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 2013-06-09T04:31:35

2013-06-07T15:30:35 --> 2013-06-08T00:30:35

The mateial is seen to drain mostly into the northern leg, giving an impression of motions in counterclockwise during this period. No impact on background corona.

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

Detected by halocme, Submitted at 2013-06-09T04:12:46

2013-06-07T15:30:35 --> 2013-06-07T17:00:35

Actions in low-lying loops (in the southern part of the encircled area) cause material to be ejected to northwest. Increased emission is seen in 193 A + 211 A, but it is in depression in 171 A, suggestive of heaitng.

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

Detected by halocme, Submitted at 2013-06-09T04:01:02

2013-06-07T08:30:35 --> 2013-06-07T13:00:35

The prominence material is ejected from the northern leg. Instead of travelling into the heliosphere, most of it seems to come back to the Sun's atmosphere. Although the rising phase reflects a possibly complicated magnetic field structure, the falling-back motion is more orderly, along closed loops with a compact footpoint area.

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

Detected by halocme, Submitted at 2013-06-09T03:40:30

2013-06-07T00:40:11 --> 2013-06-07T01:40:11

The footpoint is clearly on the visible side. This jet is hard to see in 171 A channel.

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

Detected by halocme, Submitted at 2013-06-09T03:31:51

2013-06-06T22:00:03 --> 2013-06-07T00:10:03

Initially a set of loops expands or rises westward, then simultaneous with brightening of low-lying loops (encircled) another set of loops erupts, mostly soutward (around 23:00 UT).

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

Detected by derosa, Submitted at 2013-06-09T00:11:30

2013-06-05T06:00:03 --> 2013-06-05T12:00:03

Eruption associated with an M flare that occurred in AR11762.

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Detected by derosa, Submitted at 2013-06-08T23:58:27

2013-06-04T10:00:03 --> 2013-06-05T15:00:03

Nice example of metter swirling in the curvwed magnetic field associated with a filament/prominence on the west limb. For the better part of a day, matter continually is pulled into the field overlying the filament, which we view as swirling motions above the limb.

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

Detected by derosa, Submitted at 2013-06-08T23:41:37

2013-06-04T13:00:03 --> 2013-06-04T18:00:03

Filament/prominence eruption on the northeast limb. Both ends of the filament disconnect almost simultaneously.

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

Detected by halocme, Submitted at 2013-06-08T01:09:41

2013-06-03T14:30:35 --> 2013-06-03T15:50:35

Part of the big filament that had been hanging around for a while now rotates beyond the west limb. The motions captured in this movie are suggestive of a twisted structure.

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

Detected by halocme, Submitted at 2013-06-08T01:01:18

2013-06-03T06:00:04 --> 2013-06-03T08:00:04

Following B-class flares to northeast that are associated with compact dimming, the C9.5 flare may also look eruptive in the sense that a dark loop-like structure moves out (in the box). However, this event has no trace in LASCO data.

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

Detected by halocme, Submitted at 2013-06-07T22:59:05

2013-06-03T00:00:03 --> 2013-06-03T01:10:03

EUVI data from STEREO-A show that the footpoints of the eruption are more than 30 degrees behind the limb, but the CME is inclined to east (on the basis of EUV waves), and what we see in the movie may come from only 10 degrees or less behind the limb.

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

Detected by halocme, Submitted at 2013-06-07T22:27:26

2013-06-02T23:30:35 --> 2013-06-03T00:40:35

This is almost a repeat of the previously reported event ("Mild eruption" whose time range started at 2013-06-02T14:30:35.), perhaps on a smaller scale.

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

Detected by halocme, Submitted at 2013-06-07T19:44:27

2013-06-02T14:30:35 --> 2013-06-02T15:30:35

Another mild eruption showing disturbances beyond active region scales. Even if the eruption is minor, a CME-like front is seen to form when it is observed as a limb event (by STEREO-B). The front can be traceable only to 1.32 Rs, however.

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

Detected by halocme, Submitted at 2013-06-07T05:44:03

2013-06-01T11:45:35 --> 2013-06-01T12:45:35

The eruption appears rather diffuse, but it is clearly there, even showing loop oscillations. Based on EUVI data from STEREO-A, the footpoints are about 10 degrees behind the limb. The eruption is short-lived and does not make it into the heliosphere.

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

Detected by halocme, Submitted at 2013-06-07T03:28:57

2013-06-01T00:30:35 --> 2013-06-01T03:30:35

Just a minor one. It is not clear how the jet-lik brightenings in the western area have to do with the mass falling back.

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

Detected by halocme, Submitted at 2013-06-07T03:17:57

2013-05-25T21:00:35 --> 2013-05-25T22:00:35

A small area above the limb brightens for short time. Shortly before, an eruption is seen on disk. Is it possible that this eruption is related to the brightening above the limb? This is at 304 A only.

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

Detected by halocme, Submitted at 2013-06-07T03:02:31

2013-05-25T08:40:11 --> 2013-05-25T09:40:11

Small mass ejection is seen from a minor region. At 304 A, it started as emission in 304 A and then turn to absorption, shadowing a bright region on its passage.

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

Detected by halocme, Submitted at 2013-06-07T02:54:46

2013-05-25T01:20:23 --> 2013-05-25T02:40:23

Material is injected from south and reaches the northern end of the structure, which seems to be quite complex on the basis of the trajectory of the material. There is no indication that this is an eruption.

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

Detected by halocme, Submitted at 2013-06-07T02:47:51

2013-05-24T20:30:35 --> 2013-05-24T22:00:35

Material is ejected from the northern leg of a closed structure. Part of it is returned, another part to the southen leg, and small part escaped. The response of the adjacent corona was negligible.

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

Detected by halocme, Submitted at 2013-06-07T02:34:26

2013-05-24T15:50:23 --> 2013-05-24T17:20:23

This is not disruptive, but it slowly pulls loops from the eastern part of the region to to open up.