
Detected by halocme, Submitted at 2018-03-02T00:58:39
2018-02-19T13:50:25 --> 2018-02-19T17:00:01
Based on no footpoint brightening or post-eruption arcade, the source region of this eruption should be far behind the limb. The eruption is better seen at 171 A than at 211 A, including a linear structure after the corona opens up.
Detected by halocme, Submitted at 2018-03-02T00:50:54
2018-02-19T04:30:01 --> 2018-02-19T06:30:01
As the coronal structure "opens up" with the eruption that accompanies minor dimming, the adjacent structure to the north is seen to shrink.
Detected by halocme, Submitted at 2018-03-02T00:05:23
2018-02-18T12:15:01 --> 2018-02-18T13:05:25
Unwinding motions give an impression of a counterclockwise rotation. As the filament hit the overlying structure, it produced a jet-like eruption toward west.
Detected by Jacob Parker, Submitted at 2018-02-28T21:58:14
2018-02-22T09:21:43 --> 2018-02-22T09:53:25
An EE captured within a very small active region on a very very quiet sun.
Detected by Jacob Parker, Submitted at 2018-02-28T21:55:12
2018-02-24T00:09:04 --> 2018-02-24T01:59:13
This filament was observed as part of HOP345 w/ Hinode. Subsequent observation traced the filament across this disk.
Detected by Ted Tarbell, Submitted at 2018-02-28T00:55:45
2018-02-14T23:31:32 --> 2018-02-14T23:41:58
Nice spectra of ribbon and bi-directional jets
Detected by Ted Tarbell, Submitted at 2018-02-28T00:50:01
2018-02-15T21:38:16 --> 2018-02-15T21:38:16
High SNR spectra, full readout
Detected by Ted Tarbell, Submitted at 2018-02-28T00:39:40
2018-02-16T04:26:46 --> 2018-02-16T04:43:20
GOES B3, biggest from this AR in its last 5 days before rotating off
Detected by Ted Tarbell, Submitted at 2018-02-28T00:32:11
2018-02-17T02:04:21 --> 2018-02-17T02:19:53
Sit and stare, 60 sec exposures
Detected by Ted Tarbell, Submitted at 2018-02-28T00:29:49
2018-02-17T01:12:09 --> 2018-02-17T02:00:01
Big AR over W limb
Detected by Ted Tarbell, Submitted at 2018-02-28T00:23:11
2018-02-15T23:45:54 --> 2018-02-16T00:03:05
GOES B1.5 (haha)
Detected by Ted Tarbell, Submitted at 2018-02-28T00:19:40
2018-02-15T22:29:21 --> 2018-02-15T22:38:41
High SNR spectra, full readout, lossless compression, 60 sec exposure
Detected by Ted Tarbell, Submitted at 2018-02-27T23:59:25
2018-02-15T12:44:50 --> 2018-02-15T12:44:50
High SNR spectra, full readout (I think)
Detected by Gregal Vissers, Submitted at 2018-02-20T19:33:49
2018-01-29T04:46:34 --> 2018-01-29T04:59:28
UV bursts in network region, not crossed by the slit.
Detected by Gregal Vissers, Submitted at 2018-02-20T19:11:21
2018-01-28T05:46:18 --> 2018-01-28T06:10:51
Bright beads propagating along a curved trajectory between two network patches. The rastering slit catches (part of) one and tracks it for most of its visible lifetime.
Detected by Gregal Vissers, Submitted at 2018-02-20T19:05:40
2018-01-28T18:27:23 --> 2018-01-28T19:14:39
UV bursts in a network region, with the raster crossing the events once.
