Recent Events Reported by Observers

Detected by schryver, Submitted at 2016-01-13T20:32:32

2016-01-12T05:48:06 --> 2016-01-12T11:08:06

Eruption from a region of mixed-polarity enhanced network, apparently creating a temporary void in the coronal connections into long loops connecting to quiet Sun.

Detected by cheung, Submitted at 2016-01-12T02:59:47

2016-01-09T13:34:06 --> 2016-01-09T14:40:06

This mini-filament eruption leads to a blow out jet. During the eruption the filament material seems to be torn apart and slamed into a magnetic wall.

Detected by cheung, Submitted at 2016-01-12T02:59:46

2016-01-09T13:34:06 --> 2016-01-09T14:40:06

This mini-filament eruption leads to a blow out jet. During the eruption the filament material seems to be torn apart and slamed into a magnetic wall.

Detected by schryver, Submitted at 2016-01-11T19:00:20

2016-01-10T01:58:18 --> 2016-01-10T02:46:18

QS filament activation, with apparent ribbons, but no signs of eruption.

Detected by weiliu, Submitted at 2016-01-09T01:37:16

2015-12-25T00:00:06 --> 2015-12-26T00:00:06

coronal rain occurred near a possible dip in the loops, and slides down loops...

Detected by weiliu, Submitted at 2016-01-09T01:31:03

2015-12-25T06:40:06 --> 2015-12-25T07:50:06

Surge like sudden flow in a filament near an AR.

Detected by weiliu, Submitted at 2016-01-09T01:27:17

2015-12-25T03:50:06 --> 2015-12-25T05:30:06

A surge like eruption has a circular shape developing, together with remote brightenings next to a nearby AR (to the southwest of the main eruption). The whole thing appears to be aligned along a structure, in a fashion similar to a filament channel.

Detected by weiliu, Submitted at 2016-01-09T01:12:50

2015-12-25T17:00:06 --> 2015-12-25T18:30:06

An active region filament kinked and disrupted (but material falls back), causing flaring brightening.

Detected by cheung, Submitted at 2016-01-07T22:54:37

2016-01-07T10:00:06 --> 2016-01-07T20:00:06

Coronal cavity above a filament off the west limb

Detected by cheung, Submitted at 2016-01-07T22:54:36

2016-01-07T10:00:06 --> 2016-01-07T20:00:06

Coronal cavity above a filament off the west limb

Detected by halocme, Submitted at 2016-01-07T05:56:19

2016-01-06T12:00:06 --> 2016-01-06T13:00:06

The initial part of an eruption is captured. EUVI-A images indicated that it was from AR 12473, now more than 40 degrees behind the limb. The eruption produced a bright partial halo CME with shock signatures, but unfortunately we did not see the details after the onset because of EVE FOV maneuver (13:15-16:00 UT)

Detected by halocme, Submitted at 2016-01-07T05:48:29

2016-01-06T10:00:06 --> 2016-01-06T13:00:06

A small filament erupted from a quiescent region, showing coronal dimming at high altitudes and formation of two-ribbon flare emission. It resulted in a slow CME.

Detected by halocme, Submitted at 2016-01-07T05:48:29

2016-01-06T10:00:06 --> 2016-01-06T13:00:06

A small filament erupted from a quiescent region, showing coronal dimming at high altitudes and formation of two-ribbon flare emission. It resulted in a slow CME.

Detected by halocme, Submitted at 2016-01-07T05:42:37

2016-01-05T02:30:34 --> 2016-01-05T05:30:34

This was likely to be associated with AR 12473, which was already 25-30 degrees behind the limb. The eruption shows helical motions and the overlying corona is seen to dim. It resulted in a narrow CME.

Detected by halocme, Submitted at 2016-01-07T05:42:36

2016-01-05T02:30:34 --> 2016-01-05T05:30:34

This was likely to be associated with AR 12473, which was already 25-30 degrees behind the limb. The eruption shows helical motions and the overlying corona is seen to dim. It resulted in a narrow CME.

Detected by halocme, Submitted at 2016-01-07T05:36:30

2016-01-04T10:40:10 --> 2016-01-04T16:00:10

This was a diffuse eruption, but two-ribbon-like emission was clearly seen northwest of the filament.

Detected by halocme, Submitted at 2016-01-07T05:30:53

2016-01-03T09:00:06 --> 2016-01-03T12:00:06

The southeastern part of AR 12473 hosted a filament that erupted. It did not give much impact on the overlying coronal structures.

Detected by halocme, Submitted at 2016-01-07T05:25:29

2016-01-03T02:30:34 --> 2016-01-03T04:30:34

Similar pattern to the previous event in AR 12473.

Detected by halocme, Submitted at 2016-01-07T05:21:47

2016-01-02T22:40:10 --> 2016-01-02T23:30:10

Eruption or double sided flow, that is, toward west and higher and toward southeast and lower. AR 12473 has repeatedly shown this pattern.

Detected by halocme, Submitted at 2016-01-06T05:49:10

2016-01-01T00:00:06 --> 2016-01-06T00:00:06

Many brightenings were seen inside the dark coronal hole, but this five-day movie does not readily indicate dynamic evolution of the coronal hole boundary. This coronal hole was likely responsible for the fast (>600 km/s) solar wind that started around 01 UT on 2016-01-06.