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

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

Detected by anny, Submitted at 2014-02-01T00:22:16

2014-01-26T01:12:03 --> 2014-01-26T04:06:03

Some explosive activity along a filament on the SW disk.

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

Detected by anny, Submitted at 2014-02-01T00:09:07

2014-01-25T00:00:03 --> 2014-01-26T00:00:03

A prominence forms at the N limb. A visually small fraction of it then gets ejected, while the rest falls back on the surface as coronal rain.

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

Detected by derosa, Submitted at 2014-01-25T03:07:08

2014-01-18T05:00:03 --> 2014-01-18T22:00:03

Prominence material is observed to flow from one place to another. Simultaneously, a coronal cavity [as evident from the curved lower boundary evident in the ramped-up 171 channel] is observed to lift off. These dynamics do not appear to be associated with any explosive event; rather it appears to be more of a slowly evolving ejection that is proceeds via the gradual expansion of coronal plasma.

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

Detected by derosa, Submitted at 2014-01-25T03:07:07

2014-01-18T05:00:03 --> 2014-01-18T22:00:03

Prominence material is observed to flow from one place to another. Simultaneously, a coronal cavity [as evident from the curved lower boundary evident in the ramped-up 171 channel] is observed to lift off. These dynamics do not appear to be associated with any explosive event; rather it appears to be more of a slowly evolving ejection that is proceeds via the gradual expansion of coronal plasma.

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

Detected by schryver, Submitted at 2014-01-22T16:24:15

2014-01-21T07:52:03 --> 2014-01-21T11:16:03

Filament eruption

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

Detected by derosa, Submitted at 2014-01-21T03:32:49

2014-01-16T10:00:03 --> 2014-01-16T17:00:03

Filament on southwest limb activates. Some material is observed to stream down toward photosphere. It is unclear whether material was also ejected upward.

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

Detected by weiliu, Submitted at 2014-01-18T03:50:09

2013-12-18T04:40:03 --> 2013-12-18T06:00:03

Surge from active region

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

Detected by weiliu, Submitted at 2014-01-18T03:44:13

2013-12-18T06:40:03 --> 2013-12-18T07:40:03

A moderate surge from an active region.

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

Detected by cheung, Submitted at 2014-01-17T02:06:35

2014-01-15T22:30:03 --> 2014-01-16T01:45:03

Filament material seems to corkscrew along some field lines before draining back.

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

Detected by halocme, Submitted at 2014-01-09T08:48:15

2013-12-25T16:30:35 --> 2013-12-25T18:00:35

Following a small-scale eruption, larger-scale loops are pushed sideways. This seems to correspond to an unimpressive CME observed at 18:00 UT.

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

Detected by halocme, Submitted at 2014-01-09T08:38:03

2013-12-24T09:15:35 --> 2013-12-24T11:15:35

As the prominence erupts, it appears to deflect southward. The prominence itself seems to have complex internal structures.

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

Detected by halocme, Submitted at 2014-01-09T08:27:02

2013-12-24T02:50:23 --> 2013-12-24T05:00:23

This is again searched from CME observations. The source region could be far behind the limb.

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

Detected by halocme, Submitted at 2014-01-09T08:15:44

2013-12-24T01:30:35 --> 2013-12-24T03:10:35

Because of a LASCO CME, we know something occurred around the position angle of 240 degrees (measured counterclockwise from the north pole). In this case the eruption was clearly on the far side. The most apparent signature is oscillations of coronal structures.

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

Detected by halocme, Submitted at 2014-01-09T08:15:42

2013-12-24T01:30:35 --> 2013-12-24T03:10:35

Because of a LASCO CME, we know something occurred around the position angle of 240 degrees (measured counterclockwise from the north pole). In this case the eruption was clearly on the far side. The most apparent signature is oscillations of coronal structures.

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

Detected by halocme, Submitted at 2014-01-09T08:05:06

2013-12-23T07:00:35 --> 2013-12-23T20:00:35

The north and south polar regions seem to host prominence activities in this time frame.

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

Detected by halocme, Submitted at 2014-01-09T07:58:59

2013-12-23T07:20:23 --> 2013-12-23T10:00:23

This prominence eruption suggests the presence of helical structures at both high and low altitudes. The associated CME was narrow but of flux-rope type.

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

Detected by halocme, Submitted at 2014-01-09T07:44:34

2013-12-22T18:00:03 --> 2013-12-23T03:00:03

This seems to be a prominence close to the north pole, indicating the presence of mixed polarity. No corresponding signatures are found in lower latitude regions.

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

Detected by halocme, Submitted at 2014-01-09T07:36:49

2013-12-22T23:50:23 --> 2013-12-23T01:20:23

This flare is again characterized by the surge-like ejection, dark in 211 A and 171 A. It was immediately followed by a M-class flare somewhere else, and not registered as a separate event. A bright CME was associated, which started narrow but later became extended.

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

Detected by halocme, Submitted at 2014-01-09T07:36:48

2013-12-22T23:50:23 --> 2013-12-23T01:20:23

This flare is again characterized by the surge-like ejection, dark in 211 A and 171 A. It was immediately followed by a M-class flare somewhere else, and not registered as a separate event. A bright CME was associated, which started narrow but later became extended.

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

Detected by halocme, Submitted at 2014-01-09T07:20:49

2013-12-22T18:50:23 --> 2013-12-22T21:00:23

This C6.1 flare is characterized by fast collimated ejections. A narrow (not flux-rope type) CME was already observed by LASCO at 19:48 UT.