Highest Rated Events (only 193 and 304 shown) All AR FE FL

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2011-10-04T19:55:30

2011-10-01T08:44:04 --> 2011-10-01T12:22:04

A clour of plasma emitting in 304 and 171A is thrown away during a large eruption and runs away from the field of view at very large speed. It takes it about 17 minutes from the beginning of the eruption to reach the highlighted region as opposed to half hour till the main front gets there.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2011-10-04T19:45:55

2011-10-01T08:44:04 --> 2011-10-01T12:22:04

Spectacular eruption of seemingly minor flux rope. There was a small flare immediately prior to this eruption in a nearby active region, the one that produced another large erution shortly afterwards.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2011-09-19T04:40:30

2011-09-07T21:42:36 --> 2011-09-08T02:06:36

X1.8 class flare truggered a spectacular large-scale eruption. The erupted matter at first appears bright in 304A and dark opaque in 211A and 171A. Some of the erupted material falls back to the region connected to the erupted site by loops emittin gin 211A. However, big amount of material falls back to an otherwise unremarkable requion on the quiet Sun as coronal rain bright in all these three wavelengths. Remarkably, the nearby filament, almost adjacent to the site of the eruption, does not erupt, although is clearly disturbed by the eruption as it is seen oscillating.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2011-09-19T04:40:29

2011-09-07T21:42:36 --> 2011-09-08T02:06:36

X1.8 class flare truggered a spectacular large-scale eruption. The erupted matter at first appears bright in 304A and dark opaque in 211A and 171A. Some of the erupted material falls back to the region connected to the erupted site by loops emittin gin 211A. However, big amount of material falls back to an otherwise unremarkable requion on the quiet Sun as coronal rain bright in all these three wavelengths. Remarkably, the nearby filament, almost adjacent to the site of the eruption, does not erupt, although is clearly disturbed by the eruption as it is seen oscillating.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2011-09-19T04:40:28

2011-09-07T21:42:36 --> 2011-09-08T02:06:36

X1.8 class flare truggered a spectacular large-scale eruption. The erupted matter at first appears bright in 304A and dark opaque in 211A and 171A. Some of the erupted material falls back to the region connected to the erupted site by loops emittin gin 211A. However, big amount of material falls back to an otherwise unremarkable requion on the quiet Sun as coronal rain bright in all these three wavelengths. Remarkably, the nearby filament, almost adjacent to the site of the eruption, does not erupt, although is clearly disturbed by the eruption as it is seen oscillating.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by asainz, Submitted at 2011-08-26T02:28:07

2011-08-23T07:40:04 --> 2011-08-25T13:20:04

Coronal structure moves from the North pole to lower latitude position. It starts as tornado in the North Pole, then it moves down through the polar cap forming wide, diffuse loops, it seems to be broken and it eventually reconnects to the surface in a lower latitude.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by asainz, Submitted at 2011-08-11T00:53:38

2011-08-07T00:00:04 --> 2011-08-08T12:50:04

Filament eruption in the North polar cap, ending with a broken loop returning to the Sun as coronal rain.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by weiliu, Submitted at 2011-08-06T02:21:23

2011-08-04T03:30:00 --> 2011-08-04T09:00:00

Splendid filament eruption and coronal EUV wave at the M9 flare. The wave covers about 3/4 of the entire solar disk.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-07-01T00:31:20

2011-06-13T22:59:55 --> 2011-06-15T11:59:55

Large-scale eruption with apparent post-eruption arcades as in AR events, but spread over more than a solar radius across the disk above quiet Sun.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-07-01T00:13:29

2011-06-27T22:00:04 --> 2011-06-30T00:06:04

Emerging small active region, visible over multiple days, as it grows and interacts with its surroundings, moving across the central meridian.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-07-01T00:05:33

2011-06-29T00:12:04 --> 2011-06-29T01:58:04

Eruption at the SW limb, with an expansion front, and wave-like phenomena on the edges of the expansion front after the eruption has passed by.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2011-06-14T16:41:15

2011-06-13T00:50:34 --> 2011-06-13T02:29:56

A humongous surge following a flare. The fractionation of the globules in 304 as the surge material falls back toward the surface is particularly interesting.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-06-08T15:24:22

2011-06-07T05:35:56 --> 2011-06-07T10:31:56

An M2.5 flare associated with the largest, most impressive filament eruption seen to date with AIA. Large amounts of chromospheric material are thrown upward (much is part of a CME), with subsequently much falling down again and creating impact brighteninings over half a solar radius away.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-06-08T15:24:19

2011-06-07T05:35:56 --> 2011-06-07T10:31:56

An M2.5 flare associated with the largest, most impressive filament eruption seen to date with AIA. Large amounts of chromospheric material are thrown upward (much is part of a CME), with subsequently much falling down again and creating impact brighteninings over half a solar radius away.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-05-19T17:31:57

2011-05-11T01:43:55 --> 2011-05-11T03:55:55

Filament eruption (and two-ribbon flare), transitioning into a clear "bubble-like" coronal propagating front (EIT wave) as the eruption transitions to a CME.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-05-19T17:31:54

2011-05-11T01:43:55 --> 2011-05-11T03:55:55

Filament eruption (and two-ribbon flare), transitioning into a clear "bubble-like" coronal propagating front (EIT wave) as the eruption transitions to a CME.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-05-10T19:48:48

2011-05-09T18:35:55 --> 2011-05-09T23:51:55

Eruption on the NE limb showing a very strong volume expansion and a coronal propagating front.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-04-29T22:30:57

2011-04-28T03:07:55 --> 2011-04-28T14:43:55

Formation of an absorbing filament over quiet Sun near SE limb.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-03-30T22:13:04

2011-02-10T00:00:04 --> 2011-02-15T06:00:04

Active region emergence from start to past X2.2 flare (4.25d interval).

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2011-03-23T21:55:32

2011-03-16T18:28:05 --> 2011-03-16T20:12:05

The 171-193-211 color changes in the quiet-Sun corona following an eruption further west suggest that the coronal propagating front ("EIT wave") is associated with a coronal temperature change (possibly adiabatic, possibly reflecting heating).