Recent Events Reported by Observers
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Detected by Tiago Pereira, Submitted at 2017-02-14T16:52:10
2017-02-11T13:46:17 --> 2017-02-11T14:08:22
Large coronal jet near the decaying AR12630.
Detected by Tiago Pereira, Submitted at 2017-02-14T16:49:57
2017-02-11T12:49:21 --> 2017-02-11T13:05:08
Large coronal jet on West limb, near the decaying AR12630.
Detected by Tiago Pereira, Submitted at 2017-02-14T16:43:21
2017-02-10T20:12:11 --> 2017-02-10T20:14:40
Small flaring region (ribbon?) see in AR12635.
Detected by Tiago Pereira, Submitted at 2017-02-14T11:35:19
2017-02-09T18:16:22 --> 2017-02-09T18:47:10
A wide jet coming off from an unnamed AR near West limb. AR very bright at the limb, and coronal rain also seen. Largest loops off the AR have a flat top.
Detected by gchintzo, Submitted at 2017-02-14T00:27:09
2017-02-12T12:00:09 --> 2017-02-13T16:00:09
A narrow, trans-equatorial coronal hole. Coronal holes are predominantly unipolar regions (here, green positive magnetic field, red negative magnetic field). Note the significant amount of activity within the coronal hole, primarily at locations where 'parasitic' negative patches exist (red color). Each negative patch seems to be connected to a nearby positive patch; several of these ad-hoc bipoles seem to host mini-sigmoids in the corona, which some of those mini-sigmoids erupt/interact with neighboring ones.
Detected by gchintzo, Submitted at 2017-02-14T00:17:13
2017-02-11T00:00:09 --> 2017-02-11T23:50:09
A pair of North Hemisphere Active Regions (ARs) in close proximity. The ARs have their polarity orientation almost in parallel. Interesting connectivity arises in the corona - especially an "X-point"-like configuration of fieldilnes.
Detected by Tiago Pereira, Submitted at 2017-02-13T14:45:18
2017-02-10T10:02:39 --> 2017-02-10T11:07:58
Flux emergence is seen in AR12635, a young active region. (It was not named at time of planning.)
Detected by Tiago Pereira, Submitted at 2017-02-15T00:39:33
2017-02-10T07:28:45 --> 2017-02-10T07:49:13
Reconnection jet (inverse Y shaped) near leading spot of AR12635 (at the time of planning this AR was not named). Also occurs in similar place in previous raster.
Detected by Tiago Pereira, Submitted at 2017-02-15T00:39:34
2017-02-10T01:49:38 --> 2017-02-10T03:03:14
An unusual eruption (filament?) seem from AR12630 as it goes around the limb. Seen in all SJIs, plenty of swirling motions, some of the plasma falls back down as coronal rain, other gets projected and hangs around looking like prominence material that falls back down (see following OBS, taken after eclipse).
Detected by halocme, Submitted at 2017-02-12T00:29:11
2017-02-10T07:00:09 --> 2017-02-10T12:00:09
A very minor eruption. Not clear how high the filament reached.
Detected by halocme, Submitted at 2017-02-10T06:40:39
2017-02-10T02:30:01 --> 2017-02-10T03:00:01
A small filament erupted showing rotation (in 171 A), and disturbed the overlying corona to oscillate. Part of the corona stayed dimmed for 30-40 minutes (but no obvious CME).
Detected by halocme, Submitted at 2017-02-09T19:19:49
2017-02-07T16:00:09 --> 2017-02-07T20:00:09
Curious about what AIA saw while IRIS recorded "Small hot loops (Other)". In an extended field of view and temporal range, we indeed see a microflare + jet (17:55-18:10), which would be easily overlooked while hunting for big eruptions.
Detected by halocme, Submitted at 2017-02-09T19:40:39
2017-02-08T12:00:09 --> 2017-02-09T15:00:09
A new region with sunspots emerged north of AR 12634, which no longer shows spots. This may be promoted to AR 12635. It initially produced a few C-class flares, but may have already stabilized.
Detected by halocme, Submitted at 2017-02-09T18:16:52
2017-02-08T15:30:01 --> 2017-02-08T16:30:01
A small filament erupted from a quiescent region. Interestingly, the eruption was nearly cosincident with the earuption from behind the northwest limb. This was perhaps by chance.
Detected by halocme, Submitted at 2017-02-09T18:08:59
2017-02-08T15:30:01 --> 2017-02-08T16:30:01
This must have been from the backside since no eruptive signatures were noted on the visible side. A narrow CME was associated with this eruption. See the SEEDS CME catalog at http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170208.161208.w042.v0328.p297&frame=16&r.
Detected by Tiago Pereira, Submitted at 2017-02-09T16:25:12
2017-02-07T17:04:34 --> 2017-02-07T18:11:03
Small hot loops in AR12634, perhaps a microflare?
Detected by halocme, Submitted at 2017-02-08T07:59:16
2017-02-07T11:00:09 --> 2017-02-07T12:50:09
This occurred in the northern part of AR 12632, separate from but maybe affected by the earlier eruption in the southern part. The LASCO movie http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170207.100007.w035.v0346.p292&frame=13&r contains both eruptions.
Detected by halocme, Submitted at 2017-02-08T07:40:39
2017-02-07T07:40:13 --> 2017-02-07T10:40:13
This eruption started with tumbling motions of low-lying prominences. LASCO data do not clearly reveal a flux rope in the outflow (see http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170207.100007.w035.v0346.p292&frame=13&r), but it looks more like a CME than earlier events on Feb 5.
Detected by halocme, Submitted at 2017-02-08T07:40:39
2017-02-07T07:40:13 --> 2017-02-07T10:40:13
This eruption started with tumbling motions of low-lying prominences. LASCO data do not clearly reveal a flux rope in the outflow (see http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170207.100007.w035.v0346.p292&frame=13&r), but it looks more like a CME than earlier events on Feb 5.
Detected by halocme, Submitted at 2017-02-08T07:29:36
2017-02-06T04:00:09 --> 2017-02-06T05:00:09
The footpoint brightening occurred nearly simultaneously with an ejeciton that looked like a jet. Quick-look at the photospheric magnetograms indicates that the footpoint corresponds to cancellation rather than emergence.
