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

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

Detected by phiggins, Submitted at 2013-07-24T16:32:13

2013-07-22T00:00:03 --> 2013-07-22T10:00:03

AR 11801 emerging over the East limb. The occurrence of rapid loop reconfiguration and chromospheric mass injection into the corona is evident.

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

Detected by phiggins, Submitted at 2013-07-24T16:24:31

2013-07-22T00:00:03 --> 2013-07-22T07:25:03

Behind-the-limb surge of filament material poleward.

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

Detected by phiggins, Submitted at 2013-07-23T17:54:07

2013-07-21T17:45:04 --> 2013-07-22T06:50:04

Diffuse over-lying loops to the north east move north-west, and this is followed by a localised brightening in the center north region of the FOV. A reconnection/reconfiguration front moves west. and then south, curving around the large filament in the center-south of the field of view.

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

Detected by phiggins, Submitted at 2013-07-23T17:35:59

2013-07-21T14:40:03 --> 2013-07-21T15:50:03

Two coronal jets occur at the same time. Probably confined to the two legs of a bipolar loop structure..

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

Detected by phiggins, Submitted at 2013-07-23T17:31:18

2013-07-21T13:20:03 --> 2013-07-22T03:40:03

Swirling material within a quiescent filament. Turbuklent vortex? Complex filament magnetic field?

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

Detected by phiggins, Submitted at 2013-07-23T17:05:26

2013-07-21T20:30:03 --> 2013-07-21T22:38:03

The same filament lift-off as before, but showing the cooler chromaspheric component in comparison with the hotter coronal component. The material seems to be quite diffuse, with the majority of the plane-of-sky area of the eruption being the hotter component. Perhaps this is why the erupting material seems to buoyant. The eruption is rapid and very little falls back to the surface.

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

Detected by phiggins, Submitted at 2013-07-23T16:50:51

2013-07-21T20:50:03 --> 2013-07-21T22:25:03

A possible polar-crown filament lift off at a near-perfect north-ward trajectory. The event likely occurred well beyond the West limb at >45deg latitude. There does not appear to be any pole-ward deflection, but this may be a LOS effect. There appears to be a large cavity-like structure in the coronal region where the eruption took place. This may have allowed the eruption to exhibit the uncommon trajectory.

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

Detected by derosa, Submitted at 2013-07-22T18:10:52

2013-07-20T12:00:03 --> 2013-07-20T15:00:03

Nice example of coronal cells (see Sheeley & Warren 2012 ApJ 749 40) located between a coroanl hole and a large north-south filament. Sheeley et al (2013 ApJ 772 88) argue that the direction of the horizontal field along the filament channel can be inferred by the properties of these coronal cells.

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

Detected by phiggins, Submitted at 2013-07-22T17:22:59

2013-07-21T00:00:03 --> 2013-07-21T10:10:03

Localised rotating helical sructures at the south pole. The central 3 tornadoes interact with each other. The middle one twists about the east one, and then after a time moves to twist about the west one.

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

Detected by phiggins, Submitted at 2013-07-22T17:14:26

2013-07-21T00:00:03 --> 2013-07-21T11:30:03

A prominence becomes unstable and partially erupts. Some of the material is flung southward on large overlying loops. Another portion moves northward and enters a bipolar loop, which first beightens at the loop-tops, possibly reconnecting with an overlying loop top. A current-sheet-like structure forms in a localised area at the loop top, appearing like a 'tri-corn' (see 'isle of man' flag). Material then is propelled down the legs of the loops.

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

Detected by phiggins, Submitted at 2013-07-22T16:57:14

2013-07-21T03:20:03 --> 2013-07-21T14:30:03

A C3.1 flare followed by a primarily northward-moving reconnection front, and the formation of an extended coronal dimming region and a post flare loop arcade. A small sympathetic eruption occurs to the south-east after the flare.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:2

Detected by anny, Submitted at 2013-07-19T21:34:52

2013-07-03T05:33:03 --> 2013-07-03T07:48:03

An eruption of part of a flux rope on the NW disk, with associated post-eruption arcade and coronal dimming. Note that there is a small prominence eruption at the nearby limb, which seems to start and end at the same time as the eruption on the disk.

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

Detected by anny, Submitted at 2013-07-19T21:34:51

2013-07-03T05:33:03 --> 2013-07-03T07:48:03

An eruption of part of a flux rope on the NW disk, with associated post-eruption arcade and coronal dimming. Note that there is a small prominence eruption at the nearby limb, which seems to start and end at the same time as the eruption on the disk.

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

Detected by phiggins, Submitted at 2013-07-19T20:44:29

2013-07-18T00:00:00 --> 2013-07-18T06:00:00

A series of intensifying jets at the on the NW limb is followed by a moderate flare (in 304A). The flare is perhaps triggered by the jets. The directionality of the jets is ~10 deg. northward of radial.

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

Detected by anny, Submitted at 2013-07-19T00:12:42

2013-07-02T17:12:35 --> 2013-07-02T18:27:35

This C-class flare has produced a pretty substantial diffraction pattern in 304A. The is no associated substantial brightening in 171A or in 211A.

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

Detected by anny, Submitted at 2013-07-18T23:47:14

2013-07-02T06:10:35 --> 2013-07-02T11:15:35

An eruption-like activity with following dimming and post-eruption arcade footpoint brightening, however, I have a hard time seeing the erupting structure itself.

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

Detected by anny, Submitted at 2013-07-18T23:45:03

2013-07-02T00:00:35 --> 2013-07-02T02:55:35

A pretty sigmoid eruption on the N disk.

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

Detected by weiliu, Submitted at 2013-07-18T18:09:20

2013-07-13T05:40:03 --> 2013-07-13T07:20:03

A prominence attempts to erupt but most of its material falls back.

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

Detected by cheung, Submitted at 2013-07-12T23:28:39

2013-07-09T14:00:03 --> 2013-07-09T18:10:03

A filament above a sheared PIL (far away from active regions) is activaetd. Any material that appears to have been accelerated is confined to the enclosed flux system.

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

Detected by anny, Submitted at 2013-07-02T20:22:57

2013-06-30T18:00:03 --> 2013-07-01T04:00:03

A large scale but extremely hard to see filament eruption on the SE disk/limb.