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

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

Detected by cheung, Submitted at 2013-02-15T17:14:43

2013-02-13T16:30:03 --> 2013-02-13T23:50:03

A combination of drainage along field lines and in-situ heating may have contributed to the gradual disappearance of this filament (seen in 304, orange).

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

Detected by cheung, Submitted at 2013-02-15T17:07:17

2013-02-12T20:20:03 --> 2013-02-13T06:50:03

The first eruption leads to the appearance of a post-eruption arcade. As the arcade loops start to fade, another filament from the region is launched. It is difficult to establish a direct causal connection between the first eruption and the destabilization of the second.

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

Detected by halocme, Submitted at 2013-02-12T05:07:19

2013-02-08T22:00:03 --> 2013-02-09T03:00:03

Part of the east-west filament around the center of the images is seen to reconfigure, corresponding to a diffuse outflow seen on the west limb in EUVI/STB images (23:30-01:30). We should probably not ignore such slow and subtle changes when thinking of heliospheric disturbances.

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

Detected by halocme, Submitted at 2013-02-12T04:32:36

2013-02-08T07:30:35 --> 2013-02-08T10:00:35

This eruption is found while searching limb activities in EUVI/STB images. Although the erupted filament lay east of the active region, the flaring was also seen in the active region coe.

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

Detected by halocme, Submitted at 2013-02-11T23:12:13

2013-02-09T07:10:11 --> 2013-02-09T08:40:11

An outflow and dimming high up in the corona suggests that an eruption occurs behind the limb. However, in this case, STB data indicate the source region on or slighty inside the limb. However, 304 A images do not showa trace of prominence erution.

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

Detected by halocme, Submitted at 2013-02-11T21:42:29

2013-02-08T22:00:03 --> 2013-02-08T23:00:03

A major CME by LASCO with possible shock signatures. EUVI/STA data indicates an EUV wave. The source regions is 37 degrees behind the limb.

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

Detected by halocme, Submitted at 2013-02-11T21:25:30

2013-02-08T00:40:12 --> 2013-02-08T02:00:36

Vo clear filament eruption, but this B4.0 flare seems quite dymanic. It is associated with a narrow CME observed by LASCO in the NW quadrant (but not by STEREO coronagraphs).

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

Detected by halocme, Submitted at 2013-02-11T02:45:27

2013-02-09T04:30:35 --> 2013-02-09T08:00:35

Changes in the northern part of the filament was more apparent before the eruption took off. A large area north of the eruption is seen to dim. Post-flare loops and flare ribbons are clearly observed. The associated CME is not very spectacular with the bright part confined to north. Therefore, it is not likely that this eruption will hit the geo-space.

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

Detected by anny, Submitted at 2013-02-08T20:39:14

2013-02-07T00:00:03 --> 2013-02-07T05:03:03

A large flux rope lifts up and then most of it sinks back. There is a small blob, however, that separates from the apex, keeps hanging in the corona for a little longer than the rest of the filament, and than disappears.

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

Detected by derosa, Submitted at 2013-02-08T00:51:14

2013-02-02T06:00:03 --> 2013-02-03T00:00:03

Initial stages of a small active region on the solar disk. A day or two later, this newly emergent flux region develops a sunspot and is labeled as AR11668.

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

Detected by anny, Submitted at 2013-02-07T23:42:02

2013-02-06T11:09:03 --> 2013-02-07T00:00:03

A thin vertically extended structure in 304A slowly becomes elongated in a mushroom-like structure which in turn slowly merges with a second thin vertical spike nearby. Little to nothing shows up in 211A.

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

Detected by anny, Submitted at 2013-02-07T22:51:11

2013-02-05T14:09:03 --> 2013-02-05T17:39:03

A nice swirling structure in 304A on the W imb.

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

Detected by anny, Submitted at 2013-02-07T22:49:11

2013-02-05T09:42:03 --> 2013-02-05T12:24:03

Filament eruption on the SE disk.

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

Detected by anny, Submitted at 2013-02-07T18:06:02

2013-02-05T05:24:03 --> 2013-02-05T10:48:03

Two massive spray surges burst out of the same AR on the E limb a few hours apart. They are associated with two weak flares, B-class and C-class at most.

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

Detected by derosa, Submitted at 2013-02-06T00:35:00

2013-01-31T18:00:02 --> 2013-01-31T22:00:02

A small filament aligned with the polarity inversion line separating a small bipolar region erupts, leaving behind evacuated [dark] regions in the regions where the filament was formerly anchored.

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

Detected by derosa, Submitted at 2013-02-05T22:57:48

2013-01-31T03:00:05 --> 2013-01-31T12:00:05

A horseshoe-shaped filament associated with AR11666 erupts over the southeast limb. The filament material remains active for several hours after the primary portion of the erupting filament is no longer visible.

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

Detected by derosa, Submitted at 2013-02-05T22:50:31

2013-01-31T11:00:05 --> 2013-01-31T21:00:05

Long filament erupts on the west limb, making for a spectacular eruption. Lots of apparent untwisting by this filament, which extends eastward from AR11665.

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

Detected by seguin, Submitted at 2013-02-05T02:03:10

2012-11-16T05:00:03 --> 2012-11-16T12:00:03

A large filament eruption on the eastern limb goes off nearly simultaneously with one in central longitudes, in the southern hemisphere. The southern eruption rains material into the southern polar crown coronal cavity. Both eruptions have a fair amount of coronal rain.

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

Detected by seguin, Submitted at 2013-02-05T02:03:09

2012-11-16T05:00:03 --> 2012-11-16T12:00:03

A large filament eruption on the eastern limb goes off nearly simultaneously with one in central longitudes, in the southern hemisphere. The southern eruption rains material into the southern polar crown coronal cavity. Both eruptions have a fair amount of coronal rain.

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

Detected by seguin, Submitted at 2013-02-05T02:03:08

2012-11-16T05:00:03 --> 2012-11-16T12:00:03

A large filament eruption on the eastern limb goes off nearly simultaneously with one in central longitudes, in the southern hemisphere. The southern eruption rains material into the southern polar crown coronal cavity. Both eruptions have a fair amount of coronal rain.