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 2013-09-14T16:40:46

2013-09-13T14:00:03 --> 2013-09-13T21:00:03

The slow ascent of the prominence had started before 14 UT. It is hard to link this eruption with the filaments lying on the visible disk. The associated CME, which was first found around 19 UT in LASCO C2 data, was quite major in the sense that it was still visible at the southern or souteastern limit of C3 data.

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

Detected by halocme, Submitted at 2013-09-13T23:16:53

2013-09-12T17:30:35 --> 2013-09-12T19:00:35

This appears in depression in 211 A and 193 A images. The western footpoint brightens nearly simultaneously with the outflow.

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

Detected by halocme, Submitted at 2013-09-13T23:03:03

2013-09-12T17:00:03 --> 2013-09-13T00:00:03

The outward motion (in 304 A) to northwast between 22:30 and 23:30 UT is reminiscent of the quasi-periodic fast propagating wave usually seen in 171 A images (Wei Liu et al. ApJL, 736, L13, 2011). This is long after the associated CME takes off (some time between 18 UT and 19 UT as seen in 211 A over the limb). The white-light appearance of the CME is somewhat complex, not going through gradual to sudden acceleration.

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

Detected by halocme, Submitted at 2013-09-13T22:37:13

2013-09-11T12:00:03 --> 2013-09-11T21:42:03

LASCO C2 data show a flux-rope-like feature around 17 UT with closed loops ahead. The CME becomes obvious only around 21 UT. Although it is possible that this is a deeply occulted event, the hesitant motions of the prominence may represent the low coronal manifestations of the CME, which is more clearly seen to form at higher altitudes.

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

Detected by halocme, Submitted at 2013-09-13T16:57:11

2013-09-11T08:00:03 --> 2013-09-11T10:00:03

The untwisting is more readily seen in the southern leg. There is clear connection of the northern leg with the filement (channel) on the visible side. The eruption drives a decent CME that is first seen by LASCO C2 at 09:24 UT and traceable to the edge og C3 (around 19 UT).

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

Detected by derosa, Submitted at 2013-09-11T17:32:36

2013-09-04T20:00:03 --> 2013-09-05T00:00:03

Filament from an off-limb active region shows a lot of dynamics involving both colder filament material and warmer coronal loop structures.

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

Detected by derosa, Submitted at 2013-09-11T17:32:33

2013-09-04T20:00:03 --> 2013-09-05T00:00:03

Filament from an off-limb active region shows a lot of dynamics involving both colder filament material and warmer coronal loop structures.

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

Detected by anny, Submitted at 2013-09-10T01:49:24

2013-09-05T17:28:03 --> 2013-09-05T19:36:03

A blob of plasma emitting in 304A jumps upwards, then falls back down. The 211A loops open up in the jumping phase, but do not close back in when the blob sinks down.

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

Detected by anny, Submitted at 2013-09-10T00:58:27

2013-09-05T09:50:03 --> 2013-09-05T14:32:03

A northward eruption with a very slow onset at the NW limb.

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

Detected by weiliu, Submitted at 2013-09-03T20:33:49

2013-07-13T08:30:03 --> 2013-07-13T19:30:03

Recurrent small-scale surges from an active region on the west limb, repeated over the course of about 10 hours.

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

Detected by weiliu, Submitted at 2013-09-03T20:22:39

2013-07-13T00:00:03 --> 2013-07-14T00:00:03

A large prominence at high latitudes near the south pole.

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

Detected by phiggins, Submitted at 2013-09-03T18:13:11

2013-09-02T05:40:03 --> 2013-09-02T13:40:03

Prominence material becomes unstable and partially erupts. As it does, it becomes trapped on open field lines and appears to flow back to the surface.

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

Detected by phiggins, Submitted at 2013-09-03T18:09:08

2013-09-02T06:40:03 --> 2013-09-02T07:35:03

an eclipse

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

Detected by phiggins, Submitted at 2013-09-03T18:06:12

2013-09-01T19:45:03 --> 2013-09-02T06:30:03

Avery faint filament erupts rapidly off the south limb, and shows no apparent coronal signature.

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

Detected by phiggins, Submitted at 2013-09-03T18:01:39

2013-09-01T14:15:03 --> 2013-09-01T18:45:03

A surge of filament material off the W-limb, oriented S-ward into an arc back to the surface. The filament material is threaded by coronal structures.

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

Detected by phiggins, Submitted at 2013-09-03T17:57:18

2013-08-31T00:00:03 --> 2013-08-31T19:20:03

A radial oriented prominence appears suspended by horizontal loop structures that kinks into a V-shape at the location of the intersection (possibly pulled down by the weight of the prominence material like a slingshot). A connected filament then lifts off and is siphoned into the region of horizontal structures.

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

Detected by phiggins, Submitted at 2013-09-03T17:48:40

2013-08-31T13:45:03 --> 2013-09-01T12:00:03

Large transeqatorial loops form over the E-limb. The souther foot points may be an extended plage region, as the main AR loops do not appear affected. The north foot points appear to be within a bipolar region, as lower lying loops become distorted.

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

Detected by phiggins, Submitted at 2013-09-03T17:43:19

2013-08-31T17:20:03 --> 2013-09-01T08:30:03

A filament in the S-W quadrant partially erupts and some of the material is trapped and suspanded abover the region, and then siphoned back down to the surface away from the eruption site along other over-arching loops

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

Detected by phiggins, Submitted at 2013-09-03T17:37:15

2013-08-30T22:10:03 --> 2013-08-31T03:40:03

An extended surge event occurs, rooted in a W-limb AR. The surge propagates S-ward and retreats back the way it came. The filament material leaves a wake of emission, visible in 171A, as it retreats.

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

Detected by phiggins, Submitted at 2013-09-03T17:31:37

2013-08-30T13:05:03 --> 2013-08-31T04:00:03

A prominence becomes unstable and appears to be partially siphoned up into a coronal V-loop structure which also lifts off along radial streamer-like structures visible in 171A and 211A.