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

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2016-01-12T02:58:55

2016-01-09T13:34:06 --> 2016-01-09T14:40:06

This mini-filament eruption leads to a blow out jet. During the eruption the filament material seems to be torn apart and slamed into a magnetic wall.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2016-01-12T02:58:55

2016-01-09T13:34:06 --> 2016-01-09T14:40:06

This mini-filament eruption leads to a blow out jet. During the eruption the filament material seems to be torn apart and slamed into a magnetic wall.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2015-12-29T18:28:56

2015-12-28T10:00:06 --> 2015-12-29T05:00:06

The eruption associated with the M1.86 flare in AR 12473 produced twin dimming, which is often seen in a sigmoid region. The dimming region, especially the one west of the flare, has taken long time (> 12 hours) to recover, suggesting significant mass evacuation due to the eruption. The CME from this eruption is predicted to hit Earth on 30-31 December (see https://twitter.com/halocme/status/681551822083903488 and https://twitter.com/halocme/status/681602361291227136).

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-12-10T23:25:46

2015-12-09T19:48:06 --> 2015-12-09T23:48:06

A filament adjacent to a decaying AR erupts, connecting to a trailing AR, and then reconfiguring to apparently inolve the leading edge of its AR and likely even towards a leading AR (at least distorting connecting loops).

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-12-10T20:33:37

2015-12-08T16:16:06 --> 2015-12-09T00:00:06

A quiet-Sun filament, connected at one end to a moderate AR, erupts, showing loops being moved aside, and later ribbons and post-eruption loops. As the loops continue to settle after the eruption, another eruption starts from the AR, reaching into QS and a distant trailing region in a direction some 30 degrees away from the initial eruption process: it is not obvious from the images how the fields are connected, but coronal dimming of the distant trailing QS corona suggests connections.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-12-10T20:33:37

2015-12-08T16:16:06 --> 2015-12-09T00:00:06

A quiet-Sun filament, connected at one end to a moderate AR, erupts, showing loops being moved aside, and later ribbons and post-eruption loops. As the loops continue to settle after the eruption, another eruption starts from the AR, reaching into QS and a distant trailing region in a direction some 30 degrees away from the initial eruption process: it is not obvious from the images how the fields are connected, but coronal dimming of the distant trailing QS corona suggests connections.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2015-11-16T16:29:28

2015-11-15T21:00:34 --> 2015-11-16T05:00:34

Each was a gorgeous eruption from a quiescent region. Neither may hit the Earth directly due to deflection by a coronal hole near disk center.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-11-05T21:49:47

2015-11-04T00:00:06 --> 2015-11-04T05:36:06

An AR approaching the NW limb exhibits two successive short-duration M-class flares, associated with spray-like eruptions of filament material. Following the first such eruption, a small bipolar region trailing the AR destabilizes and erupts, possibly in a form of sympathy through magnetic coupling. The second eruption is followed by coronal rain: thin, elongated strands of dark material fall down along a ridge of field, causing impact brightenings in at least Fe IX-XIV that last for a few to just over 5 minutes at any given location.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-11-05T21:49:45

2015-11-04T00:00:06 --> 2015-11-04T05:36:06

An AR approaching the NW limb exhibits two successive short-duration M-class flares, associated with spray-like eruptions of filament material. Following the first such eruption, a small bipolar region trailing the AR destabilizes and erupts, possibly in a form of sympathy through magnetic coupling. The second eruption is followed by coronal rain: thin, elongated strands of dark material fall down along a ridge of field, causing impact brightenings in at least Fe IX-XIV that last for a few to just over 5 minutes at any given location.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-11-02T22:58:54

2015-10-30T00:00:06 --> 2015-10-30T06:16:06

An eruption over QS appears to reach westward into a small bipolar region that exhibits an eruption just a few hours later.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-10-27T20:28:47

2015-10-26T05:12:06 --> 2015-10-26T12:36:06

A high-latitude filament drains and disappears.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by weiliu, Submitted at 2015-10-16T00:42:06

2015-10-14T05:50:06 --> 2015-10-15T00:00:06

Three filament eruption occurred in a series the same neighborhood within a day, possibly sympathetic events, one triggered by another. The first two seemed to be two sections of the same filament, while the 3rd one was situated in another filament channel parallel to the first one.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-10-08T20:52:16

2015-10-04T07:00:06 --> 2015-10-04T13:40:06

A QS filament to the North of a mid-size AR destabilizes and reconfigures. It looks like a loop in the configuration rises, to disappear as the system settles.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-09-22T00:25:22

2015-09-20T04:40:06 --> 2015-09-20T08:52:06

Flare on the NE limb, with a short (~2min) and intense loop-top brightening at 06:08, followed by a post-eruption arcade and coronal rain.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-08-25T15:33:30

2015-08-24T07:00:06 --> 2015-08-24T10:00:06

A flare in the trailing end of an AR (likely associated with compact flux emergence next to the trailing spot) causes an ejection towards the NE. This interacts with enhanced network field, leading to a thermal/field change, which is followed by what looks like a rerouting of a filament, with dark material suddenly rising and 'rolling' into a new configuration.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-08-24T18:04:41

2015-08-22T06:04:10 --> 2015-08-22T09:28:10

A flare from an AR in the S hemisphere leads to reconfiguration and a large-scale clear propagating front reaching to the far N of the N hemisphere, while loop oscillations are seen in the outlying loops of the exploding AR and connections to a small AR towards the N.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by juanms, Submitted at 2015-08-14T22:11:06

2015-08-12T11:10:06 --> 2015-08-12T22:30:06

The filament eruption is observed along a large distance and time, which is preciding a post flare loops growing in time. The ejected mass is concentrated mostly at both ends of the filament.The eruptuion reveals the twisted field lines.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2015-08-11T00:19:42

2015-08-07T17:36:06 --> 2015-08-08T00:00:06

Two adjacent filaments near the SE limb erupt in sequence, potentially through interaction.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2015-07-29T21:46:23

2015-07-25T13:10:06 --> 2015-07-25T16:10:06

The cool material in this quiescent filament is seen to stretch vertically during the onset of the eruption. A coronal wave propagates away from the eruption site. Transverse oscillations (swishing motions) are also induced in the residual filament material.

Rating: 5.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2015-07-29T21:46:21

2015-07-25T13:10:06 --> 2015-07-25T16:10:06

The cool material in this quiescent filament is seen to stretch vertically during the onset of the eruption. A coronal wave propagates away from the eruption site. Transverse oscillations (swishing motions) are also induced in the residual filament material.