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 2013-10-16T02:28:50

2013-10-13T10:30:35 --> 2013-10-13T16:00:35

Mass is seen to move from one leg to another of the prominence. These motions may underlie an eruption. But the overlying corona does not seem to be affected. The possibly associated CME is narrow.

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

Detected by halocme, Submitted at 2013-10-16T02:14:48

2013-10-13T08:00:03 --> 2013-10-13T09:00:03

Although flare ribbons and dimming are seen, this seems to be a failed eruption.

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

Detected by halocme, Submitted at 2013-10-16T02:14:45

2013-10-13T08:00:03 --> 2013-10-13T09:00:03

Although flare ribbons and dimming are seen, this seems to be a failed eruption.

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

Detected by halocme, Submitted at 2013-10-16T02:08:44

2013-10-13T06:45:35 --> 2013-10-13T08:25:11

The bright prominence is seen to push overlying structures into a large eruption, although CME association is unclear due to LASCO data gap and to a prior halo event. STEREO-B data show that the source region is about 10 degrees behind the limb and that it is not an active region.

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

Detected by halocme, Submitted at 2013-10-16T02:08:42

2013-10-13T06:45:35 --> 2013-10-13T08:25:11

The bright prominence is seen to push overlying structures into a large eruption, although CME association is unclear due to LASCO data gap and to a prior halo event. STEREO-B data show that the source region is about 10 degrees behind the limb and that it is not an active region.

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

Detected by halocme, Submitted at 2013-10-16T02:08:40

2013-10-13T06:45:35 --> 2013-10-13T08:25:11

The bright prominence is seen to push overlying structures into a large eruption, although CME association is unclear due to LASCO data gap and to a prior halo event. STEREO-B data show that the source region is about 10 degrees behind the limb and that it is not an active region.

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

Detected by halocme, Submitted at 2013-10-16T01:37:52

2013-10-13T04:50:23 --> 2013-10-13T06:20:23

The loops that encompass the whole active region erupted, followed by another eruption of loops in the western part. Neither of them leaves traces in coronagraph data.

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

Detected by halocme, Submitted at 2013-10-16T01:15:01

2013-10-12T16:00:03 --> 2013-10-12T23:00:03

The prominence slowly rises, and at a certain height it decides to break up into the lower part which clearly goes back to the chromosphere, and the upper part, only small part of which is seen to erupt. Essentially this is a failed eruption and indeed there is hardly a CME in LASCO data.

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

Detected by halocme, Submitted at 2013-10-16T01:14:59

2013-10-12T16:00:03 --> 2013-10-12T23:00:03

The prominence slowly rises, and at a certain height it decides to break up into the lower part which clearly goes back to the chromosphere, and the upper part, only small part of which is seen to erupt. Essentially this is a failed eruption and indeed there is hardly a CME in LASCO data.

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

Detected by halocme, Submitted at 2013-10-16T01:14:54

2013-10-12T16:00:03 --> 2013-10-12T23:00:03

The prominence slowly rises, and at a certain height it decides to break up into the lower part which clearly goes back to the chromosphere, and the upper part, only small part of which is seen to erupt. Essentially this is a failed eruption and indeed there is hardly a CME in LASCO data.

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

Detected by schryver, Submitted at 2013-10-15T23:19:21

2013-10-14T12:40:07 --> 2013-10-14T20:36:07

Two subsequent eruptions occur on a smallish AR in the southern hemisphere, associated ffirst with a high C-class eruptive flare within the AR, then disrupting the field into the leading QS region..

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

Detected by schryver, Submitted at 2013-10-15T23:19:20

2013-10-14T12:40:07 --> 2013-10-14T20:36:07

Two subsequent eruptions occur on a smallish AR in the southern hemisphere, associated ffirst with a high C-class eruptive flare within the AR, then disrupting the field into the leading QS region..

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

Detected by schryver, Submitted at 2013-10-15T23:06:50

2013-10-14T00:00:07 --> 2013-10-15T00:00:07

A QS filament approaching the NW limb shows continued activity, often almost surge-like, sometimes extending into the trailing QS region.

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

Detected by halocme, Submitted at 2013-10-15T22:41:41

2013-10-11T12:00:00 --> 2013-10-11T14:00:00

This flare is highly eruptive, a cusp-like structure is seen at high temperatures as well as coronal dimming.

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

Detected by halocme, Submitted at 2013-10-15T22:41:40

2013-10-11T12:00:00 --> 2013-10-11T14:00:00

This flare is highly eruptive, a cusp-like structure is seen at high temperatures as well as coronal dimming.

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

Detected by halocme, Submitted at 2013-10-15T22:41:38

2013-10-11T12:00:00 --> 2013-10-11T14:00:00

This flare is highly eruptive, a cusp-like structure is seen at high temperatures as well as coronal dimming.

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

Detected by halocme, Submitted at 2013-10-15T04:56:57

2013-10-12T17:30:35 --> 2013-10-12T20:00:35

A small eruption in the same active region that produced a M1.5 flare on 11 October 2013 is highly non-radial, disturbing trans-equatorial loops. An outflow may be seen in LASCO at a barely detectable level, but not a CME.

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

Detected by halocme, Submitted at 2013-10-15T03:54:18

2013-10-12T15:50:23 --> 2013-10-12T16:20:23

Dark regions in EUV (e.g., 211 A) images may be called coronal holes, but mixed polarity areas exist therein. This example shows a small eruption associated with flux emergence or cancellation within a so-called coronal hole.

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

Detected by halocme, Submitted at 2013-10-15T03:54:15

2013-10-12T15:50:23 --> 2013-10-12T16:20:23

Dark regions in EUV (e.g., 211 A) images may be called coronal holes, but mixed polarity areas exist therein. This example shows a small eruption associated with flux emergence or cancellation within a so-called coronal hole.

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

Detected by halocme, Submitted at 2013-10-15T03:19:14

2013-10-12T13:00:03 --> 2013-10-12T16:00:03

The eruption of the bright prominence in 304 A images does not give an impression that it made it to the heliosphere, but at least a real CME with internal structures, although slow, seems to be associated. Closed loops to the south expanded before the prominence eruption, and they hardly reached the LASCO FOV.