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

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Detected by halocme, Submitted at 2013-06-07T20:51:07

2013-06-02T15:00:03 --> 2013-06-02T18:30:03

Seen in 304 A images only, this filament eruption seems to experience deflection while leaving almost no traces in the corona and not changing the background GOES X-ray flux of about B3.5. It makes a nice CME already seen at 16:30 UT in COR1-A data. At later times the CME consists of a typical three-part structure in COR1/2-A. In LASCO data, it is diffuse, emerging from the east limb at 20:12 UT (consistent with the deflection?). Can this be a contributor to the medium storm on June 7 (Dst=-77 nT at 6 UT)?

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Detected by schryver, Submitted at 2013-06-03T20:46:26

2013-05-26T17:08:03 --> 2013-05-27T00:00:03

A pair of eruptions from an AR complex, the first moving northward, the second - fainter and more gradual - southward. The set of events looks much like a similar pair that occurred hours earlier, albeit at lesser intensity and extent.

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Detected by schryver, Submitted at 2013-06-03T20:44:25

2013-05-26T09:12:03 --> 2013-05-26T14:36:03

Two eruptions from a complex of active regions: the first eruption proceeds northward, with a compact post-eruption arcade in the central regionsof the complex, while the seconds starts as the first ends, moving southward, with a post-eruption arcade in the leading region of the complex. There are long-range (up to 300Mm) distortions in the surrounding QS corona that fade over several hours.

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Detected by anny, Submitted at 2013-05-21T01:11:59

2013-05-17T08:06:03 --> 2013-05-17T10:58:03

This movie shows an M-class flare, after which the eastern part of the filament (in the projection, roughly a third of its length) is gone and a bright arcade develops at the site of the flare. A massive coronal wave is triggered by this event (see my previous annotations). Yes, the western part of the filament (roughly 2/3rds in the plane of sky) do not seem to care. At all. The structure in the highlighted box does not change the shape _at_all_ in responce to all the changes around it and does not even _wiggle_ in the duration of this movie.

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Detected by weiliu, Submitted at 2013-05-21T00:28:11

2013-05-10T18:10:03 --> 2013-05-11T00:40:03

A giant prominence eruption like a huge plume of 1/2 R_sun across; the eruption velocity in the low corona is already >400 km/s. Much material falls back, lasting 6 hours after the initial eruption.

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Detected by schryver, Submitted at 2013-05-13T23:15:45

2013-05-13T15:24:07 --> 2013-05-13T18:32:07

An X3 flare (with footpoints over the NE limb) exhibits a coronal propagating front very suggestive of being related to an eruption over the NW limb: possible sympathy.

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Detected by anny, Submitted at 2013-05-06T18:58:25

2013-04-26T10:25:03 --> 2013-04-26T21:50:03

A VERY large filament, spanning to a good third of the disk, takes off, likely our direction.

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Detected by schryver, Submitted at 2013-05-02T17:19:29

2013-04-24T08:12:03 --> 2013-04-24T10:44:03

A QS filament, connecting to a very small bipolar region, activates and reconfigures with motions extending into two diametrically opposed directions.

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Detected by schryver, Submitted at 2013-05-02T17:07:36

2013-04-23T17:56:03 --> 2013-04-23T19:28:03

A region approaching the SW limb erupt, with a very pronounced "bubble", and coronal relaxation after the passage of the eruption.

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Detected by schryver, Submitted at 2013-05-02T16:44:47

2013-04-22T00:00:07 --> 2013-04-23T00:00:07

Formation of a QS filament.

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Detected by cheung, Submitted at 2013-04-12T01:05:36

2013-04-11T06:50:03 --> 2013-04-11T08:50:03

An impulsive eruption from AR 11719 sends a global blast wave propagating through much of the solar corona. The aftermath of this eruption is the appearance of post-eruption arcade loops.

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Detected by cheung, Submitted at 2013-04-12T01:05:32

2013-04-11T06:50:03 --> 2013-04-11T08:50:03

An impulsive eruption from AR 11719 sends a global blast wave propagating through much of the solar corona. The aftermath of this eruption is the appearance of post-eruption arcade loops.

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Detected by cheung, Submitted at 2013-04-12T01:05:28

2013-04-11T06:50:03 --> 2013-04-11T08:50:03

An impulsive eruption from AR 11719 sends a global blast wave propagating through much of the solar corona. The aftermath of this eruption is the appearance of post-eruption arcade loops.

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Detected by cheung, Submitted at 2013-04-12T00:49:32

2013-04-10T23:20:03 --> 2013-04-11T02:10:03

This unwinding surge is initiated after the appearance of a flare to its south. It is unclear whether this is sympathetic activity or pure coincidence. In any case, the surge does a rebound after its first descent, presumably due to an additional impulsive reconnection event lower in the atmosphere.

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Detected by cheung, Submitted at 2013-04-12T00:42:02

2013-04-09T11:35:03 --> 2013-04-09T16:37:33

A nice example of a limb eruption with pronounced lateral expansion of the magnetic bubble in the early phases of the eruption. The post-eruption arcade appears after the bubble is ejected out of the AIA field of view.

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Detected by cheung, Submitted at 2013-04-12T00:34:41

2013-04-08T12:50:03 --> 2013-04-08T15:00:03

A filament connecting different ARs destablizes and results in a confined filament eruption. There seems to be material exchange between the magnetic concentrations that form the three corners of this triangular complex.

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Detected by cheung, Submitted at 2013-04-03T18:00:01

2013-03-30T17:20:03 --> 2013-03-30T18:10:03

Prominence/filament material hovering in the solar corona oscillates in response to a nearby impulsive surge.

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Detected by cheung, Submitted at 2013-04-03T17:59:59

2013-03-30T17:20:03 --> 2013-03-30T18:10:03

Prominence/filament material hovering in the solar corona oscillates in response to a nearby impulsive surge.

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Detected by halocme, Submitted at 2013-03-22T05:53:12

2013-03-21T21:30:35 --> 2013-03-22T00:00:35

The flare appears to be closely related with the eruption of a prominence north of the flare region (encircled). During this prominence eruption (21:38-21:48 UT), the closed loops over the flare center started to rise, and the apparent speed increased from about 50 km/s around 21:46 UT to about 180 km/s around 21:58 UT. A bright CME appeared at 22:36 UT in LASCO C2 data, but its development is not yet known at this moment.

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

Detected by anny, Submitted at 2013-03-20T02:06:35

2013-03-17T16:06:03 --> 2013-03-17T19:58:03

A large filament eruption and a spectacular post-eruption arcade.