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 2011-10-03T02:59:16

2011-10-02T00:15:00 --> 2011-10-02T01:31:48

This is likely to be an Earth-directed CME, although HI1 beacon data suggest that the ejection was pimarily above ecliptic.

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

Detected by halocme, Submitted at 2011-09-30T16:50:27

2011-09-24T04:00:05 --> 2011-09-24T06:00:05

A CME-like eruption is seen in the southern region, but recurrent jet-like activities in the northern region may have helped the souther region erupt...

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

Detected by halocme, Submitted at 2011-09-30T16:02:20

2011-09-30T02:30:00 --> 2011-09-30T03:15:36

An arguable EUV wave. This does not like to be driven by a CME that opens up coronal field in a global way. It avoids the active region, and then stops at a coronal hole.

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

Detected by halocme, Submitted at 2011-09-30T15:33:31

2011-09-30T03:15:36 --> 2011-09-30T04:31:12

This event shows a pattern similar to the one observed on 29 September 2011 around 18 UT. Does not look like a full-blown CME.

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

Detected by halocme, Submitted at 2011-09-30T15:22:45

2011-09-29T17:40:12 --> 2011-09-29T19:10:12

X-ray light curves are missing during the early phase of the event, so C5.6 may not be correct. This does not seem to be a full-blown eruption.

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

Detected by halocme, Submitted at 2011-09-29T18:37:26

2011-09-29T11:45:00 --> 2011-09-29T13:46:12

The apparent filament eruption from the AR 11302 was toward south, but this large-scale eruption, not clearly seen in intensity images, was toward northwest.

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

Detected by cheung, Submitted at 2011-09-29T01:14:15

2011-09-23T23:20:04 --> 2011-09-24T01:00:04

The field lines delineated by the ejected material following the eruption are seen to vibrate.

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

Detected by cheung, Submitted at 2011-09-29T01:14:14

2011-09-23T23:20:04 --> 2011-09-24T01:00:04

The field lines delineated by the ejected material following the eruption are seen to vibrate.

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

Detected by cheung, Submitted at 2011-09-29T01:09:55

2011-09-23T11:50:04 --> 2011-09-23T13:20:04

The material lifted off from this eruption seems to "evaporate" into the ambient corona.

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

Detected by cheung, Submitted at 2011-09-29T01:01:39

2011-09-22T15:10:04 --> 2011-09-22T22:50:04

A filament erupts possibly after destabilzation following the erutpion that led to the X-class flare. A significant amount of material is seen drainiing back toward the solar surface.

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

Detected by cheung, Submitted at 2011-09-29T00:47:53

2011-09-22T08:20:04 --> 2011-09-23T06:00:04

An X-class flare is seen on the east limb of the Sun following an eruption. The cross-hair like spikes are due to the diffraction pattern of the telecope(s).

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

Detected by cheung, Submitted at 2011-09-29T00:47:52

2011-09-22T08:20:04 --> 2011-09-23T06:00:04

An X-class flare is seen on the east limb of the Sun following an eruption. The cross-hair like spikes are due to the diffraction pattern of the telecope(s).

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

Detected by halocme, Submitted at 2011-09-29T00:44:43

2011-09-27T20:20:24 --> 2011-09-27T22:00:00

Some may see an EUV wave here, but given the small distance of the propoagation, it is perhaps better to put this in a category of loop oscillation.

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

Detected by halocme, Submitted at 2011-09-28T19:12:35

2011-09-23T23:40:12 --> 2011-09-24T00:40:12

This wave is not spectacular, but the event is associated with a metric type II radio burst.

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

Detected by seguin, Submitted at 2011-09-28T18:05:53

2011-09-22T09:00:04 --> 2011-09-22T17:38:28

X1.4 flare on northeast limb of the Sun causes a coronal wave (annotated in another event, ). There is some clear post-flare loop oscillation, and what appears to be a spray surge or jet (small filament eruption?) squirting south beneath the post-eruptive loops from the south side of the active region. No filament was readily visible in the 3 channels shown here (211, 193, 171). This eruptive flare triggered a halo CME as observed by LASCO: http://umbra.nascom.nasa.gov/lasco/observations/halo/110922a/ X flare generated coronal wave event: http://lmsal.com/hek/her?cmd=view-voevent&ivorn=ivo://helio-informatics.org/CWMET_RalphSeguin_20110928_173524

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

Detected by seguin, Submitted at 2011-09-28T18:05:51

2011-09-22T09:00:04 --> 2011-09-22T17:38:28

X1.4 flare on northeast limb of the Sun causes a coronal wave (annotated in another event, ). There is some clear post-flare loop oscillation, and what appears to be a spray surge or jet (small filament eruption?) squirting south beneath the post-eruptive loops from the south side of the active region. No filament was readily visible in the 3 channels shown here (211, 193, 171). This eruptive flare triggered a halo CME as observed by LASCO: http://umbra.nascom.nasa.gov/lasco/observations/halo/110922a/ X flare generated coronal wave event: http://lmsal.com/hek/her?cmd=view-voevent&ivorn=ivo://helio-informatics.org/CWMET_RalphSeguin_20110928_173524

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

Detected by seguin, Submitted at 2011-09-28T18:05:48

2011-09-22T09:00:04 --> 2011-09-22T17:38:28

X1.4 flare on northeast limb of the Sun causes a coronal wave (annotated in another event, ). There is some clear post-flare loop oscillation, and what appears to be a spray surge or jet (small filament eruption?) squirting south beneath the post-eruptive loops from the south side of the active region. No filament was readily visible in the 3 channels shown here (211, 193, 171). This eruptive flare triggered a halo CME as observed by LASCO: http://umbra.nascom.nasa.gov/lasco/observations/halo/110922a/ X flare generated coronal wave event: http://lmsal.com/hek/her?cmd=view-voevent&ivorn=ivo://helio-informatics.org/CWMET_RalphSeguin_20110928_173524

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

Detected by seguin, Submitted at 2011-09-28T18:05:43

2011-09-22T09:00:04 --> 2011-09-22T17:38:28

X1.4 flare on northeast limb of the Sun causes a coronal wave (annotated in another event, ). There is some clear post-flare loop oscillation, and what appears to be a spray surge or jet (small filament eruption?) squirting south beneath the post-eruptive loops from the south side of the active region. No filament was readily visible in the 3 channels shown here (211, 193, 171). This eruptive flare triggered a halo CME as observed by LASCO: http://umbra.nascom.nasa.gov/lasco/observations/halo/110922a/ X flare generated coronal wave event: http://lmsal.com/hek/her?cmd=view-voevent&ivorn=ivo://helio-informatics.org/CWMET_RalphSeguin_20110928_173524

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

Detected by seguin, Submitted at 2011-09-28T17:35:36

2011-09-22T09:00:04 --> 2011-09-22T17:38:28

The X1.4 flare on Sep 22, 2011 generates a coronal wave across the entire eastern hemisphere of the Sun. I generated other movies and some combined AIA + SECCHI views, which are available here: http://lmsal.com/pub/seguin/sdo/xflare_20110922/ http://lmsal.com/pub/seguin/sdo/xflare_20110922/aia_secchi_ab_193_20110922_120s_1080p.mov http://lmsal.com/pub/seguin/sdo/xflare_20110922/aia_secchi_ab_304_20110922_120s_1080p.mov ...

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

Detected by halocme, Submitted at 2011-09-27T06:03:42

2011-09-09T05:50:24 --> 2011-09-09T07:00:00

This concludes a series of wave-like disturbances in AR 11283. A similar pattern to the previous three events is seen.