Highest Rated Events (only 193 and 304 shown) All AR FE FL
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-09-14T07:13:18
2017-09-06T08:40:13 --> 2017-09-06T10:30:37
There are some motions related to the flare and even small dimming, but overall it is a non-eruptive event and may the coronalgraph features (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170906.083607.w025.v0224.p260&frame=7&r) may not represent a real CME or related to this flare.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2017-09-06T22:09:04
2017-09-04T10:40:09 --> 2017-09-05T03:50:09
AR12674 is classified as a bipolar beta sunspot group (red negative, green positive photospheric magnetic polarities). Note the moving magnetic features/moat flow around the leading negative sunspot (positive polarity) which seem associated with jet-like activity in the corona.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by gchintzo, Submitted at 2017-09-06T21:54:11
2017-09-03T08:30:09 --> 2017-09-03T12:16:33
A confined eruption that occurred on the West limb. Note the impulsiveness of the confined eruption and the pushing of the field above it.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-06T21:22:11
2017-09-02T07:50:09 --> 2017-09-03T00:00:09
FLux emergence was observed from a small region in the southern hemisphere. A small-scale active region was formed and magnetic connection started to develop between the two near-by active regions.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-06T21:14:53
2017-09-02T14:54:09 --> 2017-09-02T17:32:09
A big eruption at the west limb. The related filament was activated and heated before the eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-06T21:14:52
2017-09-02T14:54:09 --> 2017-09-02T17:32:09
A big eruption at the west limb. The related filament was activated and heated before the eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-06T18:27:00
2017-08-31T00:00:09 --> 2017-08-31T06:10:09
A filament was observed falling back to the Sun and formed "coronal rain", which leaded multiple brightenings in the surrouding region.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-01T01:41:47
2017-08-28T02:28:09 --> 2017-08-28T06:20:09
An eruption observed at the west limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-01T01:33:40
2017-08-30T15:38:09 --> 2017-08-30T16:58:09
A jet-like eruption from AR 12672.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-09-01T01:24:47
2017-08-28T13:40:09 --> 2017-08-29T02:00:09
An eruption from AR 12672. Post-flaring coronal loops can be seen with double-ribbon feature.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2017-08-28T20:59:33
2017-08-27T16:26:09 --> 2017-08-27T22:00:09
Several filament eruptions near the east limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-08-28T06:16:20
2017-08-21T14:00:09 --> 2017-08-21T19:00:09
The NW/NNW streamer was not clear in the PSI eclipse prediction. The appearance of two bipolar regions side-by-side may indicate a pseudostreamer.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-08-28T05:14:31
2017-08-21T15:00:09 --> 2017-08-21T19:00:09
Around the time of Eclipse2017, there was actually an unimpressive CME (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20170821.160010.w037.v0191.p096&frame=17&r). STEREO-A EUVI images show a slow filament eruption behind the east limb. AIA images seem to marginally capture the post eruption arcade.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-08-28T04:58:49
2017-08-24T00:25:13 --> 2017-08-24T01:10:49
A minor eruption that accompanied the C3.0 flare in AR 12671 went primarily westward, whereas the coronal wave propagated southward. A secondary wave from the interaction of the eruption with the adjacent structure is seen off the limb. No CME was associated with this event.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-08-28T04:58:48
2017-08-24T00:25:13 --> 2017-08-24T01:10:49
A minor eruption that accompanied the C3.0 flare in AR 12671 went primarily westward, whereas the coronal wave propagated southward. A secondary wave from the interaction of the eruption with the adjacent structure is seen off the limb. No CME was associated with this event.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-08-28T00:44:32
2017-08-20T19:00:09 --> 2017-08-20T21:00:09
Another flare in AR 12672, which was similar to the earlier M1.1 event, in the sense that its eruptive action, mostly radial, left the loops above the AR oscillating.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-08-28T00:44:32
2017-08-20T19:00:09 --> 2017-08-20T21:00:09
Another flare in AR 12672, which was similar to the earlier M1.1 event, in the sense that its eruptive action, mostly radial, left the loops above the AR oscillating.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-08-28T00:35:35
2017-08-20T01:20:25 --> 2017-08-20T02:45:37
The flare occurred as AR 12672 rotated on to the visible disk. Its associated eruption was more radial than lateral (i.e. only a weak EUV wave). The loop osciollation was a notable feature of this flare.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-08-28T00:35:34
2017-08-20T01:20:25 --> 2017-08-20T02:45:37
The flare occurred as AR 12672 rotated on to the visible disk. Its associated eruption was more radial than lateral (i.e. only a weak EUV wave). The loop osciollation was a notable feature of this flare.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2017-08-28T00:25:52
2017-08-19T21:10:13 --> 2017-08-19T22:51:01
The flare in AR 12671 seemed to be triggered by a filament eruption toward north. The wave front formed as a result of the eruption and was limited to the northern direction.
