Recent Events Reported by Observers
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Detected by halocme, Submitted at 2015-01-06T15:49:26
2013-07-26T21:20:23 --> 2013-07-26T23:00:23
This modest LCPF appears to be associated a filament eruption in a quiescent region, which also resulted in a C1.8 flare (its location from NOAA being AR 11800 is wrong).
Detected by halocme, Submitted at 2015-01-06T05:05:57
2014-09-08T23:00:03 --> 2014-09-09T01:10:03
This occurred in AR 12158. The wave-like motions were seen only at a large distance from the flare, but additional QFP-like features are seen closer.
Detected by halocme, Submitted at 2015-01-06T05:05:57
2014-09-08T23:00:03 --> 2014-09-09T01:10:03
This occurred in AR 12158. The wave-like motions were seen only at a large distance from the flare, but additional QFP-like features are seen closer.
Detected by halocme, Submitted at 2015-01-06T04:00:13
2014-09-01T21:20:23 --> 2014-09-01T22:50:23
The region was around S12 E114 at the time of the eruption. It is possible to trace the eruptjon to gradual ascention of closed loops. The lateral expansion was not as obvious as the previous event from AR 12158 at N14 E126.
Detected by halocme, Submitted at 2015-01-06T04:00:12
2014-09-01T21:20:23 --> 2014-09-01T22:50:23
The region was around S12 E114 at the time of the eruption. It is possible to trace the eruptjon to gradual ascention of closed loops. The lateral expansion was not as obvious as the previous event from AR 12158 at N14 E126.
Detected by halocme, Submitted at 2015-01-06T03:27:39
2014-09-01T10:45:35 --> 2014-09-01T12:21:35
Active Region 12158 produced several big eruptions. This preceded the Earth-directed CME on Sep 10, and the region was still at E126. This LCPF not only propagated along the limb, but also into the disk.
Detected by halocme, Submitted at 2015-01-06T03:05:26
2014-05-09T02:10:11 --> 2014-05-09T03:00:11
This is one of the most impressive large-scale coronal propagating fronts (LCPFs) in 2014. The eruption that drove the wave-like disturbance originated about 30 degrees behind the limb. This was followed by the prominence eruption that was well captured by IRIS.
Detected by halocme, Submitted at 2015-01-06T03:05:25
2014-05-09T02:10:11 --> 2014-05-09T03:00:11
This is one of the most impressive large-scale coronal propagating fronts (LCPFs) in 2014. The eruption that drove the wave-like disturbance originated about 30 degrees behind the limb. This was followed by the prominence eruption that was well captured by IRIS.
Detected by halocme, Submitted at 2015-01-04T04:52:35
2014-12-26T21:00:35 --> 2014-12-26T22:20:35
This eruption may given impression that the filament was broken up (around 21:33) as a result of the bulk motion toward south (in projection), which may have resulted from large-scale instability. Part of the broken filament may bave contributed to the narrow CME, first seen at 21:48 (after 21:24) by LASCO.
Detected by halocme, Submitted at 2015-01-04T01:57:51
2014-12-26T05:30:35 --> 2014-12-26T06:10:35
This apparently comes from the slightly occulted region AR 12241. It is quite fast and extensive, which is also inhereted in the associated CME. It is also responsible for an electron event at L1.
Detected by halocme, Submitted at 2015-01-04T01:51:07
2014-12-25T22:45:35 --> 2014-12-26T00:45:35
Multiple episodes of jets are seen. The overlying coronal structures respond more to later activities, say, after 00 UT, probably because they get loosened by the earlier jets.
Detected by halocme, Submitted at 2015-01-04T01:43:45
2014-12-24T23:40:11 --> 2014-12-25T01:10:11
This comes from the slighly occulted region AR 12242 and is associated with a C2.4 flare.
Detected by halocme, Submitted at 2015-01-04T01:37:08
2014-12-24T16:50:23 --> 2014-12-24T17:30:23
Another possibly high-latitude jet. Its footpoint appears to be occulted.
Detected by halocme, Submitted at 2015-01-04T01:29:25
2014-12-24T11:50:23 --> 2014-12-24T12:50:23
This jet appears to have resulted from reconnection of small bipoles at the coronal base.
Detected by halocme, Submitted at 2015-01-04T01:16:25
2014-12-24T10:30:35 --> 2014-12-24T11:40:35
This eruption from the far side initially appeared like a jet, but as it hits the overlying coronal structures, it affected them including minor dimming. No CME associated.
Detected by halocme, Submitted at 2015-01-04T01:03:26
2014-12-24T02:20:24 --> 2014-12-24T04:20:24
The filament material that erupted appears to have mostly come back, hence a confined eruption. However, in GOES light curves, the C3.7 flare was followed by a long-decay event (around a C3 level), which concides with a post-eruption arcade including a cusp. The event was also seen as a narrow CME by LASCO.
Detected by halocme, Submitted at 2015-01-04T01:03:25
2014-12-24T02:20:24 --> 2014-12-24T04:20:24
The filament material that erupted appears to have mostly come back, hence a confined eruption. However, in GOES light curves, the C3.7 flare was followed by a long-decay event (around a C3 level), which concides with a post-eruption arcade including a cusp. The event was also seen as a narrow CME by LASCO.
Detected by halocme, Submitted at 2015-01-03T19:56:28
2014-12-24T01:35:23 --> 2014-12-24T02:01:23
The linear structure is reminiscent of a jet or surge, but this ejection seems to trace a closed loop structure.
Detected by halocme, Submitted at 2015-01-03T19:44:32
2014-12-23T23:30:35 --> 2014-12-24T01:16:35
Two jets are seen to come from different areas of AR 12241. The second one seems to be connected with a third one from the limb region, as was the case with the last event.
Detected by halocme, Submitted at 2015-01-03T19:37:46
2014-12-23T12:25:11 --> 2014-12-23T13:31:11
This event in AR 12241 seems to trigger another one closer to the limb.
