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

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

Detected by schryver, Submitted at 2013-08-07T22:00:33

2013-08-06T01:16:03 --> 2013-08-06T05:24:03

QS filament eruption with distant, over-the-limb coronal oscillations towards the NE.

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

Detected by halocme, Submitted at 2013-08-06T22:04:40

2013-08-05T23:00:03 --> 2013-08-06T00:10:03

This may present a border line between eruption and loop expansion. Dimming is clearly observed in association with the outward motion. However, no CME results from this action in the low corona.

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

Detected by halocme, Submitted at 2013-08-06T21:57:46

2013-08-05T22:00:03 --> 2013-08-05T23:10:03

The movie gives an impression that reconnection at low altitudes push matrial upward. The curved trajectory may imply that the jet traces closed field lines.

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

Detected by halocme, Submitted at 2013-08-06T21:36:59

2013-08-05T13:30:35 --> 2013-08-05T15:00:35

This surge may be of chromspheric to transition region temperature since it appers bright in 304 A and dark in 211 A images. Changes at the footpoint region do not appar to be very dynamic.

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

Detected by halocme, Submitted at 2013-08-06T21:21:08

2013-08-05T13:50:23 --> 2013-08-05T15:20:23

The prominence eruption is probably from the back side. It clearly fails to break into interplanetary space (no CME), which is partly understood by noticing that there is no dimming in the background structure. Unlike other well-known examples, this eruption is not reminiscent of kink instability.

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

Detected by halocme, Submitted at 2013-08-06T21:13:36

2013-08-05T04:55:11 --> 2013-08-05T05:55:11

The jet itself is quite diffuse, but it can still be seen both on disk and over the limb. This event is characterized in dynamic changes at the footpoints, possibly with field line mixing.

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

Detected by halocme, Submitted at 2013-08-06T21:04:24

2013-08-05T01:10:11 --> 2013-08-05T03:50:11

This erption appears to originate on the viisble side because we can identify both legs. The prominence is in the same line of sight as the cavity seen in 211 A images, but they seem to be not related. The eruption is so minor that there are no coronagraphic consequences.

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

Detected by halocme, Submitted at 2013-08-06T20:51:29

2013-08-05T01:10:11 --> 2013-08-05T02:20:11

A minor eruption in the southern region seems to start as the material ejected in the norther region arrives. This seems to be a clear case of remote trigger of an eruption.

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

Detected by halocme, Submitted at 2013-08-06T20:35:20

2013-08-04T22:10:11 --> 2013-08-04T23:50:11

The core part is seen to form, then to erupt between 22:52 UT and 22:54 UT, leaving a deep, although compact, dimming area. The white-light coronagraph manifestation is hardly a CME, which may be better called an outflow.

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

Detected by halocme, Submitted at 2013-08-06T20:24:14

2013-08-04T14:30:35 --> 2013-08-04T16:00:35

Although the eruption itself is minor, it produces a ribbon-like emission at footpoints. Besides the eruption, the filament mateiral is seen to escape sideway to north. The associated small CME in LASCO data shows closed loops following a spiky structure.

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

Detected by halocme, Submitted at 2013-08-06T19:47:36

2013-08-04T09:10:11 --> 2013-08-04T11:00:11

The eruption may be recognized only in the dimming above closed loops. No filament material is seen ejected. The even smaller eruption in northwest may not be related, since it is seen after this eruption over the limb.

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

Detected by halocme, Submitted at 2013-08-06T18:14:32

2013-08-04T06:15:35 --> 2013-08-04T07:45:35

This may look like a failed eruption. The filament does not appear to escape. However, a CME is observed by LASCO, not very impressive but not too wimpy either. Difference images in 211 A /193 A indicate some minor dimming.

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

Detected by halocme, Submitted at 2013-08-06T17:53:51

2013-08-04T05:20:23 --> 2013-08-04T06:50:23

A small prominence eruption followed by dimming in overlying structures. This is too minor to be observed later by LASCO. There is hardly a twist in the prominence and untwisting motion on the eruption.

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

Detected by halocme, Submitted at 2013-08-06T16:50:50

2013-08-03T20:20:23 --> 2013-08-03T21:30:23

This ejection is the brightest in 304 A images. It is deflected northward, presumably reflecting the open field topology. The closed loops, most pronounced in 171 A images, are not affected presumably because they just happen to be in the same line of sight.

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

Detected by halocme, Submitted at 2013-08-06T16:38:05

2013-08-03T17:30:35 --> 2013-08-03T18:30:35

A small prominence eruption is seen in 304 A images. This gives an impression of pushing surrounding open structrures aside as seen in 211 A and 171 A images. The event may be considered to be a jet, suggesting that jets and eruptions are similar after all.

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

Detected by halocme, Submitted at 2013-08-06T16:19:53

2013-08-03T05:40:11 --> 2013-08-03T06:30:11

The footpoint seems to brighten to a B1.5 level. The jet is curved, probably tracing the coronal magnetic field lines.

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

Detected by phiggins, Submitted at 2013-07-30T23:08:20

2013-07-30T00:35:03 --> 2013-07-30T14:00:03

A series of surges propagate from the corona (overarching loops) off the W-limb. The source of the material is not obvious. The material appears to be pouring from 'thin air' and falling along the loop legs. Perhaps the material was previously cool (dark in 304), and behind the visible loops and heats up as it falls around the front of the loops, becoming visible.

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

Detected by phiggins, Submitted at 2013-07-30T22:56:25

2013-07-29T22:10:03 --> 2013-07-30T00:35:03

A prominence appears to become kink-unstable. This leads to a rapid outward motion and then dissappearance of the prominence. The coronal loop structure surrounding the promenence dissappears as well, and a radial coronal cavity forms, with radial streamer-like structures moving north and south, away from the prominence's original position.

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

Detected by phiggins, Submitted at 2013-07-30T22:34:55

2013-07-29T12:10:03 --> 2013-07-29T19:45:03

This event is very similar to both SOL2013-07-25T00:55:03L141C087 and SOL2013-07-26T20:00:03L138C083 A flare occurres in the region at the SE of the FOV. A coronal dimming and surge-like disturbance then propagate north-ward. Like the event on the 25th, the 304 emission appeared diffuse. The event on the 26th appeared much brighter. These three similar events along the same filament channel appear to indicate that the same unstable magnetic configuration was reformed after each occurrence.

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

Detected by phiggins, Submitted at 2013-07-29T22:14:05

2013-07-29T01:50:03 --> 2013-07-29T08:50:03

A swirling filament appears quiescent and dark in 304A, until an arcade of loops rapidly forms behind the E-limb, causing the filament material to flow along an overarching filament structure appearing bright in 304. Then both the original filament and the arcade recede and vanish.