Recent Events Reported by Observers

Detected by Milan Gosic, Submitted at 2016-08-01T04:19:06

2016-07-24T01:09:21 --> 2016-07-24T01:19:56

This C1.9 flare happened on 24-Jul-2016 at 01:09 UT in AR12565. The flare is visible in the lower right part of the movie. The slit does not cover the flaring region.

Detected by Milan Gosic, Submitted at 2016-08-01T03:56:57

2016-07-24T20:57:52 --> 2016-07-25T02:58:37

Coronal rain above AR12567 is formed after an M1.9 class flare occurred on 24-Jul-2017 at 17:30 UT.

Detected by Milan Gosic, Submitted at 2016-08-01T03:51:48

2016-07-24T17:30:49 --> 2016-07-24T18:32:31

This M1.9 class flare happened in AR12567 on 24-Jul-2017 at 17:30 UT. The slit does not cover the flare. At the end of the movie coronal rain caused by this flare can also be seen.

Detected by Nicole Schanche, Submitted at 2016-07-29T21:30:54

2015-05-18T21:02:26 --> 2015-05-18T21:54:58

This small jet occurs at the limb. It seems to be coming from the area of AR12339 after it has rotated behind the limb.

Detected by Jakub Prchlik, Submitted at 2016-07-29T21:15:22

2015-03-01T05:20:52 --> 2015-03-01T05:27:58

Filament eruption observed in 1330, 1400, and 2796 A. The activation starts simultaneously at two locations near the filament's base. Then the activation brakes up into three small streams.

Detected by Jakub Prchlik, Submitted at 2016-07-29T20:56:19

2015-02-28T13:59:08 --> 2015-02-28T14:53:39

Explosive event occurs between two coronal holes. Both 1330 A and 1400 A show two ribbon structures during the event, while the event barely contrasts with the background at 2796 A. The emission in 2796 A does not cross the slit, however, the event does cross the slit in both 1330 A and 1400 A. 2832 A does not observe the event.

Detected by Nicole Schanche, Submitted at 2016-07-29T20:45:52

2015-05-15T14:50:42 --> 2015-05-15T15:28:30

This brightening along the magnetic field line is not associated with a flare event by GOES. It also does not appear to lie within a filament.

Detected by Jakub Prchlik, Submitted at 2016-07-29T20:39:37

2015-02-26T23:39:25 --> 2015-02-27T00:27:46

A slowly building helix shaped explosive event crosses over a sunspot. After peak intensity, the explosive event quickly fades away. The event is visible in 1400 A but not in 2796 A.

Detected by Nicole Schanche, Submitted at 2016-07-29T20:18:48

2015-05-14T21:07:31 --> 2015-05-14T21:22:40

This event looks like the footprint of a small flare or perhaps a jet seen straight on. There is no flare recorded at the time in the NOAA GOES database.

Detected by Nicole Schanche, Submitted at 2016-07-29T20:05:36

2015-05-14T13:49:15 --> 2015-05-14T15:01:22

Two ribbons can be clearly seen in this C2.8 flare. There also appears to be material ejected from the eastern edge of the eruption. However, the FOV is not large enough to see whether the material leaves or falls back down.

Detected by Nicole Schanche, Submitted at 2016-07-29T19:52:37

2015-05-14T02:16:13 --> 2015-05-14T02:58:31

This small brightening appears to be a small flare. However, there was no event identified in the NOAA GOES database.

Detected by Nicole Schanche, Submitted at 2016-07-29T19:31:01

2015-05-13T20:19:19 --> 2015-05-13T21:12:53

This small but complex B4.6 flare occurs in the center of this movie, to the southwest of the main sunspot. The bright region appears twisted. The same region again brightens at the end of this movie, but cuts off before the second brightening is complete.

Detected by Jakub Prchlik, Submitted at 2016-07-29T15:56:45

2014-09-10T16:55:56 --> 2014-09-10T17:57:56

The GOES classified X 1.6 Flare encompasses most of the image and is visible in both 1400 A and 2796 A. The flares starts with two separate ribbons (one in the center and another in the top right), which presumably connect off the image during peak intensity. The central ribbon crosses the slit soon after formation and remains on the slit for the rest of the observation.

Detected by Jakub Prchlik, Submitted at 2016-07-29T14:47:28

2014-09-15T09:53:31 --> 2014-09-15T10:02:19

The filament activation's visibility is function of wavelength. At 1400 A the event produces a bright s-like pattern, which evolves into a high intensity blob. During the activation's peak extent, the activation's edge crosses the slit. However, at 2796 A the activation is only visible as a blob in a small portion 1400 A's active region during peak intensity. The 2796 A emission does not cross the slit. The filament activation is not visible at 2832 A.

Detected by Jakub Prchlik, Submitted at 2016-07-29T14:14:31

2014-09-15T07:08:37 --> 2014-09-15T07:24:52

A strong coronal jet twice originates during eruptions. The jet emits in 1330 A, while in 2796 A the jet is visible in absorption. The slit does not cross the jet, however, the slit does cross the eruptions.

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.