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 2012-01-28T02:27:00

2012-01-24T12:20:24 --> 2012-01-24T13:40:24

This jet in the polar region and its associated post-eruption loops are best observed at 211 A. They are hardly recognizable at 171 A.

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

Detected by halocme, Submitted at 2012-01-28T02:20:11

2012-01-24T13:30:00 --> 2012-01-24T15:00:00

The eruption is observed in the form of dimming at 211 A. Surge-like motions follow at 304 A. This eruption is associated with a minor CME.

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

Detected by halocme, Submitted at 2012-01-28T02:02:48

2012-01-24T01:50:24 --> 2012-01-24T03:20:24

This is so diffuse that one almost needs difference images to show it. The driver for this jet is not found for now.

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

Detected by halocme, Submitted at 2012-01-28T01:40:41

2012-01-23T19:20:24 --> 2012-01-23T21:20:24

A small eruption occurs in the western hemisphere, close to the central meridian, propagating toward east and causing an outflow/jet on the NE limb. This is just an impression from viewing difference movies, but such a large-scale linke may be possible.

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

Detected by anny, Submitted at 2012-01-27T03:03:17

2012-01-25T23:22:04 --> 2012-01-26T06:48:04

A flare triggers a spray surge in AR on the NW limb. Soon after that there are a few bubble eruptions visible in 211A channel with little activity in 304A.

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

Detected by anny, Submitted at 2012-01-27T03:03:14

2012-01-25T23:22:04 --> 2012-01-26T06:48:04

A flare triggers a spray surge in AR on the NW limb. Soon after that there are a few bubble eruptions visible in 211A channel with little activity in 304A.

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

Detected by halocme, Submitted at 2012-01-26T23:17:50

2012-01-23T00:00:04 --> 2012-01-23T06:00:04

This movie contains two episodes of eruptions producing two halo CMEs. The first one is less noticeable, until 02:30 or so, showing opening up of large-scale structures. The second event involves the eruption of a clear filament, whose activation already started during the first episode. The halo CME from the second event is more northward and much faster, overtaking the second one by 04:12 UT.

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

Detected by halocme, Submitted at 2012-01-26T23:02:32

2012-01-22T21:00:36 --> 2012-01-23T00:00:36

Again, the movie shows downflows more than the eruption. But this is associated with a slow CME observed by LASCO.

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

Detected by halocme, Submitted at 2012-01-26T22:53:34

2012-01-22T13:40:12 --> 2012-01-22T16:40:12

The movie gives an impression that the filament material just comes back to the Sun, but some of it may have escaped into the heliosphere. The surrounding large-scale loops at 193 A and 171 A seem to be largely unaffected.

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

Detected by halocme, Submitted at 2012-01-26T22:34:06

2012-01-22T12:20:24 --> 2012-01-22T14:00:24

There are two locations that show upward, then downward motions nearly simultaneously. They may be classified in a better way than coronal jets.

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

Detected by halocme, Submitted at 2012-01-26T22:15:49

2012-01-22T08:00:04 --> 2012-01-22T11:00:04

A non-eruptive flare appears to trigger an eruptive one to the east. No clear filament is seen in the eruption, which is mostly horizontal, toward east.

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

Detected by halocme, Submitted at 2012-01-26T02:40:54

2012-01-22T02:15:00 --> 2012-01-22T06:15:00

These motions are most readily seen at 304 A, with the large-scale structures in 211 A and 171 A hardly affected. This results in a slow CME that contains a flux rope.

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

Detected by halocme, Submitted at 2012-01-26T02:20:58

2012-01-22T02:30:00 --> 2012-01-22T03:32:00

This eruption seems to be so minor that the surrounding large-scale structures are hardly disturbed.

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

Detected by halocme, Submitted at 2012-01-26T02:13:09

2012-01-21T18:00:04 --> 2012-01-22T03:30:04

The motions appear to intensify during this period, although the filament itself does not erupt.

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

Detected by berger, Submitted at 2012-01-20T22:13:50

2012-01-17T20:00:04 --> 2012-01-18T05:00:04

This is the same cavity noted on 15-Jan-2012 but with a better line of sight and with a much brighter central "chewy nougat" emission region. The associated quiescent prominence is quite dynamic in the 304 channel. 171 structure is weak however and does not show typical "horn" protrusions into the cavity.

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

Detected by berger, Submitted at 2012-01-20T00:28:19

2012-01-14T00:00:04 --> 2012-01-14T11:00:04

Ephemeral active region emerges in southern end of the large transequatorial coronal hole.

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

Detected by berger, Submitted at 2012-01-19T23:26:40

2012-01-14T19:45:04 --> 2012-01-15T00:00:04

Confined eruption from small active region bowls over a nearby filament, vaporizing it in the process. The vaporized filament detritus appears to spiral northward before crashing into the chromosphere in several disparate locations.

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

Detected by berger, Submitted at 2012-01-19T22:44:58

2012-01-13T00:00:04 --> 2012-01-14T00:00:04

Moderate coronal rain event from active region behind W limb.

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

Detected by berger, Submitted at 2012-01-19T22:34:34

2012-01-13T04:30:04 --> 2012-01-14T00:00:04

Moderate sized flux emergerence event in plage.

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

Detected by berger, Submitted at 2012-01-19T22:31:44

2012-01-13T00:00:04 --> 2012-01-14T00:00:04

Large filament in NW activates and shows large counterstreaming flows with brightening in 304.