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 2015-12-06T06:14:29

2015-12-02T04:20:22 --> 2015-12-02T05:30:22

Another C-class flare in AR 12458. Compared with the previous one on Dec 1 at 08:10 (C3.6), the eruptive signatures are significantly suppressed even though we see overlying coronal structures open up (producing minor dimming) and post-eruption arcades form. LASCO images show a diffuse outflow which can hardly be a CME.

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

Detected by halocme, Submitted at 2015-12-02T03:26:21

2015-12-01T07:45:34 --> 2015-12-01T09:00:34

This flare in AR 12458 accompanied fast-mode MHD waves, seen as a large-scale coronal propagating front (LCPF) both on disk and over the limb and narrow wave trains in the direction of 1 o'clock. Possibly because of the well-connected location, an electron event was observed by ACE/EPAM (but not protons).

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

Detected by halocme, Submitted at 2015-12-02T03:26:21

2015-12-01T07:45:34 --> 2015-12-01T09:00:34

This flare in AR 12458 accompanied fast-mode MHD waves, seen as a large-scale coronal propagating front (LCPF) both on disk and over the limb and narrow wave trains in the direction of 1 o'clock. Possibly because of the well-connected location, an electron event was observed by ACE/EPAM (but not protons).

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

Detected by cheung, Submitted at 2015-11-24T22:52:04

2015-11-22T07:00:06 --> 2015-11-22T11:00:06

Much of the material in this confined/failed filament eruption seem to drain back toward the solar chromosphere. Bright loop footpoints at the western edge of the filament system are seen to light up as a consequence of mass drainage.

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

Detected by cheung, Submitted at 2015-11-24T22:43:36

2015-11-18T21:00:06 --> 2015-11-19T04:10:06

This filament eruption seems to lose steam before material is able to be ejected out of the Sun's gravitational well. Most of the filament material seems to disappear in-situ or or to drain down along loops.

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

Detected by cheung, Submitted at 2015-11-24T22:36:47

2015-11-18T17:56:06 --> 2015-11-18T19:06:06

The erupting material exhibits apparent unwinding motion.

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

Detected by halocme, Submitted at 2015-11-15T08:11:03

2015-11-13T21:55:10 --> 2015-11-13T22:45:10

The eruption was narrow, but it imacted the overlying corona. Around the same time, a region to the northeast also gave a minor rruption. Perhaps it was by coincidence.

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

Detected by halocme, Submitted at 2015-11-15T08:11:02

2015-11-13T21:55:10 --> 2015-11-13T22:45:10

The eruption was narrow, but it imacted the overlying corona. Around the same time, a region to the northeast also gave a minor rruption. Perhaps it was by coincidence.

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

Detected by halocme, Submitted at 2015-11-15T07:54:54

2015-11-12T12:50:22 --> 2015-11-12T16:30:22

This activity led the prominence to disappear. This seems to have had no impact in the corona.

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

Detected by halocme, Submitted at 2015-11-15T07:46:50

2015-11-11T19:50:22 --> 2015-11-11T22:40:22

The diffuse front above the limb without a cool prominence indicates that there is an eruption on the backside.

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

Detected by halocme, Submitted at 2015-11-15T07:35:17

2015-11-10T16:40:10 --> 2015-11-10T17:50:10

A jet containing cool material that is seen in 304 A images. The event may be related to the motions in the circular filament.

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

Detected by halocme, Submitted at 2015-11-15T07:35:16

2015-11-10T16:40:10 --> 2015-11-10T17:50:10

A jet containing cool material that is seen in 304 A images. The event may be related to the motions in the circular filament.

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

Detected by halocme, Submitted at 2015-11-15T07:27:14

2015-11-10T13:50:22 --> 2015-11-10T16:50:22

No front was seen in 211 A images, consistent with no CME in LASCO data.

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

Detected by halocme, Submitted at 2015-11-15T07:18:12

2015-11-10T07:20:22 --> 2015-11-10T07:59:34

Essentially a repeat of the previous event (2015-11-09 16:25), but the oscillations less clear.

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

Detected by halocme, Submitted at 2015-11-15T07:18:11

2015-11-10T07:20:22 --> 2015-11-10T07:59:34

Essentially a repeat of the previous event (2015-11-09 16:25), but the oscillations less clear.

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

Detected by halocme, Submitted at 2015-11-15T01:51:55

2015-11-09T12:30:34 --> 2015-11-09T14:30:34

This is a big eruption resulting in a partial halo CME. A large-scale coronal propagating front (LCPF) is seen, but it mostly goes to the radial direction due to the coronal hole to the west.

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

Detected by halocme, Submitted at 2015-11-15T01:41:37

2015-11-10T01:45:34 --> 2015-11-10T02:41:34

Essentially a repeat of the previous event (2015-11-09 16:25).

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

Detected by halocme, Submitted at 2015-11-15T01:41:37

2015-11-10T01:45:34 --> 2015-11-10T02:41:34

Essentially a repeat of the previous event (2015-11-09 16:25).

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

Detected by halocme, Submitted at 2015-11-15T01:37:03

2015-11-09T16:25:10 --> 2015-11-09T17:01:10

A confined eruption appears to trace closed structures, causing them to oscillate.

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

Detected by halocme, Submitted at 2015-11-15T01:37:03

2015-11-09T16:25:10 --> 2015-11-09T17:01:10

A confined eruption appears to trace closed structures, causing them to oscillate.