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 2016-07-17T06:16:59

2016-07-13T14:25:10 --> 2016-07-13T15:51:10

This seems to come from the following part of AR 12562. The ejection may be confined and deflected to east, as seen in a brightening near the south pole.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-17T05:09:56

2016-07-12T08:00:06 --> 2016-07-12T09:10:06

This is a quite bright jet, but the cenrtral part appears dark especially in 211 A images. The footpoints are appaerntly occulted.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-17T04:59:21

2016-07-12T01:10:10 --> 2016-07-12T02:20:10

A tiny filament appears to have erupted from a small region. But not only a post-eruption arcade formed but also dimming was seen above the region (over the limb) and at a remote region to northwest, suggesting that the eruption may have been more extended than the small region.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-17T04:35:07

2016-07-11T18:20:22 --> 2016-07-11T19:30:22

This seems to start as slow rise of a small filament, which then gets broken up into a narrow eruption. Footpoint brightening is hardly seen.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-17T00:45:41

2016-07-10T15:05:22 --> 2016-07-10T15:51:22

A diffuse eruption whose source regtion may have been slighly occulted, given that part of the erupting prominence was seen in 304 A images.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-17T00:34:34

2016-07-10T00:30:34 --> 2016-07-10T02:30:34

Yet another homologous eruption from AR 12564 that caused oscillations of the coronal structures to the north. The eruption itself was collimated and the associated CME was localized (cf. https://twitter.com/halocme/status/752002717048975360).

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-17T00:34:33

2016-07-10T00:30:34 --> 2016-07-10T02:30:34

Yet another homologous eruption from AR 12564 that caused oscillations of the coronal structures to the north. The eruption itself was collimated and the associated CME was localized (cf. https://twitter.com/halocme/status/752002717048975360).

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-16T23:52:23

2016-07-09T21:15:34 --> 2016-07-09T22:51:34

This event may be homologous to the earlier C2.6 flare. But the eruption is more collimated and the wave propagating clockwise is less pronounced. Moreover, the coronal structure that was traversed by the eruption is seen to oscillate.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-16T23:52:22

2016-07-09T21:15:34 --> 2016-07-09T22:51:34

This event may be homologous to the earlier C2.6 flare. But the eruption is more collimated and the wave propagating clockwise is less pronounced. Moreover, the coronal structure that was traversed by the eruption is seen to oscillate.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-16T23:52:21

2016-07-09T21:15:34 --> 2016-07-09T22:51:34

This event may be homologous to the earlier C2.6 flare. But the eruption is more collimated and the wave propagating clockwise is less pronounced. Moreover, the coronal structure that was traversed by the eruption is seen to oscillate.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-16T21:45:49

2016-07-09T15:40:10 --> 2016-07-09T17:40:10

The non-radial eruption started in AR 12564. A coronal wave is seen to propagate preferentially clockwise over the limb.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-16T21:45:49

2016-07-09T15:40:10 --> 2016-07-09T17:40:10

The non-radial eruption started in AR 12564. A coronal wave is seen to propagate preferentially clockwise over the limb.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-16T06:07:24

2016-07-08T01:35:22 --> 2016-07-08T03:05:22

This appears to be a repetition of the earlier event (around 7 July 2016 23:30).

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-16T06:02:39

2016-07-08T01:25:10 --> 2016-07-08T02:15:10

The source region may be on the backside - no footpoint brightening seen.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-16T05:54:11

2016-07-07T23:35:22 --> 2016-07-08T00:25:22

A mini-filament eruption seems to trigger a jet that was ejected to northwest, leaving post-flare loops to the left.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-16T05:42:59

2016-07-07T23:25:10 --> 2016-07-08T00:21:10

A collimated ejection toward south, giving an impression that the coronal structure far south gets disturbed.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2016-07-16T05:35:16

2016-07-07T07:40:10 --> 2016-07-07T08:40:10

The wave seems to be deflected to east by the coronal hole to the north of AR 12561.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by gchintzo, Submitted at 2016-07-07T21:55:13

2016-07-06T15:00:06 --> 2016-07-07T18:00:06

Simultaneous emergence of two small bipoles in close proximity to each other and the associated coronal activity (C5.1 flare). The quality of the movie is affected during a scheduled SDO spacecraft roll.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by gchintzo, Submitted at 2016-07-07T20:58:17

2016-07-05T18:00:06 --> 2016-07-06T04:00:06

A patch of cool filament material is being displaced during the filament activation. The activation causes flare ribbon-like activity in the north east end of the filament. At the end of the activation, the cool material patch undergoes oscillations.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by gchintzo, Submitted at 2016-07-07T20:32:10

2016-07-05T13:00:06 --> 2016-07-06T04:00:06

Post-flare loop activity (B1.6 flare) in the center of the field of view following filament activation (possibly associated with a CME observed in SOHO/LASCO). IRIS observed the activation in coordination with GREGOR. To see the IRIS data follow the link: http://www.lmsal.com/hek/hcr?cmd=view-event&event-id=ivo://sot.lmsal.com/VOEvent23VOEvent_IRIS_20160704_075921_3660258324_2016-07-04T07:59:212016-07-04T07:59:21.xml