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

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-09T07:20:47

2013-12-22T18:50:23 --> 2013-12-22T21:00:23

This C6.1 flare is characterized by fast collimated ejections. A narrow (not flux-rope type) CME was already observed by LASCO at 19:48 UT.

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Detected by halocme, Submitted at 2014-01-09T07:09:52

2013-12-22T04:30:35 --> 2013-12-22T07:00:35

The eruption seems to be bounced back twice. The coronal response seems to be minimal.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-09T07:03:36

2013-12-22T01:45:35 --> 2013-12-22T07:25:35

The impression of tumbling motions may just come from ejection of material from one leg of the prominence to the other. It is not clear how high the morions reach.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-09T06:49:44

2013-12-21T03:20:23 --> 2013-12-21T05:00:23

This is presumably originates from behind the limb. Part of the prominence is seen bright in 171 A and 211 A indicating that it heats up during the eruption. Other smooth structures are seen primarily in 304 A. The response of the overlying structure (e.g., dimming) is very small.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-09T06:41:41

2013-12-20T20:00:31 --> 2013-12-21T05:00:31

This is a minor eruption primarily seen in 304 A channel. Like other cases, the prominence erupts with untwisting motions.

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Detected by halocme, Submitted at 2014-01-09T06:33:11

2013-12-20T10:30:00 --> 2013-12-20T13:00:00

This flare was preceded by a C2.2 flare. It may have played a role of destabilizing the structure that was erupted in a limited way in the main flare. The eruption appears to be largely confined, although leaving some dimming signatures.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-09T06:33:11

2013-12-20T10:30:00 --> 2013-12-20T13:00:00

This flare was preceded by a C2.2 flare. It may have played a role of destabilizing the structure that was erupted in a limited way in the main flare. The eruption appears to be largely confined, although leaving some dimming signatures.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-09T06:33:10

2013-12-20T10:30:00 --> 2013-12-20T13:00:00

This flare was preceded by a C2.2 flare. It may have played a role of destabilizing the structure that was erupted in a limited way in the main flare. The eruption appears to be largely confined, although leaving some dimming signatures.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-09T06:24:43

2013-12-20T06:30:35 --> 2013-12-20T10:30:35

The filament lay north of AR 11920. The movie captures its slow rise, and the coronal response after the filament reached the cirtain height. Two-ribbon emission is seen, not reaching the GOES background level in X-rays.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-01-07T01:25:27

2014-01-06T05:10:03 --> 2014-01-06T07:20:03

Most of the filamentary material (304, orange) from this eruption seems to slide back down toward the lower atmosphere. Nevertheless the temporal change in the off-limb signal in 211 (green) sugguests an irrevocable change in the large-scale coronal field.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-01-07T00:55:47

2014-01-05T17:40:03 --> 2014-01-05T18:50:03

Surges are launched in succession at the edge of this emerging flux region.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-01-07T00:55:44

2014-01-05T17:40:03 --> 2014-01-05T18:50:03

Surges are launched in succession at the edge of this emerging flux region.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by cheung, Submitted at 2014-01-07T00:51:24

2014-01-05T15:56:03 --> 2014-01-05T16:50:03

The two jets occur in succession and both exhibit apparent rotational motion.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-06T15:37:42

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: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-06T05:10:40

2013-12-31T09:45:35 --> 2013-12-31T12:45:35

This flare was slightly limb occulted. The dimming is seen above the flare loops. This immediately became a bright and fast (~1000 km s-1) CME. The top of some of these loops shows hot plasma in 193 A channel, above which downflows are indicated as they are in certain eruptive flares.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-06T05:10:39

2013-12-31T09:45:35 --> 2013-12-31T12:45:35

This flare was slightly limb occulted. The dimming is seen above the flare loops. This immediately became a bright and fast (~1000 km s-1) CME. The top of some of these loops shows hot plasma in 193 A channel, above which downflows are indicated as they are in certain eruptive flares.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-06T04:54:21

2013-12-30T19:45:35 --> 2013-12-30T22:45:35

There are two episodes of eruption. First, multiple loops interacted in the eastern part of the region, leading to an eruption. The second episode seems to be more straightforward, and the eruption is faster. These are very diffuse and difference movies are needed to see them. Part of the motions may represent waves rather than mass motions.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-06T04:42:04

2013-12-30T10:40:11 --> 2013-12-30T12:40:11

The motion toward south is noted only in difference images because it is too diffuse in intensity images. There is no clear filament eruption in 304 A or 211 A channel. Perhaps we are looking at a wave rather than a mass motion.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-06T04:33:01

2013-12-29T01:40:11 --> 2013-12-29T04:40:11

In difference images in these channels, we note four eruptions in three hours. First, a small eruption in the eastern hemisphere, like E50, and another one in the northen hemisphere, like N40. Then bigger ones near the southwast limb and over the west limb.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2014-01-06T04:33:01

2013-12-29T01:40:11 --> 2013-12-29T04:40:11

In difference images in these channels, we note four eruptions in three hours. First, a small eruption in the eastern hemisphere, like E50, and another one in the northen hemisphere, like N40. Then bigger ones near the southwast limb and over the west limb.