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 2019-11-12T04:01:54

2019-10-30T12:45:01 --> 2019-10-30T13:30:37

Another example of a polar jet that seems to involve cool filament material.

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

Detected by halocme, Submitted at 2019-11-12T01:43:39

2019-10-29T14:55:13 --> 2019-10-29T15:55:13

This appears to involve a mini-filament.

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

Detected by halocme, Submitted at 2019-11-12T01:37:55

2019-10-28T03:10:13 --> 2019-10-28T05:00:37

A prominence is seen to erupt, reaching a certain height, but there is no sign at 211 A that the overlying corona is affected. This is likely a confined eruption, and indeed there was no CME.

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

Detected by halocme, Submitted at 2019-11-12T01:31:09

2019-10-27T18:25:13 --> 2019-10-27T20:06:01

This gives an impression that the eruption started above the bright loops. There was no associated CME.

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

Detected by halocme, Submitted at 2019-11-12T01:05:37

2019-10-26T11:40:13 --> 2019-10-26T13:10:13

We see two jets. Did the first one lead to the formation of a temporary mini-filament, which triggered the second jet?

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

Detected by halocme, Submitted at 2019-11-12T00:56:35

2019-10-26T09:30:01 --> 2019-10-26T10:40:49

This started as an ejection of cool material in helical motions and then followed large scale structures around what looked like a flux rope.

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

Detected by halocme, Submitted at 2019-11-11T22:09:36

2019-10-25T17:15:01 --> 2019-10-25T18:30:37

This event took place in a quiescent region at high latitude. The motion was highly non-radial. 304 A images indicate the presence of a small filament and cool material in the body of the jet.

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

Detected by halocme, Submitted at 2019-11-11T18:10:27

2019-10-24T15:35:25 --> 2019-10-24T16:45:01

This occurred in a quiescent region (no AR anyway). The trajectory seems to be affected by adjacent coronal structures.

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

Detected by gchintzo, Submitted at 2019-11-07T01:57:37

2019-11-06T01:40:09 --> 2019-11-06T21:00:09

A cavity on the north west limb expands and moves southward. Note a faint cavity from the same location that exhibits the same behavior.

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

Detected by gchintzo, Submitted at 2019-11-07T00:51:59

2019-11-02T00:00:09 --> 2019-11-04T19:00:09

This AR exhibits an inverse polarity orientation (as compared to the hemispheric rule). This fact, combined with the high latitude of this AR suggests that Cycle 25 has just started

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

Detected by gchintzo, Submitted at 2019-10-16T17:38:00

2019-10-15T05:50:09 --> 2019-10-15T19:10:09

A coronal cavity seen rolling from high latitude to low latitude and dissipate in the east limb of the sun

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

Detected by halocme, Submitted at 2019-07-26T00:43:20

2019-07-23T22:10:13 --> 2019-07-24T00:10:13

One of those mini-filament eruptions that can easily be seen even during solar minimum.

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

Detected by gchintzo, Submitted at 2019-07-19T21:50:18

2019-07-13T19:10:09 --> 2019-07-14T11:10:09

An eruption from decaying NOAA AR12744. Note the orientation and tilt of the polarities (red negative, green positive) with respect to the local latitude (30 deg south) which suggests the AR belongs to the new solar cycle 25. The eruption was recorded in the LASCO coronagraphic observations (355 km sec-1; http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20190714.040007.w011.v0355.p245&frame=2&r)

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

Detected by halocme, Submitted at 2019-07-10T07:42:46

2019-07-08T19:00:09 --> 2019-07-08T20:30:09

A prominence was deformed when the eruption from the south arrived, starting a slow oscillation.

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

Detected by halocme, Submitted at 2019-07-10T07:42:38

2019-07-08T19:00:09 --> 2019-07-08T20:30:09

A prominence was deformed when the eruption from the south arrived, starting a slow oscillation.

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

Detected by halocme, Submitted at 2019-07-10T07:34:37

2019-07-08T00:25:13 --> 2019-07-08T02:15:13

This jet was seen to propagate in a no-radial direction. It had an appearance of containing a flux rope.

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

Detected by halocme, Submitted at 2019-07-10T07:29:46

2019-07-07T07:55:13 --> 2019-07-07T09:21:13

Small eruption that looked explosive from a region with the new solar cycle polarity arrangement (but not making it to a sunspot active region).

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

Detected by halocme, Submitted at 2019-05-29T07:07:11

2019-05-25T21:15:01 --> 2019-05-25T23:01:01

The eruption occurred in what could be considered a coronal bright point (although it was largish). The area south of the region dimmed temporarily.

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

Detected by halocme, Submitted at 2019-05-29T06:55:30

2019-05-25T05:05:25 --> 2019-05-25T06:45:25

The eruption likely occurred on the backside. It appeared to trigger another one to the north on the visible side.

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

Detected by halocme, Submitted at 2019-05-29T06:49:11

2019-05-23T06:40:13 --> 2019-05-23T07:30:37

This jet contains cool material initially ejected in helical motions.