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

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

Detected by cheung, Submitted at 2014-04-28T17:55:37

2014-04-24T23:50:04 --> 2014-04-25T10:30:04

The footpoints of the flare loops in this X1.3 flare are occulted by the east limb. Supra-arcade downflows can be seen near the top of the candle flame, which appears after the impulsive phase.

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

Detected by cheung, Submitted at 2014-04-28T17:55:36

2014-04-24T23:50:04 --> 2014-04-25T10:30:04

The footpoints of the flare loops in this X1.3 flare are occulted by the east limb. Supra-arcade downflows can be seen near the top of the candle flame, which appears after the impulsive phase.

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

Detected by cheung, Submitted at 2014-04-15T18:40:17

2014-04-11T18:00:03 --> 2014-04-12T05:50:03

The rain that condenses out of the corona seem to be momentarily trapped above a set of active region loops. Eventually they manage to find a way to disappear (i.e. go out of the 304 passband) or slide down.

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

Detected by cheung, Submitted at 2014-04-11T22:40:19

2014-04-11T14:30:03 --> 2014-04-11T15:40:03

The surge resulting from this eruption results in a set of field lines traced out by the ejeccting filamentary material (304). The 304 channel clearly delineates separate magnetic subdomains. The intermitent structures at the bonudary of these subdomains is suggestive of bursty reconnection.

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

Detected by cheung, Submitted at 2014-04-11T22:40:18

2014-04-11T14:30:03 --> 2014-04-11T15:40:03

The surge resulting from this eruption results in a set of field lines traced out by the ejeccting filamentary material (304). The 304 channel clearly delineates separate magnetic subdomains. The intermitent structures at the bonudary of these subdomains is suggestive of bursty reconnection.

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

Detected by cheung, Submitted at 2014-04-11T22:40:17

2014-04-11T14:30:03 --> 2014-04-11T15:40:03

The surge resulting from this eruption results in a set of field lines traced out by the ejeccting filamentary material (304). The 304 channel clearly delineates separate magnetic subdomains. The intermitent structures at the bonudary of these subdomains is suggestive of bursty reconnection.

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

Detected by cheung, Submitted at 2014-04-11T18:40:17

2014-04-07T18:50:03 --> 2014-04-08T00:40:03

These vertical fingers of coronal rain in 304 emanate from the bottom of an overlying cavity.

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

Detected by cheung, Submitted at 2014-04-11T18:40:16

2014-04-07T18:50:03 --> 2014-04-08T00:40:03

These vertical fingers of coronal rain in 304 emanate from the bottom of an overlying cavity.

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

Detected by anny, Submitted at 2014-04-09T01:40:17

2014-04-02T12:38:03 --> 2014-04-02T17:10:03

A sigmoid filament erupts on the NE disk. While the eruptied matter itself is barely visible, this event is followed by major footpoint brightening, dramatic reconfiguration of the overlying field, a coronal wave and a spectacular elongated post-flare arcade.

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

Detected by schryver, Submitted at 2014-04-03T20:12:36

2014-03-31T14:16:03 --> 2014-04-01T00:00:03

A large complex filament system activates, connecting southern latitudes to the equatorial region and a smallish AR. Lots of fleeting brightenings, twirling loops, and thermal changes.

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

Detected by schryver, Submitted at 2014-04-03T20:07:17

2014-03-30T10:24:03 --> 2014-03-30T14:24:03

A flare+eruption from a mid-sized region in the NW at the same time as a large filament eruption from a region towards the NE limb.

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

Detected by schryver, Submitted at 2014-04-03T19:46:04

2014-03-28T20:00:03 --> 2014-03-29T01:28:03

A most unusual prominence activation over the NE limb, in which what looks like a hedgerow filament is seen to connect in EUV channels to structure towards the north of it, while the entire top part appears to spin as it lifts.

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

Detected by anny, Submitted at 2014-03-25T00:30:55

2014-03-16T01:48:03 --> 2014-03-16T06:15:03

A massive spectacular filament eruption, which appears to be directed southwards and is associated with an EUV wave.

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

Detected by schryver, Submitted at 2014-03-12T21:05:49

2014-03-10T15:36:03 --> 2014-03-11T00:00:03

A QS filament reaching into the trailing edge of a compact AR destabilizes and erupts, followed by what looks like a similar eruption (but with no obvious filament) in the region leading the AR. As the first filament erupts, robbons form around the leading configuration, suggestion couplings not readily seen in the loop patterns....

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

Detected by schryver, Submitted at 2014-03-12T21:05:49

2014-03-10T15:36:03 --> 2014-03-11T00:00:03

A QS filament reaching into the trailing edge of a compact AR destabilizes and erupts, followed by what looks like a similar eruption (but with no obvious filament) in the region leading the AR. As the first filament erupts, robbons form around the leading configuration, suggestion couplings not readily seen in the loop patterns....

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

Detected by schryver, Submitted at 2014-03-12T20:46:11

2014-03-08T18:00:03 --> 2014-03-08T21:50:03

A quiet Sun region shows signs of extensive reconfiguration, with ribbons as expected in a QS filament eruption, but without obvious coronal sinatures of such an eruption.

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

Detected by cheung, Submitted at 2014-02-25T18:02:23

2014-02-25T00:40:03 --> 2014-02-25T01:50:03

A filament destabilizes and is quickly ejected out of the corona. Mid-eruption the filament looks like a bottle opener. Associated with the ejection of the filament is a global coronal wave and flare loops.

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

Detected by cheung, Submitted at 2014-02-25T18:02:22

2014-02-25T00:40:03 --> 2014-02-25T01:50:03

A filament destabilizes and is quickly ejected out of the corona. Mid-eruption the filament looks like a bottle opener. Associated with the ejection of the filament is a global coronal wave and flare loops.

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

Detected by cheung, Submitted at 2014-02-25T18:02:21

2014-02-25T00:40:03 --> 2014-02-25T01:50:03

A filament destabilizes and is quickly ejected out of the corona. Mid-eruption the filament looks like a bottle opener. Associated with the ejection of the filament is a global coronal wave and flare loops.

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

Detected by halocme, Submitted at 2014-02-18T01:18:46

2014-02-16T09:10:11 --> 2014-02-16T10:00:35

The flare was of short duration. In the GOES X-ray light curve, (start, peak, end) = (09:20, 09:26, 09:29). But it launched a nice large-scale coronal propagating front (LCPF) or EUV wave, which was quite fast, e.g., 1000 km s(-1). Apparently, it was also associated with a CME, that at least initially looked like a halo.