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 2015-01-10T04:36:02
2014-12-29T15:20:23 --> 2014-12-29T17:00:23
Two eruptions, one near AR 12246 and another probably behind the east limb, are seen nearly at the same time, suggesting a possible large-scale link.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-10T04:25:29
2014-12-29T08:30:35 --> 2014-12-29T09:30:35
This eruption is from the same region as the previous two (Dec 28 00:50, 10:50). Smaller opening, but the filament is suggestive of more twisting.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-10T04:17:00
2014-12-28T10:45:35 --> 2014-12-28T11:45:35
The same region as the previous event (Dec 28, 00:50) erupted. The filament is more clearly seen in this event, which also seems to be more explosive.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-10T04:06:15
2014-12-28T00:45:35 --> 2014-12-28T01:59:35
This may correspond to what used to be called a mini-filament eruption. As a result a small area is seen to dim.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-10T03:50:50
2014-12-27T17:50:23 --> 2014-12-27T18:40:23
The 304 A images alone give us an impression of a minor eruption, but it seems to have more global effects. Large-scale structures to the south oscillate as a result of the eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-10T03:50:50
2014-12-27T17:50:23 --> 2014-12-27T18:40:23
The 304 A images alone give us an impression of a minor eruption, but it seems to have more global effects. Large-scale structures to the south oscillate as a result of the eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by weiliu, Submitted at 2015-01-07T01:23:58
2015-01-03T00:00:03 --> 2015-01-04T00:00:03
A ploar crown prominence appears in the lower portion of concaved shaped loops, possibly a coronal cavity. It lifts off gradually, dispersed, flows sideway, and disappears.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2015-01-06T22:50:59
2015-01-06T05:10:03 --> 2015-01-06T06:00:03
The optically thick filament vanishes whiles bright strands appear in the 304 channel. The apparent motion of the material in the bright strands suggests the heated plasma is trapped in the AR.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2015-01-06T20:00:48
2015-01-05T17:10:03 --> 2015-01-05T18:22:03
The west end of this AR filament seems to be destabilized by magnetic cancellation between opposite polarities of the AR.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-06T18:24:59
2013-08-08T17:30:35 --> 2013-08-08T19:10:35
AR 11810 looked sigmoidal prior to the eruption that triggered this LCPF. The associated flare was only B4.1.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-06T18:24:58
2013-08-08T17:30:35 --> 2013-08-08T19:10:35
AR 11810 looked sigmoidal prior to the eruption that triggered this LCPF. The associated flare was only B4.1.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-06T18:24:58
2013-08-08T17:30:35 --> 2013-08-08T19:10:35
AR 11810 looked sigmoidal prior to the eruption that triggered this LCPF. The associated flare was only B4.1.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-06T15:49:20
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).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-06T15:49:19
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).
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-06T04:00:03
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-06T04:00:02
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-04T04:52:30
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-04T01:57:46
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-04T01:51:02
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.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2015-01-04T01:43:39
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.
