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

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

Detected by schryver, Submitted at 2015-05-06T22:24:33

2015-05-05T20:25:03 --> 2015-05-06T03:00:03

Filament eruption (curiously synchronous with distant X-class flare)

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Detected by schryver, Submitted at 2015-04-30T19:50:18

2015-04-27T22:00:03 --> 2015-04-29T07:45:03

A very large filament erupts, immediately following an eruption on its trailing side, where another eruption occurs right after. There is also some activity in the leading AR, but causality of timing is unclear.

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Detected by halocme, Submitted at 2015-04-13T22:02:27

2015-04-04T22:00:03 --> 2015-04-05T02:00:03

The eastern part of the long filament erupted, resulting in two-ribbion and post-eruption arcade emission that peaked at the GOES C3.8 level. In a later stage the eruption looked more like a big surge in 304 A iimages. The eruption seemed to activate the western part of the filament.

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

Detected by halocme, Submitted at 2015-04-09T00:44:47

2015-03-15T00:30:35 --> 2015-03-15T02:30:35

This is the origin of the St. Patrick's day storm, which recorded Dst ~ -220 nT. The event started off with a jet or surge (C2.4 flare), which seemed to hit a larger filament and then let it go. The main eruption was associated with a C9.1 LDE.

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

Detected by schryver, Submitted at 2015-04-06T17:23:49

2015-04-04T21:25:03 --> 2015-04-05T05:35:03

A long filament snakes across the Sun from N to S hemisphere. The southernmost extension destabilizes and erupts, with signatures also on a filament towards the N that is not obviously connected.

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

Detected by schryver, Submitted at 2015-03-30T18:44:43

2015-03-27T06:28:03 --> 2015-03-28T00:00:03

Very large prominence over the NE limb erupts, followed by coronal rain and high afterglow.

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

Detected by schryver, Submitted at 2014-12-30T19:19:37

2014-12-24T02:21:35 --> 2014-12-24T03:32:23

Filament eruption, with much of the filament confined to a higher new configuration. Looks like an aneurism from the initial filament configuration, that at least partly remains lying low.

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

Detected by cheung, Submitted at 2014-12-12T20:34:48

2014-12-12T02:50:03 --> 2014-12-12T06:40:03

This filament eruption from the southern hemisphere occurs at about the same time as the larger one in the north (http://lmsal.com/hek/her?cmd=view-voevent&ivorn=ivo://helio-informatics.org/FEMET_MarkCheung_20141212_203117). There is no clear evidence that the two are causually related (non-sympathy?).

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

Detected by cheung, Submitted at 2014-12-12T20:31:24

2014-12-11T23:20:03 --> 2014-12-12T08:50:03

Before eruption, this horseshoe-shaped quiescent filament mainly resided above the polarity inversion line of a decayed AR(s). However the southern end of the filament is anchored close to AR 12232. It is unclear whether the eruption is triggered by the evolution of AR 12232, or flux cancellation across the polarity inversion line below the rest of the filament, or a combination of the two. It is also possible that the launch is triggered by other eruptive events further afield, though none have scales comparable to this eruption. The filament eruption southwest of this event may be a candidate for sympathy, though it is much smaller.

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

Detected by schryver, Submitted at 2014-11-26T23:50:18

2014-11-09T06:12:03 --> 2014-11-09T12:20:03

Possible sympathetic eruptions on disk and over E limb.

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

Detected by cheung, Submitted at 2014-10-17T17:40:50

2014-10-10T15:40:07 --> 2014-10-11T00:00:07

A long post-eruption arcade is left in the wake of the eruption. The initial arcade loops are sheared and roughly aligned in the general direction of the polarity inversion line (PIL). As the eruption progresses, higher reaching arcade loops that are more penpendicular to the PIL appear.

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

Detected by schryver, Submitted at 2014-10-14T22:17:50

2014-09-26T03:54:03 --> 2014-09-26T06:05:27

Major eruption from the E limb

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

Detected by schryver, Submitted at 2014-10-14T22:17:45

2014-09-26T03:20:03 --> 2014-09-26T06:20:03

A large, complex filament eruption over the E limb, with fibrils of material being apparently pulled back rather than falling back.

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

Detected by schryver, Submitted at 2014-10-14T22:17:43

2014-06-04T10:16:03 --> 2014-06-05T00:00:03

A very large, unusually high filament/prominence erupts from over quite Sun, with an extensive, beautiful pattern of ribbons and afterglow over a large region of QS.

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

Detected by schryver, Submitted at 2014-10-14T22:17:43

2014-05-04T14:16:03 --> 2014-05-04T22:24:03

Prominence eruption over the NW limb.

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

Detected by schryver, Submitted at 2014-10-14T22:17:43

2014-04-29T18:04:03 --> 2014-04-29T22:56:03

Prominence eruption from the SW limb, with post-eruption ribbons, and with an apparent disconnect of the ejected material at some 100Mm above the limb.

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

Detected by schryver, Submitted at 2014-10-14T22:17:42

2014-04-28T01:04:03 --> 2014-04-28T21:20:03

Although the AIA 171/193/211 images show no direct evidence of a large-scale, slow eruption, the 'discoloration', as a signature of thermal changes in the quiet-Sun corona, are reminiscent of those typically seen during eruptions. The 304 channel shows a long, thin, multistranded filament erupting, and SOHO/LASCO C2 data show a large, northward CME at what appears to be the corresponding location and time.

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

Detected by schryver, Submitted at 2014-10-14T22:17:42

2014-04-18T04:04:03 --> 2014-04-18T18:00:03

A long-lived polar-crown filament activates in association with an eruption from a QS region south of an AR towards the north of both. Then an M7 flare and eruption occurs that leads to oscillations and distortions in the polar-crown filament, which subsequently loses its configuration and disappears as much of its cool material slides towards the W and N to a QS region just on the li mb.

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

Detected by schryver, Submitted at 2014-10-14T22:17:42

2014-01-02T09:04:03 --> 2014-01-02T11:32:03

A near-equatorial QS filament erupts from near the W limb. Synchronously, an AR filament near DC activates, as does a filament SE of the primary eruption. A fragment of a prominence to the S of the eruption exhibits briefly oscillations.

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

Detected by schryver, Submitted at 2014-10-14T22:17:41

2014-01-01T18:28:03 --> 2014-01-01T21:04:03

An M9 flare from a region in the SW quadrant associated with a filament eruption, with much (most?) of the material falling back onto the surface.