Highest Rated Events (only 193 and 304 shown) All AR FE FL
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-01-19T00:23:51
2017-01-14T12:00:09 --> 2017-01-14T13:13:21
A small-scale active region surge. The eruption is a confined one.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-01-19T00:13:45
2017-01-14T07:04:09 --> 2017-01-14T09:12:09
Two eruptions occured at the east and west limb nearly at the same time.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-01-18T23:28:42
2017-01-09T14:04:09 --> 2017-01-09T15:57:09
Filament eruption near an active region. Multiple brightenings are seen during the process.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-01-18T23:11:11
2017-01-09T15:22:09 --> 2017-01-09T16:45:09
On-disk minifilament eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-01-18T19:49:25
2017-01-09T00:00:09 --> 2017-01-09T03:10:09
On-disk minifilament eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-01-18T19:39:10
2017-01-09T13:56:09 --> 2017-01-09T16:06:09
A minifilament eruption from the southern coronal hole.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T16:48:45
2017-01-02T14:50:25 --> 2017-01-02T17:00:25
As is often the case, only small part of the filament appeared to erupt. The motions seemed to trace a helical structure. No clear CME association.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T16:37:36
2017-01-02T02:00:09 --> 2017-01-02T13:00:09
This coronal hole was impressively large. However, not the whole area was permeated by open field lines, in this case of negative polarity. There were bright points here and there, which sometimes showed transient activities including jets.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T16:26:58
2017-01-02T08:00:09 --> 2017-01-02T10:00:09
The eruption accompanies whirling motions that also propagated to an adjacent filament on the disk. The corona was hardly affected by this eruption, and no CME resulted.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T07:50:40
2017-01-01T06:00:09 --> 2017-01-01T10:00:09
This filament eruption is diffuse and its associated chromospheric flare emission is also weak. No CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T07:40:45
2016-12-31T22:00:06 --> 2016-12-31T23:00:06
It appears that a minor eruption involving a filament in AR 12622 excited a neighboring longer filament, resulting in two-ribbon emission.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T07:40:45
2016-12-31T22:00:06 --> 2016-12-31T23:00:06
It appears that a minor eruption involving a filament in AR 12622 excited a neighboring longer filament, resulting in two-ribbon emission.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T07:33:22
2016-12-30T19:00:06 --> 2016-12-30T21:00:06
The eruption appears to be confined. It was limb-occulted. There was a time lag of the adjecent coronal structure to respond to the eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T07:28:20
2016-12-30T03:40:10 --> 2016-12-30T05:40:10
This is probably an ejeciton of mass into a filament due to reconnection at its leg, which is in the periphery of AR 12622.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T07:06:37
2016-12-29T02:00:06 --> 2016-12-29T11:00:06
This appears to occur behind but close to the limb. Turbulent motions precede the eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T06:56:21
2016-12-28T00:00:06 --> 2016-12-29T00:00:06
This coronal hole was quite eye-catching. There are quite a few bright points inside the coronal hole. The coronal hole is not rooted by open field lines and interchange reconnection could be frequent occuring not only around the coronal hole boundaries but also inside.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-01-12T06:43:24
2016-12-26T10:40:14 --> 2016-12-26T13:00:14
This is a diffuse eruption, wider than a typical jet. The source region is probably slightly behind the limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2016-12-19T18:54:19
2016-12-17T16:20:06 --> 2016-12-17T22:40:06
Synchronous activities were observed from two distanced active regions.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2016-12-19T18:35:31
2016-12-17T23:40:06 --> 2016-12-19T00:00:06
A flux emerging region was observed in the on-disk coronal hole (near the boundary). The emerged flux then deveoped connections with the surrounding small-scale fluxes.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2016-12-17T00:59:21
2016-12-15T03:23:06 --> 2016-12-15T04:07:06
A failed eruption was observed at the west limb. Wave-feature was observed propagating across field lines. A flux-rope like structure was also observed to raise and fall back.
