Recent Events Reported by Observers

Detected by Jakub Prchlik, Submitted at 2016-07-29T13:45:52

2014-09-14T00:12:55 --> 2014-09-14T00:21:09

Low intensity flare observed in 1330 and 2796 A. AIA 131 also detects the flare event, but does not classify the flare.

Detected by Jakub Prchlik, Submitted at 2016-07-29T13:20:09

2014-09-11T07:54:26 --> 2014-09-11T10:59:50

A peacock tail visible in 1330, 1400, and 2796 A lasts the entire observation. 1330, 1400, and 2796 also show an eruption, which last from 10:28 to 10:49. The eruption does not affect the peacock tail's intensity.

Detected by Jakub Prchlik, Submitted at 2016-07-29T12:45:30

2014-09-09T12:15:06 --> 2014-09-09T12:34:12

A C 3.2 flare that crosses the slit (2-3 frames after peak intensity).

Detected by Jakub Prchlik, Submitted at 2016-07-28T21:07:30

2014-10-09T18:24:55 --> 2014-10-09T21:57:24

Prominence initial fades until a nearby eruption occurs. After the eruption, the prominence increases in intensity. Soon after the coronal rain from the eruption ceases, the prominence again fades. This process is visible in 1400 A and 2796 A and crossed by the slit.

Detected by Jakub Prchlik, Submitted at 2016-07-28T20:55:10

2014-10-12T00:00:00 --> 2014-10-12T04:04:39

Prominence visible in 1400 A and 2796 A but not in 2832 A. The prominence evolves from horned to arch-like during the observation, however, this may be due to perspective.

Detected by Jakub Prchlik, Submitted at 2016-07-28T20:41:07

2014-10-11T19:02:25 --> 2014-10-11T19:55:07

Two eruptions in the image's upper left corner cause coronal rain. The coronal rain crosses the slit near the rain event's base. Both 1330 A and 1400 A easily show the event, while 2796 A shows minimal contrast with the background.

Detected by Jakub Prchlik, Submitted at 2016-07-28T20:21:00

2014-10-10T15:03:01 --> 2014-10-10T17:35:31

Three distinct eruption events occur in the same location. Both 1330 A and 2796 A show the eruptions. The final eruption is the brightest in both wavelengths.

Detected by Jakub Prchlik, Submitted at 2016-07-28T20:01:56

2014-10-08T14:19:38 --> 2014-10-08T16:42:28

Peacock tails last the entire observation in both 1330 A and 2796 A. Both 1330 A and 2796 A also show a coronal jet near the observation's end. However, the jet is in emission in 1330 A, but in absorption in 2796 A. Also, there is an eruption near the bottom of the image, which crosses the slit for the last half of the observation.

Detected by Jakub Prchlik, Submitted at 2016-07-28T19:28:26

2016-04-28T09:53:52 --> 2016-04-28T10:08:49

Jet protrudes from the coronal hole's edge. Both 1330 and 1400 A show the event, but it is brightest in 1400 A. However, neither 2796 or 2832 A show activity.

Detected by Jakub Prchlik, Submitted at 2016-07-28T19:11:01

2016-04-26T04:19:23 --> 2016-04-26T05:32:37

A peacock tail wall just to the right of the observation's center. The observation also shows a few other peacock tail structures scattered about the bright active region.

Detected by Jakub Prchlik, Submitted at 2016-07-28T18:59:27

2016-05-01T12:25:15 --> 2016-05-01T12:50:25

Off limb coronal rain at the bottom right image corner. The event is visible in 1330, 1400, and 2796 A, however, it is strongest in 1400 A.

Detected by Jakub Prchlik, Submitted at 2017-07-24T06:32:21

2016-02-18T07:44:11 --> 2016-02-18T09:04:02

Multiple edge on jets span the active region. Many of the jets cross the slit.

Detected by jinmeng, Submitted at 2016-08-01T18:15:38

2016-07-26T02:30:06 --> 2016-07-27T02:30:06

Several eruptions occurred near the west limb. Most of them are from AR 12568(?). The disturbances from the eruptions seem to cause a filament eruption to the south at last.

Detected by jinmeng, Submitted at 2016-08-01T18:15:38

2016-07-26T02:30:06 --> 2016-07-27T02:30:06

Several eruptions occurred near the west limb. Most of them are from AR 12568(?). The disturbances from the eruptions seem to cause a filament eruption to the south at last.

Detected by jinmeng, Submitted at 2016-08-01T18:15:38

2016-07-27T05:30:06 --> 2016-07-27T22:20:06

An eruption behind the east limb. ~8 hours before the final eruption, coronal loops were observed slowly rising up (some of them may become open). The global change of the corona may lead to the final eruption.

Detected by jinmeng, Submitted at 2016-07-26T22:54:29

2016-07-23T03:40:06 --> 2016-07-23T10:30:06

EUV waves associated with the eruption from AR 12565.

Detected by jinmeng, Submitted at 2016-07-26T23:27:06

2016-07-23T03:40:06 --> 2016-07-23T10:30:06

Two flares are observed close in time from AR 12565. The first one seems non-eruptive and the second one released large amount of material into the corona. Part of the filament material came back after the eruption.

Detected by jinmeng, Submitted at 2016-07-26T23:27:06

2016-07-22T04:50:06 --> 2016-07-22T18:30:06

A filament eruption occurred near the east limb. The eruption also affected another nearby filament but did not make it to erupt.

Detected by jinmeng, Submitted at 2016-07-26T22:25:52

2016-07-20T22:00:06 --> 2016-07-21T07:00:06

An eruptive from AR 12567. An M1.0 flare is associated with this eruption.

Detected by jinmeng, Submitted at 2016-07-26T22:14:54

2016-07-21T15:20:06 --> 2016-07-22T00:00:06

Flux emergence from south polar region, which leads to the brightening of a small region.