Recent Events Reported by Observers

Detected by Jakub Prchlik, Submitted at 2016-08-01T20:17:11

2014-06-19T18:52:21 --> 2014-06-19T19:26:19

1330, 1400, and 2796 A all show a two ribboned flare. The shorter of the two ribbons appears to connect two filament holes, while the longer ribbon starts at the edge of one filament and continues off the image.

Detected by Milan Gosic, Submitted at 2016-08-01T20:06:56

2016-07-22T07:31:30 --> 2016-07-22T12:39:55

The movie shows two long duration peacock tails above light bridges in AR12567 and AR12565. The peacock tails are visible during the entire duration of the movie, while the left one (in AR12567) is also partially covered by the slit.

Detected by Jakub Prchlik, Submitted at 2016-08-01T19:57:05

2014-06-18T21:46:49 --> 2014-06-18T22:20:17

Oscillations observed in a C shaped sunspot. The oscillations are also clearly visible in the NUV continuum.

Detected by Jakub Prchlik, Submitted at 2016-08-01T19:42:56

2014-06-18T15:41:18 --> 2014-06-18T15:56:54

1330, 1400, and 2796 A all show a GOES C 1.1 flare. The flare's intensity localizes in two separate ribbon structures near two sunspots. The ribbon structures do not cross the slit, however, lower intensity flares concurrent with the flare do cross the slit. A low intensity flare precedes the main flare (by 45 minutes) between the same two sunspots. Similar to the main flare, the main ribbons of the preceding (weaker) flair do not cross the slit, but weaker parts of the flare do.

Detected by Jakub Prchlik, Submitted at 2016-08-01T18:47:22

2014-06-17T13:13:57 --> 2014-06-17T13:27:17

All observed wavelengths (1330, 1400, and 2796 A) show a C1.0 GOES flare event, however, the only a portion of the flare emerges at the top of the observation. The emerging flare briefly crosses the top of the slit, but useful spectroscopic information seems unlikely. Three smaller flares follow the GOES identified flare and cross the slit.

Detected by Nicole Schanche, Submitted at 2016-08-01T17:44:23

2015-01-05T17:39:21 --> 2015-01-05T18:06:26

The observation begins with the C7.4 flare already in progress. A large C-shaped flare ribbon can be seen, with a second ribbon stretching from the center of the C to the far right of the frame.

Detected by Nicole Schanche, Submitted at 2016-08-01T17:37:31

2015-01-03T21:54:06 --> 2015-01-03T22:27:45

A C1.3 flare peaking at 22:23 was reported in the NOAA/GOES flare archive. This observations shows what looks like a curving, elongated C-dahape flare ribbon brightening around the time of the flare.

Detected by Nicole Schanche, Submitted at 2016-08-01T17:32:11

2015-01-03T13:48:00 --> 2015-01-03T14:23:39

The NOAA/GOES flare database detected a C1.8 flare beginning at 13:37 and peaking at 14:13. The flare site appears to be bright for the duration of this IRIS observation, although a brightening flare event concurrent with the GOES flare is observed. This is the same flare site as the long duration C1.7 flare earlier in the same day.

Detected by Jakub Prchlik, Submitted at 2016-08-01T17:28:04

2014-06-17T04:51:52 --> 2014-06-17T05:17:24

A GOES C4.7 flare is visible in 1330, 1400, and 2796 A. After staring, the flare does not significantly expand along the ribbon, however, the flare increases the ribbon width. During the flare, the ribbon does not cross any sunspots. Instead, the flare weaves between three to four sunspots.

Detected by Nicole Schanche, Submitted at 2016-08-01T17:26:46

2015-01-03T10:19:39 --> 2015-01-03T11:10:49

The flare shows twisting of the magnetic field lines and two thin ribbons during the eruption. Material can be seen leaving the main flare site to the left. This region of this flare remains bright for the duration of this observation (>1hr).

Detected by Nicole Schanche, Submitted at 2016-08-01T16:54:04

2016-01-03T10:53:19 --> 2016-01-03T11:48:34

This observation catches part of the filament associated with AR12473. The prominence material can be seen moving both directions. A small ejection into the filament occurs around 11:30.

Detected by Jakub Prchlik, Submitted at 2016-08-01T16:11:50

2015-05-22T16:30:04 --> 2015-05-22T17:04:06

IRIS captures a B5.4 flare. The flare is visible in 1330 A and 2796 A, but shows a higher intensity contrast in 1330 A. During the flare's peak, Mg II h/k, Si IV, and C II displays blue shifted emission.

Detected by Nicole Schanche, Submitted at 2016-08-01T15:58:30

2016-01-02T11:00:55 --> 2016-01-02T11:20:41

Two small explosive events occur simultaneously in AR12473. The event on the left appears to be a small, failed eruption, while the one on the right appears to be a typical jet, although the observation ends early one in the jet development. Neither brightenings were recorded as flares in the NOAA/GOES flare catalog.

Detected by Jakub Prchlik, Submitted at 2016-08-01T15:50:47

2015-05-21T18:07:13 --> 2015-05-21T18:21:28

Eruption is visible in 1330 A and 2796 A. Following the eruption, 2796 A displays waves of absorption. Since the event crosses the slit, the spectrum shows the post eruption absorption is in the wings of Mg II h and k.

Detected by Nicole Schanche, Submitted at 2016-08-01T15:48:39

2016-01-01T23:08:15 --> 2016-01-01T23:56:58

This observation shows what looks like downward flowing material in two flare ribbons. The ribbons slowly move farther apart as the observation progresses. While a large flare is not seen, it would appear that this ribbon spreading is associated with an M2.3 flare that occurred at this time in the same active region.

Detected by Nicole Schanche, Submitted at 2016-08-01T15:34:39

2015-12-31T11:22:10 --> 2015-12-31T12:06:46

This small ribbon brightening was not associated with a flare in the NOAA/GOES flare database. However, after the ribbon brightening, the overlying material also brightens along arching magnetic field lines.

Detected by Nicole Schanche, Submitted at 2016-08-01T15:26:35

2015-12-30T10:59:59 --> 2015-12-30T11:16:28

The beginning of this movie shows the peak and decline of a small flare, not identified in the NOAA/GOES flare archive. I therefore label it an explosive event.

Detected by Jakub Prchlik, Submitted at 2016-08-01T15:09:45

2015-05-20T15:30:59 --> 2015-05-20T16:27:14

Both 1330 A and 2796 A show emission from a surge event, but the 1330 A intensity shows a higher emission contrast than 2796 A. However, 2796 A displays a ribbon of faint absorption preceding the surge, which the surge follows.

Detected by Jakub Prchlik, Submitted at 2016-08-01T13:11:21

2015-05-19T11:19:23 --> 2015-05-19T11:43:33

IRIS captures multiple brightening events in 1400 A and 2796 A. Starting at 11:23:47.930 the brightening area shows an outward material flow in 1400 A, which ends at 11:43:01.050. However, 2796 A does not observe the material flow. After the material flow ends, the brightening events are lower in intensity than the preceding brightening events in both 1400 A and 2796 A.

Detected by Milan Gosic, Submitted at 2016-08-01T04:40:09

2016-07-23T13:01:57 --> 2016-07-23T13:31:16

Eruption with a jet-like ejection between AR12567 and AR12565. The event is covered by the slit.