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

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2012-11-09T00:45:28

2012-11-06T06:52:03 --> 2012-11-06T12:48:03

Above a small AR at the W limb, a field configuration appears to 'roll' as it moves upward, with emission first dropping, then recovering.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2012-11-09T00:42:52

2012-11-06T00:00:03 --> 2012-11-06T02:16:03

Strong eruption from small bipole, with assiated 'dimming' and field oscillations.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2012-11-06T19:10:45

2012-11-04T13:21:03 --> 2012-11-06T00:00:03

Emergence of moderate AR

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2012-11-02T01:22:21

2012-10-30T04:00:03 --> 2012-10-30T13:55:03

Half of a large filament seems to disappear, while the other half is not noticably affected.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2012-10-17T01:04:45

2012-10-15T10:20:03 --> 2012-10-15T20:20:03

A particularly clear example of coronal rain. It is followed by eruption and brightening of 171A loops. Note the large jet-like configuration on the bottom of the S edge of the highlighted AR.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2012-10-04T22:58:11

2012-10-04T05:48:12 --> 2012-10-04T08:24:12

An eruption from a very compact region near DC appears related to one seen above the NW limb over a region already beyond the limb.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2012-09-21T22:49:53

2012-09-16T09:40:03 --> 2012-09-16T10:40:03

In 304 (orange), much of the material lifted in this surge can be seen to drain back down. In 171 (green), one finds a faint puff that ascends (on top of the 304 material) the magnetic chimney but never falls.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2012-09-12T02:54:29

2012-09-10T07:28:03 --> 2012-09-10T14:46:03

A very spectacular coronal rain, large enough to be possibly called "coronal implosion"

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2012-09-12T02:24:12

2012-09-09T17:26:03 --> 2012-09-09T19:56:03

Eruption of a small flux rope causes distant footpoint-like brightening, which is suggestive of that it broke throuth an arcade connecting to the region of the brightening. But there is another filament between the eruption and the footpoint brightening, and the reconnection in the overlying arcade does not seem to cause any disturbance to this second filament.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2012-09-06T00:28:53

2012-09-04T22:04:35 --> 2012-09-05T03:16:35

Polar-crown filament eruption

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2012-08-22T01:10:06

2012-08-17T20:15:03 --> 2012-08-18T02:40:03

A close-up view on the site of the filament eruption. Despite quite spectacular foorpoint brightening, little of the flux rope is seen erupting until the later stages when it takes off from the field of view (dark feature travelling towards the top left corner).

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2012-08-22T01:00:51

2012-08-17T20:25:03 --> 2012-08-18T09:00:03

The filament itself is not visible well until the last stages of the eruption, hovewer, the post-eruption brightening is quite spectacular in all channels.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2012-08-21T23:29:13

2012-08-17T20:30:03 --> 2012-08-18T09:00:03

Spray surges seem to be repetitively happening in the same location. What is going on there?

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2012-08-21T23:08:27

2012-08-16T17:25:03 --> 2012-08-16T19:45:03

The overlying structure which shows in 304 (but not in 211 or 171) is suggestive of that the erupting structure is much thicker than the filament itself, and that the filament resides at its bottom. The cavity does not appear like a sphere, more like a thicker "shell" around the erupting flux rope. It is an interesting observation as I do not recall observing the signature of the top of the cavity that clearly in 304A and not in other channels.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2012-08-17T01:01:59

2012-08-15T01:40:04 --> 2012-08-15T09:20:04

The loops associated with AR 11540 near the limb brightened at about the time that the eruption from AR 11543 took place. Following the loop brightenings once finds the appearance of new coronal condensations draining from the bright loops.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2012-08-17T01:01:58

2012-08-15T01:40:04 --> 2012-08-15T09:20:04

The loops associated with AR 11540 near the limb brightened at about the time that the eruption from AR 11543 took place. Following the loop brightenings once finds the appearance of new coronal condensations draining from the bright loops.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2012-08-14T00:26:06

2012-08-11T10:30:04 --> 2012-08-11T11:45:04

This polar filament was in the process of lifting off when this eruption from the lower latitudes took place. It's unclear whether there is connection between the two.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2012-08-14T00:26:03

2012-08-11T10:30:04 --> 2012-08-11T11:45:04

This polar filament was in the process of lifting off when this eruption from the lower latitudes took place. It's unclear whether there is connection between the two.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2012-08-10T18:07:00

2012-08-09T19:40:04 --> 2012-08-10T00:00:04

A filament from a compact AR destabilizes and erupts, with some twisting motion, in what appears to be the start of a CME.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2012-08-10T18:03:52

2012-08-09T16:36:04 --> 2012-08-09T21:00:04

An eruption from what looks like a compact bipole on the side of a larger AR sends a perturbation front across QS loops towards the W and NW.