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 2014-04-26T02:43:07
2014-04-19T11:15:35 --> 2014-04-19T12:15:35
In this case, the one in the south was followed by another one in the north. These ejections were related with a broad (but diffuse) front in between, suggestive of a CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-04-26T02:43:06
2014-04-19T11:15:35 --> 2014-04-19T12:15:35
In this case, the one in the south was followed by another one in the north. These ejections were related with a broad (but diffuse) front in between, suggestive of a CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-04-26T02:25:40
2014-04-19T09:00:03 --> 2014-04-19T09:50:27
It appears that the second event occurred while a footpoint of the first event was still in motion, therefore suggesting a causal relation. The first one was more ejective and the second one more clearly showed a twisted structure.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2014-04-25T02:08:22
2014-04-22T04:44:03 --> 2014-04-22T17:26:03
A prominence slowly forms on the S pole, slowly develops and slowly takes off.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-04-24T23:37:48
2014-04-19T06:30:35 --> 2014-04-19T07:30:35
During 19-21 April 2014, many eruptions of different sizes and appearances were seen near the west limb, and most the subsequent annotations may deal with them. In this event, the off-limb part may attract more attention, but the motions and brightening northeast of the main flaring region remind us that a larger area participated in the eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-04-24T23:37:46
2014-04-19T06:30:35 --> 2014-04-19T07:30:35
During 19-21 April 2014, many eruptions of different sizes and appearances were seen near the west limb, and most the subsequent annotations may deal with them. In this event, the off-limb part may attract more attention, but the motions and brightening northeast of the main flaring region remind us that a larger area participated in the eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-15T22:40:23
2014-04-14T21:10:03 --> 2014-04-15T15:00:03
A filament destabilizes but its rise is halted mid-corona. Thereafter the 304 material drains out of the field lines (or is heated out of the passband), the temporarily invisible loop seems to eventually reappear in 211 and 171.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-15T22:40:23
2014-04-15T17:20:03 --> 2014-04-15T19:00:03
This filament eruption leads to the injection of material into high-reaching loops.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-15T22:40:22
2014-04-15T17:20:03 --> 2014-04-15T19:00:03
This confined eruption seems to have only a small impact on neighboring loops. However, it occurs just about half an hour before another filament eruption at the preceding edge of AR 12035.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-15T22:40:22
2014-04-14T21:10:03 --> 2014-04-15T15:00:03
A filament destabilizes but its rise is halted mid-corona. Thereafter the 304 material drains out of the field lines (or is heated out of the passband), the temporarily invisible loop seems to eventually reappear in 211 and 171.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-15T18:40:17
2014-04-12T07:00:03 --> 2014-04-12T08:50:03
Much of the material seen in the 304 signal seem to disappear in situ, so perhaps it is heated out of the passband.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-11T22:40:17
2014-04-09T23:30:03 --> 2014-04-10T00:30:03
This faint filament in 304 seems to erupt in such a way that the material from the legs of the filament get sucked up toward the apex.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-11T22:40:17
2014-04-11T11:10:03 --> 2014-04-11T13:20:03
A small eruption injects filament material into neighboring field lines
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-11T19:40:17
2014-04-09T23:20:03 --> 2014-04-10T00:30:03
This filament activation reveals some twisted field lines wrapping around the filament.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-11T18:40:20
2014-04-08T03:00:03 --> 2014-04-09T05:10:03
The hopping motion seems associated with the rise of the overlying coronal cavity.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-11T18:40:18
2014-04-08T03:00:03 --> 2014-04-09T05:10:03
The hopping motion seems associated with the rise of the overlying coronal cavity.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-04-11T18:40:17
2014-04-08T03:00:03 --> 2014-04-09T05:10:03
The hopping motion seems associated with the rise of the overlying coronal cavity.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2014-04-09T01:40:18
2014-04-03T21:50:03 --> 2014-04-04T00:00:03
A blob of coronal puff, propelled upwards in a filament eruption, persists in the S corona for prolonged time, wiggling and getting distorted.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2014-04-09T01:40:18
2014-04-03T14:10:03 --> 2014-04-03T17:38:03
A confined eruption on the W limb. Note the proximity of a coronal null in the plane of sky.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2014-04-09T01:40:17
2014-04-02T10:48:03 --> 2014-04-02T12:44:03
A sigmoid flow along a silament. One half of the S appears to be elevated above the surface.
