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 2013-10-16T23:14:33

2013-10-15T00:00:03 --> 2013-10-16T03:00:03

Smallish active regions and their surroundings exhibit multiple eruptions and flares (high-C and low-M) as activity couples from one region into another, including high over the SW limb.

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

Detected by halocme, Submitted at 2013-10-16T02:44:56

2013-10-13T00:00:03 --> 2013-10-13T02:30:03

This eruption is associated with a halo CME observed by LASCO. The front does not appear sharp, and it becomes clear only far from the flare location.

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

Detected by halocme, Submitted at 2013-10-15T21:37:31

2013-10-12T14:00:07 --> 2013-10-12T16:30:07

A local erupting plasma interacted with large-scale field that was highly non-radial. The multiplicity of the jet may reflect interactions with adjacent and similarly oriented field.

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

Detected by anny, Submitted at 2013-10-11T21:50:12

2013-10-06T18:06:03 --> 2013-10-06T23:03:03

Two small prominences and the associated cavities erupt almost simultaneously. Can these be different parts of the same erupted structure? The event is followed by some reconfiguration of loops in an active region between the sites of the eruptions.

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

Detected by halocme, Submitted at 2013-10-11T16:57:43

2013-10-11T07:00:07 --> 2013-10-11T09:00:07

The front is seen mostly along the limb (largely counterclockwise), although we also note disturbances on disk. The flare region seems to be slightly behind the limb. Empirically, a LCPF and eruption of this scale (including oscillations of trans-equatorial loops) accompanies a fast and wide CME, although no LASCO data are seen for this event as of now thanks to the government shutdown.

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

Detected by halocme, Submitted at 2013-10-11T16:57:41

2013-10-11T07:00:07 --> 2013-10-11T09:00:07

The front is seen mostly along the limb (largely counterclockwise), although we also note disturbances on disk. The flare region seems to be slightly behind the limb. Empirically, a LCPF and eruption of this scale (including oscillations of trans-equatorial loops) accompanies a fast and wide CME, although no LASCO data are seen for this event as of now thanks to the government shutdown.

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

Detected by halocme, Submitted at 2013-10-07T15:12:17

2013-10-05T04:00:03 --> 2013-10-05T08:00:03

The eruptive signatures are clearly noted in AIA images even though the source region is estimated to be more than 30 degrees behind the limb. The event is associated with a type II radio burst (both metric and DH), and a halo CME. Based on the LASCO MVI files archived at NRL (no movies available at GSFC because of the goverment shutdown), the bright CME is first observed at 07:10 (at the heliocentric distance of 2.8-2.9 Rs and PA of 125 deg), and the linear speed is only about 630 km/s using five difference images.

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

Detected by schryver, Submitted at 2013-09-25T21:13:03

2013-09-24T18:36:03 --> 2013-09-25T00:00:03

A quiet-Sun filament/prominence erupts over the NE limb, with prominent post-eruption emission following ribbon expansion.

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

Detected by cheung, Submitted at 2013-09-21T00:32:16

2013-09-18T16:30:03 --> 2013-09-18T22:00:03

A quiescent filament is swishing back and forth while some eruption gives ejected plasma a rollercoaster ride.

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

Detected by cheung, Submitted at 2013-09-21T00:27:29

2013-09-19T02:10:03 --> 2013-09-19T04:30:03

A confined eruption occurs from behind the limb (since there are no clearly illuminated on-disk footpoints). There is some cusp/dome structure in the foreground with loops clearly delineated with filament material (perhaps near a qsl?).

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

Detected by cheung, Submitted at 2013-09-21T00:27:27

2013-09-19T02:10:03 --> 2013-09-19T04:30:03

A confined eruption occurs from behind the limb (since there are no clearly illuminated on-disk footpoints). There is some cusp/dome structure in the foreground with loops clearly delineated with filament material (perhaps near a qsl?).

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

Detected by cheung, Submitted at 2013-09-21T00:27:25

2013-09-19T02:10:03 --> 2013-09-19T04:30:03

A confined eruption occurs from behind the limb (since there are no clearly illuminated on-disk footpoints). There is some cusp/dome structure in the foreground with loops clearly delineated with filament material (perhaps near a qsl?).

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

Detected by cheung, Submitted at 2013-09-17T00:18:23

2013-09-15T09:00:03 --> 2013-09-15T14:40:03

Some of the material seems to drain back down to one leg of the filament.

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

Detected by schryver, Submitted at 2013-08-20T18:26:18

2013-08-20T03:44:03 --> 2013-08-20T12:44:03

An AR at the W limb erupts (with some oscillatory motions high in the corona), upon which a long quiet-Sun (near polar-crown) filament erupts on the S hemisphere. The timing is suggestive of a sympathetic set of events, but direct evidence is not obvious.

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

Detected by schryver, Submitted at 2013-08-20T18:26:12

2013-08-20T03:44:03 --> 2013-08-20T12:44:03

An AR at the W limb erupts (with some oscillatory motions high in the corona), upon which a long quiet-Sun (near polar-crown) filament erupts on the S hemisphere. The timing is suggestive of a sympathetic set of events, but direct evidence is not obvious.

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

Detected by schryver, Submitted at 2013-08-19T17:37:57

2013-08-18T19:44:03 --> 2013-08-18T22:36:03

A high coronal - over the W limb - eruption is followed by the eruption of an adjacent filament (with a propagating front) and the beginnings of a filament activation trailing into QS.

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

Detected by halocme, Submitted at 2013-08-16T00:20:33

2013-08-14T18:30:35 --> 2013-08-14T23:30:35

The presence of the filament is noted in all of the 304, 211 and 171 A channels. Eruption of such a filament indeed results in a decent three-part CME in LASCO data.

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

Detected by anny, Submitted at 2013-08-14T00:34:22

2013-08-02T12:18:03 --> 2013-08-02T15:38:03

A filament erupts on the SW disk. Its northern end has a nice "swirl" shape. Post-eruption arcade follows.

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

Detected by halocme, Submitted at 2013-08-05T17:54:01

2013-08-03T02:00:35 --> 2013-08-03T12:00:35

Although the origin of this activity is TBD, it may reperesent at least part of the diffuse, slow and long-lasting outflow (and yet containing a flux-rope-like feature) in LASCO data. The prominence can be tracked in AIA data roughly between 03 UT and 08 UT, most notably in 171 A.

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

Detected by anny, Submitted at 2013-07-22T20:04:36

2013-07-18T19:39:03 --> 2013-07-19T00:00:03

Large prominence eruption on the W limb.