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 2013-10-15T03:19:12

2013-10-12T13:00:03 --> 2013-10-12T16:00:03

The eruption of the bright prominence in 304 A images does not give an impression that it made it to the heliosphere, but at least a real CME with internal structures, although slow, seems to be associated. Closed loops to the south expanded before the prominence eruption, and they hardly reached the LASCO FOV.

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

Detected by halocme, Submitted at 2013-10-14T22:32:57

2013-10-11T15:00:11 --> 2013-10-11T18:00:11

There is no associated feature on the visible disk (such as post-eruption arcades), so this diffuse eruption (found only in difference movies) is probably from the backside.

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

Detected by anny, Submitted at 2013-10-11T23:40:31

2013-10-07T06:57:35 --> 2013-10-07T19:51:35

A massive prominence slowly rotates onto the visible disk. It is unclear whether it is the same structure as the filament on the disk; on visual impression it seems that they are the same structure. The reason I'm annotating this structure is because how clearly its structure shows up on this movie.

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

Detected by anny, Submitted at 2013-10-11T23:40:30

2013-10-07T06:57:35 --> 2013-10-07T19:51:35

A prominence at the NW limb expands in size until it turns into an umbrella-like structure. Due to the gap in the data, it is not clear whether it erupts or not. After the data coverage is resumed, the "umbrella" is gone.

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

Detected by anny, Submitted at 2013-10-11T23:40:29

2013-10-07T06:57:35 --> 2013-10-07T19:51:35

A prominence at the NW limb expands in size until it turns into an umbrella-like structure. Due to the gap in the data, it is not clear whether it erupts or not. After the data coverage is resumed, the "umbrella" is gone.

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

Detected by anny, Submitted at 2013-10-11T23:40:27

2013-10-07T05:21:35 --> 2013-10-07T11:03:35

A nice example of a single, isolated coronal droplet traveling along an arch slightly the SE limb.

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

Detected by anny, Submitted at 2013-10-11T21:50:08

2013-10-06T18:06:03 --> 2013-10-06T23:03:03

Two small prominences and the associated cavities erupt almost simultaneously. Can these be different parts of the same erupted structure? The event is followed by some reconfiguration of loops in an active region between the sites of the eruptions.

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

Detected by halocme, Submitted at 2013-10-11T16:57:46

2013-10-11T07:00:07 --> 2013-10-11T09:00:07

The front is seen mostly along the limb (largely counterclockwise), although we also note disturbances on disk. The flare region seems to be slightly behind the limb. Empirically, a LCPF and eruption of this scale (including oscillations of trans-equatorial loops) accompanies a fast and wide CME, although no LASCO data are seen for this event as of now thanks to the government shutdown.

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

Detected by anny, Submitted at 2013-10-10T00:34:59

2013-10-05T07:09:03 --> 2013-10-05T21:00:03

A prominence at the N limb swirls around and eventually falls on the surface as coronal rain.

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

Detected by anny, Submitted at 2013-10-10T00:29:57

2013-10-05T06:54:03 --> 2013-10-05T08:57:03

A cavity eruption in 211A channel is coincidental with a strong spray surge at one of the footpoints of the loops surrounding the cavity

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

Detected by anny, Submitted at 2013-10-10T00:29:56

2013-10-05T06:54:03 --> 2013-10-05T08:57:03

A cavity eruption in 211A channel is coincidental with a strong spray surge at one of the footpoints of the loops surrounding the cavity

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

Detected by halocme, Submitted at 2013-10-09T15:25:20

2013-10-06T13:00:03 --> 2013-10-06T17:00:03

This may not look like a major eruption. It is associated with a modest C1.1 LDE. However, it is associated with the only halo CME during the interval that can be responsible for the moderate storm that started late on 8 October 2013 (KP=5). The CME is quite diffuse with the northern part being more visible in spite of the location of the eruption (AR 1859, a good number for a geoeffective event). There is no clear filament eruption in 304 A images.

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

Detected by halocme, Submitted at 2013-10-07T15:12:20

2013-10-05T04:00:03 --> 2013-10-05T08:00:03

The eruptive signatures are clearly noted in AIA images even though the source region is estimated to be more than 30 degrees behind the limb. The event is associated with a type II radio burst (both metric and DH), and a halo CME. Based on the LASCO MVI files archived at NRL (no movies available at GSFC because of the goverment shutdown), the bright CME is first observed at 07:10 (at the heliocentric distance of 2.8-2.9 Rs and PA of 125 deg), and the linear speed is only about 630 km/s using five difference images.

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

Detected by halocme, Submitted at 2013-10-07T15:12:13

2013-10-05T04:00:03 --> 2013-10-05T08:00:03

The eruptive signatures are clearly noted in AIA images even though the source region is estimated to be more than 30 degrees behind the limb. The event is associated with a type II radio burst (both metric and DH), and a halo CME. Based on the LASCO MVI files archived at NRL (no movies available at GSFC because of the goverment shutdown), the bright CME is first observed at 07:10 (at the heliocentric distance of 2.8-2.9 Rs and PA of 125 deg), and the linear speed is only about 630 km/s using five difference images.

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

Detected by weiliu, Submitted at 2013-10-01T23:51:21

2013-09-30T17:30:03 --> 2013-09-30T18:40:03

An interesting surge with part of it following a loop-shaped trajectory (likely guieded by coronal loops), and another part of it returning along the original path of ascent close to the local vertical.

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

Detected by weiliu, Submitted at 2013-10-01T23:27:11

2013-09-29T10:40:03 --> 2013-09-29T12:10:03

A surge likely associated with a behind-the-limb eruption on the east limb. Note the wavy trajectory of the ejected material.

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

Detected by derosa, Submitted at 2013-10-01T00:26:43

2013-09-28T08:00:03 --> 2013-09-28T12:00:03

Two small and not-really-very exciting filament activations on/near the east limb are notable only for the fact they are nearly simultaneous. I leave open the question as to whether they are causally related.

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

Detected by halocme, Submitted at 2013-10-01T00:10:39

2013-09-29T21:00:35 --> 2013-09-29T23:59:59

Someone asked the space weather forum if the Sun is dead, but this is the first major eruption in weeks. As expected, a halo CME is associated. LASCO saw its first sign at 22:12 UT. It is probably Earth-directed, and several heliospheric predictions will be made. The associated flare is C1.2.

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

Detected by schryver, Submitted at 2013-09-25T21:06:24

2013-09-23T22:04:03 --> 2013-09-24T00:00:03

Compact eruption from QS with coronal dimmings in adjacent QS corona.

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

Detected by schryver, Submitted at 2013-09-25T21:04:36

2013-09-23T07:00:03 --> 2013-09-23T13:28:03

Quiet-Sun filament eruption from the SW quadrant.