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 2017-05-30T23:57:19

2017-05-24T09:30:09 --> 2017-05-24T21:10:09

Three eruptions from AR 12660 were observed. The second one is more energetic than the other two.

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

Detected by jinmeng, Submitted at 2017-05-27T02:44:39

2017-05-21T00:00:09 --> 2017-05-22T15:30:09

Flux emergence and active region forming process were observed.

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

Detected by jinmeng, Submitted at 2017-05-27T02:34:09

2017-05-23T12:40:09 --> 2017-05-23T18:20:09

An eruption was observed from AR 12660.

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

Detected by jinmeng, Submitted at 2017-05-27T02:09:13

2017-05-20T14:10:09 --> 2017-05-21T00:00:09

A filament eruption was observed near the East Limb.

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

Detected by jinmeng, Submitted at 2017-05-27T01:27:28

2017-05-20T15:00:09 --> 2017-05-20T20:45:45

A small quiet Sun filament eruption near the south polar region.

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

Detected by jinmeng, Submitted at 2017-05-27T01:21:07

2017-05-18T02:20:09 --> 2017-05-18T08:00:09

A small explosive event in the quiet Sun was observed near the east limb, with synchronous activitiy seen near the north polar coronal hole.

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

Detected by gchintzo, Submitted at 2017-05-23T18:09:53

2017-05-15T08:50:09 --> 2017-05-17T04:00:09

A narrow North-South oriented coronal hole (dark region) traversing the solar equator.

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

Detected by halocme, Submitted at 2017-05-07T06:01:56

2017-05-05T22:30:01 --> 2017-05-05T23:30:01

This flare may be called eruptive by some, because a large area to the north seems to have been impacted. But there is no way it was associated with a CME even in the limb view. There may have been disturbances due to MHD waves but it seems that no flux rope was involved, hence no CME.

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

Detected by halocme, Submitted at 2017-05-07T05:38:12

2017-05-05T03:50:25 --> 2017-05-05T05:30:25

The pre-eruption filament is not clear, but the formation of flare ribbons and loops between them suggests an eruption. An area larger to the south more extended than the ribbons is seen to dim, especially in 171 A.

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

Detected by halocme, Submitted at 2017-05-07T05:38:12

2017-05-05T03:50:25 --> 2017-05-05T05:30:25

The pre-eruption filament is not clear, but the formation of flare ribbons and loops between them suggests an eruption. An area larger to the south more extended than the ribbons is seen to dim, especially in 171 A.

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

Detected by halocme, Submitted at 2017-05-07T05:13:29

2017-05-03T19:55:13 --> 2017-05-03T21:31:13

Continued surge-like activities came from two regions near the limb. It is not clear whether the eruptions only delineated closed structures, or how the two regions were linked.

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

Detected by halocme, Submitted at 2017-05-07T05:03:39

2017-05-02T11:50:25 --> 2017-05-02T15:50:25

The pre-eruption filament was not clearly seen, but a moving dark feature may have been a filament eruption. The event was captured only in 304 A channel, without showing clear flare ribbons or post eruption arcades

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

Detected by halocme, Submitted at 2017-05-07T04:49:58

2017-05-01T12:55:13 --> 2017-05-01T13:50:25

This eruption was associated with a B3.0 flare from the same region (without NOAA AR number) as the earlier B9.9 flare. The eruption itself was weaker, but the coronal wave is clearly seen to propagate counterclockwise along the limb in difference images especially in 193 A channel.

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

Detected by halocme, Submitted at 2017-05-07T04:49:58

2017-05-01T12:55:13 --> 2017-05-01T13:50:25

This eruption was associated with a B3.0 flare from the same region (without NOAA AR number) as the earlier B9.9 flare. The eruption itself was weaker, but the coronal wave is clearly seen to propagate counterclockwise along the limb in difference images especially in 193 A channel.

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

Detected by halocme, Submitted at 2017-05-07T04:39:49

2017-05-01T03:50:25 --> 2017-05-01T04:30:01

The eruption associated with the B9.9 flare was pronounced in the radial direction. But difference images also show a large scale wave propagating counterclockwise along the limb.

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

Detected by halocme, Submitted at 2017-05-07T04:39:49

2017-05-01T03:50:25 --> 2017-05-01T04:30:01

The eruption associated with the B9.9 flare was pronounced in the radial direction. But difference images also show a large scale wave propagating counterclockwise along the limb.

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

Detected by halocme, Submitted at 2017-05-07T00:08:06

2017-04-30T18:15:01 --> 2017-04-30T19:15:01

This jet is not clear close to the origin, although small post flare loops are seen indicating magnetic reconnection between closed and open field lines. It is easier to be seen at higher altitudes (within AIA FOV) as the surrounding structures being pushed away. Running difference images (not shown here) reveal an outward motion in intensity deficit (dimming) in all the three channels in the movie.

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

Detected by halocme, Submitted at 2017-05-06T20:05:56

2017-04-29T22:40:13 --> 2017-04-30T05:00:13

The eruption started slowly in AR 12653 (without a clear filament as a marker) but produced significant coronal dimming on both sides of the flare ribbons. Post eruption arcades were formed, explaining the associated B3.0 long-decay event in soft X-rays. This eruption did not arrive at Earth.

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

Detected by halocme, Submitted at 2017-05-06T20:05:56

2017-04-29T22:40:13 --> 2017-04-30T05:00:13

The eruption started slowly in AR 12653 (without a clear filament as a marker) but produced significant coronal dimming on both sides of the flare ribbons. Post eruption arcades were formed, explaining the associated B3.0 long-decay event in soft X-rays. This eruption did not arrive at Earth.

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

Detected by halocme, Submitted at 2017-05-06T19:56:32

2017-04-29T12:50:25 --> 2017-04-29T14:40:25

This may be a disk view of a failed eruption which does not escape from the Sun. It occurred in AR 12653, which had already decayed to 1/3 of its maximum size.