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 2014-12-02T20:58:15

2014-11-23T03:00:03 --> 2014-11-23T13:24:03

Reconfiguration of near & over the limb (SW) set of loops apparently retracting and mildly oscillation, then apparently forming a new filament configuration.

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

Detected by schryver, Submitted at 2014-12-01T19:51:12

2014-11-18T15:16:03 --> 2014-11-18T23:00:03

A QS filament arches over a compact ER and its corona, destabilizing and reconfiguring as it eventually moves off the bipole.

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

Detected by schryver, Submitted at 2014-11-27T00:27:08

2014-11-11T10:28:07 --> 2014-11-11T14:32:07

Two adjacent eruptions, likely sympathetic: one from a sigmoid in what looks like a decayed AR, and another from QS trailing/northward of a larger AR.

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 schryver, Submitted at 2014-10-23T18:34:02

2014-10-19T03:44:03 --> 2014-10-19T09:20:03

A surge (strongly nonradial, directed towards the S) occurs (with much material later sliding back down again), in association with an X1.1 flare. The flare is associated with strong brightening of high loops (particularly in the 193 channel in the 211/193/171 triplet), but with no obvious bright kernels or diffraction patterns, and with saturation in the 193 channel only clearly at the loop tops.

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

Detected by cheung, Submitted at 2014-10-17T17:40:51

2014-10-11T02:10:07 --> 2014-10-12T12:40:07

NOAA AR 12187 emerges as it rotates across the east limb. The emergence of magnetic flux drives intense atmospheric responses. These include surges at the periphery of the emerging flux region and eruptions resulting from magnetic reconnection.

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 cheung, Submitted at 2014-10-17T17:40:49

2014-10-11T02:10:07 --> 2014-10-12T12:40:07

NOAA AR 12187 emerges as it rotates across the east limb. The emergence of magnetic flux drives intense atmospheric responses. These include surges at the periphery of the emerging flux region and eruptions resulting from magnetic reconnection.

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

Detected by cheung, Submitted at 2014-10-17T17:40:49

2014-10-09T00:00:07 --> 2014-10-09T15:20:07

Magnetic reconnection between neighboring loops in this compact emerging flux region leads to intermittent flashes of energy release.

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

Detected by cheung, Submitted at 2014-10-17T17:40:47

2014-10-11T02:10:07 --> 2014-10-12T12:40:07

NOAA AR 12187 emerges as it rotates across the east limb. The emergence of magnetic flux drives intense atmospheric responses. These include surges at the periphery of the emerging flux region and eruptions resulting from magnetic reconnection.

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

Detected by cheung, Submitted at 2014-10-17T17:40:47

2014-10-09T00:00:07 --> 2014-10-09T15:20:07

Magnetic reconnection between neighboring loops in this compact emerging flux region leads to intermittent flashes of energy release.

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

Detected by schryver, Submitted at 2014-10-14T22:18:12

2013-01-13T22:15:35 --> 2013-01-14T03:50:35

An apparent segment of a coronal null fan 'clears out', best seen in 193, in associateing with some oscillatory loop motions, to refill after about 2.5h.

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

Detected by schryver, Submitted at 2014-10-14T22:18:08

2014-06-15T04:32:03 --> 2014-06-15T10:04:03

An eruption from just behind the NW limb opens the high coronal field, rocking it into oscillations, and suggestive of a high-coronal null-point configuration in the afterglow.

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

Detected by schryver, Submitted at 2014-10-14T22:17:56

2014-06-03T03:36:03 --> 2014-06-03T07:08:03

The 1-2MK plasma lights up around the absorption feature of a prominence over the SE limb, with lots of dynamics (up and down) in the dark, cool material.

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.