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

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

Detected by cheung, Submitted at 2013-02-13T00:37:58

2013-02-11T21:20:03 --> 2013-02-12T00:20:03

The eruption seems to impulsively generate a shock that propagats ahead of the rising filamentary material.

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

Detected by cheung, Submitted at 2013-02-13T00:37:56

2013-02-11T21:20:03 --> 2013-02-12T00:20:03

The eruption seems to impulsively generate a shock that propagats ahead of the rising filamentary material.

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

Detected by cheung, Submitted at 2013-02-13T00:26:55

2013-02-11T02:00:03 --> 2013-02-11T04:30:03

A gentle filament ejection that takes place over the course of two hours.

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

Detected by anny, Submitted at 2013-02-07T22:55:24

2013-02-05T18:15:03 --> 2013-02-06T00:00:03

This filament appears to make a full circle around a unipolar patch on the quiet sun.

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

Detected by halocme, Submitted at 2013-01-24T20:40:24

2013-01-23T11:00:03 --> 2013-01-23T16:00:03

It is straightforward to link this filament eruption with the partial halo CME observed by LASCO. The fine structure of the associated chromospheric brightening (not even making it to a GOES B-class flare) may reflect the complexity of the magnetic field structure.

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

Detected by cheung, Submitted at 2013-01-23T18:46:34

2013-01-23T02:50:03 --> 2013-01-23T04:50:03

The timing of these loop motions in the AR in the northern hemisphere is suggestive of a connection with the filament eruption that is synchronously occuring in the southern hemisphere. This may just be a coincidence. In any case, global evolutionary models of the coronal magnetic field will likely be necessary to (in)validate this tentative connection.

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

Detected by cheung, Submitted at 2013-01-23T18:33:42

2013-01-23T08:30:03 --> 2013-01-23T10:50:03

This filament activation occured following the second large filament eruption to originate from this region in the previous 36 hours. Sympathetic events?

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

Detected by anny, Submitted at 2013-01-22T00:33:36

2013-01-19T12:30:03 --> 2013-01-19T14:21:03

This vent in AR at the W limb possible resembles a spray surge, except that it appears to stay close to the surface.

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

Detected by anny, Submitted at 2013-01-21T20:57:42

2013-01-19T09:45:03 --> 2013-01-19T13:09:03

A site of a slowly pouring coronal rain pours down more plasma as a massive filament eruption passes by.

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

Detected by anny, Submitted at 2013-01-21T20:47:42

2013-01-19T09:45:03 --> 2013-01-19T13:09:03

A massive filament eruption on the E disk. Note the twisted structure ad how the remnant of the filament flows northwards towards a nearby active region.

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

Detected by halocme, Submitted at 2013-01-12T18:38:21

2013-01-11T08:30:35 --> 2013-01-11T10:10:35

Although the front is not clear, there is certainly a large scale propagation of disturbances associated with the M1.3 flare. The propagation seems to follow the onset of the associated filament eruption.

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

Detected by halocme, Submitted at 2013-01-12T18:04:56

2013-01-06T06:15:35 --> 2013-01-06T07:15:35

This event, associated with a C1.0 flare, came from the region west of the one that produced the previous minor wave. Even though this wave is faint, it appears less constrained thann the previous one.

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

Detected by anny, Submitted at 2013-01-10T02:54:07

2013-01-09T10:03:03 --> 2013-01-09T16:33:03

A rapid eruption, best seen in 171A, unleashes a sall coronal wave (211A). At the same time, there is a slow prominence eruption (annotated earlier) in where the wave passed by. It is not clear whether these two events are connected or influence one another.

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

Detected by anny, Submitted at 2013-01-10T02:48:05

2013-01-09T22:39:03 --> 2013-01-09T23:00:03

A flare (in the sense that it produced a diffraction pattern, it wasn't registered by GOES) on the W limb throws a small blob upwards. This blob is very bright and it trabels unusually fast. After going past the overlying loop bundle, it rapidly slows down and disappears. There is an associated cavity eruption visible in 211 channel. The 171 channel shows how does this feature travel past the overlying loop bundle: it clearlys get disturbed by the passing feature but soon regains its shape and position.

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

Detected by anny, Submitted at 2013-01-10T02:48:03

2013-01-09T22:39:03 --> 2013-01-09T23:00:03

A flare (in the sense that it produced a diffraction pattern, it wasn't registered by GOES) on the W limb throws a small blob upwards. This blob is very bright and it trabels unusually fast. After going past the overlying loop bundle, it rapidly slows down and disappears. There is an associated cavity eruption visible in 211 channel. The 171 channel shows how does this feature travel past the overlying loop bundle: it clearlys get disturbed by the passing feature but soon regains its shape and position.

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

Detected by anny, Submitted at 2013-01-10T02:26:01

2013-01-09T01:00:03 --> 2013-01-09T08:12:03

A massive prominence lifts off on the SW limb. Most of it falls to a distant location as coronal rain, and there is a small blob which leaves the field of view in the SW direction. I am not sure whether to classify this event as a filament activation or a minor eruption so I mark it as both. It is definitely a beautiful event.

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

Detected by halocme, Submitted at 2013-01-09T07:38:41

2012-05-26T20:20:24 --> 2012-05-26T21:20:24

Strong wave from a region 30 degrees behind the limb that is still visible from Earth.

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

Detected by halocme, Submitted at 2013-01-09T07:23:24

2012-07-02T10:30:00 --> 2012-07-02T12:00:00

Although not as spectacular as the filament eruption that fully develops after 11 UT, we can certainly find a coronal wave or propagating front in this movie (10:46-10:55) disturbing the high latiyude region close to the south pole.

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

Detected by anny, Submitted at 2013-01-09T01:05:50

2013-01-07T05:00:03 --> 2013-01-07T13:12:03

Massive eruption at the SW limb. I think it should be named the "Julian Christmas" eruption. Note the abrupt radial edge of the part of the filament which falls back down after the eruption.

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

Detected by halocme, Submitted at 2013-01-04T21:06:58

2013-01-03T19:10:11 --> 2013-01-03T21:10:11

The small filament eruption results in a two-ribbon flares and dimming at high altitudes.