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

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by schryver, Submitted at 2014-02-12T17:32:24

2014-02-11T01:48:35 --> 2014-02-11T05:28:35

A compact flare in a region SEof DC flares, as a spary/surge from a region to its NW occurs.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by weiliu, Submitted at 2014-02-10T02:14:43

2012-01-21T07:00:04 --> 2012-01-21T15:00:04

The filament on the disk (not the largest one near the disk center) first erupted, producing a nice two-ribbon flare. Then the one closer to the limb erupted, producing a surge (most mass falls back along a spine-fan like trajectory), rapidly followed by another filament eruption from the same region.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-02-10T02:14:34

2012-10-10T05:20:03 --> 2012-10-10T08:10:03

The following attributes suggest an emerging flux region just behind the limb: 1. Very dynamic loops structures, 2. Frequent surges (optically thick material) in the foreground of the EUV loops, and 3. A localized brightening, possibly due to reconnection event(s). Surges are commonly found in the periphery of emerging flux regions as the emerging magnetic field impinges on pre-existing neighbouring field. The squeezing of the field could squirt dense material into a surge.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-02-10T02:14:33

2012-04-25T10:00:04 --> 2012-04-25T11:50:04

Some energetic event leads to a surge of material into a magnetic fan.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-02-10T02:14:29

2012-10-10T05:20:03 --> 2012-10-10T08:10:03

The following attributes suggest an emerging flux region just behind the limb: 1. Very dynamic loops structures, 2. Frequent surges (optically thick material) in the foreground of the EUV loops, and 3. A localized brightening, possibly due to reconnection event(s). Surges are commonly found in the periphery of emerging flux regions as the emerging magnetic field impinges on pre-existing neighbouring field. The squeezing of the field could squirt dense material into a surge.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-02-10T02:14:24

2012-04-07T22:40:04 --> 2012-04-08T07:10:04

The source region of this filament eruption is most likely beyond the western horizon of the solar disk. Post-eruption arcade loops are seen in AIA images but there is no corresponding large GOES flare. This is possibly due to occultation of the footpoints.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-02-10T02:14:21

2012-05-30T01:40:04 --> 2012-05-30T03:20:04

The rise of the filament material is halted and the material drains back down to the footpoints of the relaxed magnetic structure.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-02-10T02:14:19

2012-10-10T13:45:03 --> 2012-10-10T15:25:03

A small eruption in the neighbourhood of AR 11583 leads to an impulsive reconnection event that forms a coronal jet. The material spewed out by the jet follows a set of closed field lines so that most of the material sseems to be trapped in the corona and/or is forced to return to lower layers of the atmosphere.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-02-10T02:14:16

2012-10-10T13:45:03 --> 2012-10-10T15:25:03

A small eruption in the neighbourhood of AR 11583 leads to an impulsive reconnection event that forms a coronal jet. The material spewed out by the jet follows a set of closed field lines so that most of the material sseems to be trapped in the corona and/or is forced to return to lower layers of the atmosphere.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-02-05T01:46:54

2014-01-28T00:00:03 --> 2014-01-29T00:00:03

A lot seems to be going on in this remarkable active region over the last several days. Right now, it is positioned right at the E limb which might make it a favorable subject of future studies.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-02-05T01:40:24

2014-01-28T15:08:03 --> 2014-01-29T00:00:03

A large prominence detatches on one end and slowly contracts towards the other end.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-02-05T01:37:12

2014-01-28T03:48:03 --> 2014-01-28T10:18:03

A C9-class flare is immediately followed by coronal rain formation above the site of the flare, on the E limb. The massive spray surge erupts from visually where the rain has fallen down, immediately after it's done falling.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-02-05T01:37:11

2014-01-28T03:48:03 --> 2014-01-28T10:18:03

A C9-class flare is immediately followed by coronal rain formation above the site of the flare, on the E limb. The massive spray surge erupts from visually where the rain has fallen down, immediately after it's done falling.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-02-01T00:26:26

2014-01-26T20:24:03 --> 2014-01-27T00:00:03

A large prominence eruption, visually originating behind the SE limb. Note a handful of fine-scale 171A "grains of sand" expelled (visually between the two main footpoints).

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by weiliu, Submitted at 2014-01-18T04:05:28

2013-12-19T22:50:03 --> 2013-12-20T00:10:03

An interesting surge exhibits unwinding twists as it erupts and follows a curved path, much like an event seen by Hinode in greater detail (see http://adsabs.harvard.edu/abs/2009ApJ...707L..37L

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-01-17T02:06:33

2014-01-15T22:30:03 --> 2014-01-16T01:45:03

Filament material seems to corkscrew along some field lines before draining back.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by slater, Submitted at 2014-01-09T04:34:43

2014-01-07T17:30:35 --> 2014-01-08T03:30:35

Large eruptive flare from AR 11944. Complex multi-ribbons (at least three). Flare associated with flux system connecting the leading spot of the region with decaying active region flux to the west. Two sets of post flare loops connecting two different flux systems. Blast directed to the southwest.

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-06T15:37:39

2014-01-06T07:30:35 --> 2014-01-06T08:59:23

The eruption should be from a far-side region since there is hardly an increase in GOES soft X-ray flux. A bright prominence eruption, dimming and loop oscillations are clearly seen. This is associated with a proton event that extends to > 100 MeV (thanks, Sam, for reporting this.)

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-06T15:37:36

2014-01-06T07:30:35 --> 2014-01-06T08:59:23

The eruption should be from a far-side region since there is hardly an increase in GOES soft X-ray flux. A bright prominence eruption, dimming and loop oscillations are clearly seen. This is associated with a proton event that extends to > 100 MeV (thanks, Sam, for reporting this.)

Rating: 4.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by anny, Submitted at 2014-01-03T22:54:28

2013-12-08T19:42:03 --> 2013-12-09T00:00:03

A small bubble (bright in 304A) is ejected from an AR at the E disk. This bubble travels along the nearby filament-like structure, gradually increasing in size, then goes past the dark 304A structure, lifts up along what appears a spiral trajectory, and falls down over an extended patch in the quiet sun as coronal rain.