Recent Events Reported by Observers
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Detected by jinmeng, Submitted at 2016-06-03T19:59:27
2016-05-21T08:10:06 --> 2016-05-21T11:50:06
A small jet observed from AR 12546.
Detected by jinmeng, Submitted at 2016-06-02T22:47:34
2016-05-20T23:20:06 --> 2016-05-21T04:10:06
A large jet was observed from AR 12546. The jet leads to corona activities to the north and south of the active region through direct magnetic connections. The filament material associated with the jet failed to erupt.
Detected by jinmeng, Submitted at 2016-06-02T22:47:33
2016-05-20T23:20:06 --> 2016-05-21T04:10:06
A large jet was observed from AR 12546. The jet leads to corona activities to the north and south of the active region through direct magnetic connections. The filament material associated with the jet failed to erupt.
Detected by jinmeng, Submitted at 2016-06-02T22:34:40
2016-05-20T08:00:06 --> 2016-05-20T11:40:06
A flare occurred at AR 12546. The reonnection makes a filament unstable and erupts at last.
Detected by forecaster, Submitted at 2016-06-01T02:52:30
2016-05-30T04:00:06 --> 2016-05-30T08:45:06
Small C class flare in emerging flux region.
Detected by forecaster, Submitted at 2016-06-01T02:34:19
2016-03-31T00:00:06 --> 2016-03-31T02:00:06
Twisting filament eruption from the SW limb.
Detected by Mark Cheung, Submitted at 2016-05-22T22:34:06
2016-05-18T17:46:09 --> 2016-05-18T18:10:06
No NOAA-reported GOES flare associated with this event.
Detected by Mark Cheung, Submitted at 2016-05-22T22:18:01
2016-05-18T14:14:58 --> 2016-05-18T14:48:07
This event does not seem to be associated with a NOAA-reported GOES flare.
Detected by Mark Cheung, Submitted at 2016-05-22T22:17:35
2016-05-18T14:14:58 --> 2016-05-18T14:48:07
This event does not seem to be associated with a NOAA-reported GOES flare.
Detected by Mark Cheung, Submitted at 2016-05-22T22:09:48
2016-05-18T06:46:11 --> 2016-05-18T11:57:45
This population of spicules seems to be predominantly slanted to the south.
Detected by Mark Cheung, Submitted at 2016-05-22T22:07:48
2016-05-18T06:46:11 --> 2016-05-18T07:43:03
Large intermittent blue- and red-shifted features in Si IV, C II and Mg h & k spectra at a Y-shaped feature appearing in (the southern edge of FOVs) NUV and FUV slitjaw images.
Detected by Mark Cheung, Submitted at 2016-05-22T22:07:41
2016-05-18T06:46:11 --> 2016-05-18T07:43:03
Large intermittent blue- and red-shifted features in Si IV, C II and Mg h & k spectra at a Y-shaped feature appearing in (the southern edge of FOVs) NUV and FUV slitjaw images.
Detected by Mark Cheung, Submitted at 2016-05-22T21:52:26
2016-05-18T05:06:41 --> 2016-05-18T05:23:16
Perhaps a jet resulting from reconnection through a null point or separator above a magnetic dome.
Detected by Mark Cheung, Submitted at 2016-05-22T21:41:53
2016-05-18T01:09:23 --> 2016-05-18T03:55:01
Type II spicules incessantly generated in a coronal hole at the south pole
Detected by Mark Cheung, Submitted at 2016-05-22T21:26:45
2016-05-17T20:01:30 --> 2016-05-17T20:21:40
This compact flare has a two-ribbon structure in the SJI 1330, 1400 and 2976 channels.
Detected by Mark Cheung, Submitted at 2016-05-22T21:19:31
2016-05-17T17:06:22 --> 2016-05-17T23:48:54
Transition region loops (SJI 1330 and 1400) that are seemingly pinched at the sites of converging photospheric flows (as seen in SJI 2832 sequences) suggest resistive flux emergence is taking place. The magnetic reconnection / cancellation taking place at and above the convergence sites create longer loops that straddle multiple flow cells. The convergence sites are also locations of enhanced emission in the SJI 1330, 1400 and 2796 channels (i.e. UV burst or bombs).
Detected by Mark Cheung, Submitted at 2016-06-27T19:26:06
2016-05-17T17:06:22 --> 2016-05-17T23:48:54
Transition region loops (SJI 1330 and 1400) that are seemingly pinched at the sites of converging photospheric flows (as seen in SJI 2832 sequences) suggest resistive flux emergence is taking place. The magnetic reconnection / cancellation taking place at and above the convergence sites create longer loops that straddle multiple flow cells. The convergence sites are also locations of enhanced emission in the SJI 1330, 1400 and 2796 channels (i.e. UV burst or bombs).
Detected by Mark Cheung, Submitted at 2016-05-22T20:56:33
2016-05-17T12:42:34 --> 2016-05-17T15:38:20
Transition region loops (SJI 1330 and 1400) that are seemingly pinched at the sites of converging photospheric flows (as seen in SJI 2832 sequences) suggest resistive flux emergence is taking place. The magnetic reconnection / cancellation taking place at and above the convergence sites create longer loops that straddle multiple flow cells. The convergence sites are also locations of enhanced emission in the SJI 1330, 1400 and 2796 channels (i.e. UV burst or bombs).
Detected by Mark Cheung, Submitted at 2016-06-27T19:26:06
2016-05-17T12:42:34 --> 2016-05-17T15:38:20
Transition region loops (SJI 1330 and 1400) that are seemingly pinched at the sites of converging photospheric flows (as seen in SJI 2832 sequences) suggest resistive flux emergence is taking place. The magnetic reconnection / cancellation taking place at and above the convergence sites create longer loops that straddle multiple flow cells. The convergence sites are also locations of enhanced emission in the SJI 1330, 1400 and 2796 channels (i.e. UV burst or bombs).
Detected by Mark Cheung, Submitted at 2016-05-22T20:49:51
2016-05-17T05:32:58 --> 2016-05-17T06:07:14
Transition region loops (SJI 1330 and 1400) that are seemingly pinched at the sites of converging photospheric flows (as seen in SJI 2832 sequences) suggest resistive flux emergence is taking place. The magnetic reconnection / cancellation taking place at and above the convergence sites create longer loops that straddle multiple flow cells. The convergence sites are also locations of enhanced emission in the SJI 1330, 1400 and 2796 channels (i.e. UV burst or bombs).
