Recent Events Reported by Observers

Detected by Patricia Jibben, Submitted at 2017-01-26T21:40:28

2017-01-24T19:11:28 --> 2017-01-24T19:26:27

This event is bright in 1400 but is not in 2796.

Detected by Patricia Jibben, Submitted at 2017-01-26T21:28:12

2017-01-24T19:27:53 --> 2017-01-24T19:29:40

The jet happens along the northern plage boundary.

Detected by Donald Schmit, Submitted at 2017-01-25T13:25:24

2017-01-23T20:00:43 --> 2017-01-23T20:28:55

Interesting and odd shape dark loop in Mg II SJI. This is emerging AR 12627

Detected by Donald Schmit, Submitted at 2017-01-25T13:20:53

2017-01-21T20:59:52 --> 2017-01-21T21:15:13

Another small flare that doesn't show up in goes in decaying AR 12626

Detected by Donald Schmit, Submitted at 2017-01-25T13:15:38

2017-01-21T14:24:52 --> 2017-01-21T14:40:34

This flare in AR 12626 did not show up in GOES. The AR is in the decaying phase.

Detected by Donald Schmit, Submitted at 2017-01-24T20:37:00

2017-01-19T08:36:13 --> 2017-01-19T09:32:55

This filament is unusually shaped. It basically a pillar and off the top is a flow of coronal rain that is downward and divergent

Detected by Donald Schmit, Submitted at 2017-01-24T20:29:13

2017-01-18T19:51:18 --> 2017-01-18T20:04:52

There are two parts to this jet. A bright loop and a collimated ejecta that appears to be moving fast.

Detected by halocme, Submitted at 2017-01-21T02:41:21

2017-01-19T09:00:09 --> 2017-01-19T13:00:09

An example of a prominence that undergoes unwinding motions and takes off gradually without explosive motions. This was probably related to a slow CME that appeared around 12:30 UT (https://sohowww.nascom.nasa.gov/data/REPROCESSING/Completed/2017/c2/20170119/20170119_1512_c2_512.jpg shows it at a later time).

Detected by halocme, Submitted at 2017-01-21T01:40:36

2017-01-19T09:45:01 --> 2017-01-19T10:30:37

This may be the first coronal wave we have observed since late October 2016. It is minor, but still disturbs a large area to southwest. No active region or flare is associated. No CME either.

Detected by Jakub Prchlik, Submitted at 2017-01-19T21:33:48

2017-01-15T23:12:54 --> 2017-01-15T23:59:07

IRIS observes a prominence on the NW limb, which is primarily visible in 2796 ?? (Mg II). However, the prominence is also visible in 1400 ??. The prominence's arch shape remains stable throughout the observation.

Detected by Jakub Prchlik, Submitted at 2017-01-19T21:30:20

2017-01-15T22:03:56 --> 2017-01-15T22:36:29

IRIS observes a prominence on the NW limb, which is primarily visible in 2796 ?? (Mg II). However, the prominence is also visible in 1400 ??. As the movie progress the prominence progress from a pointed to a more semicircular arch.

Detected by Jakub Prchlik, Submitted at 2017-01-19T21:25:09

2017-01-14T21:24:55 --> 2017-01-14T22:14:14

IRIS observes a prominence on the NW limb, which is primarily visible in 2796 ?? (Mg II).

Detected by Jakub Prchlik, Submitted at 2017-01-19T21:21:44

2017-01-14T22:51:03 --> 2017-01-14T23:48:46

IRIS observes a prominence on the NW limb, which is primarily visible in 2796 ?? (Mg II).

Detected by Jakub Prchlik, Submitted at 2017-01-19T21:06:00

2017-01-12T06:33:08 --> 2017-01-12T06:59:41

Although no obvious filament appears in the SJI, Mg II h and k shows absorption in the line core that is spatially coincident with a filament. The absorption is visible throughout the observation near slit's southern most extent.

Detected by Jakub Prchlik, Submitted at 2017-01-19T21:00:35

2017-01-11T19:05:16 --> 2017-01-11T19:37:27

Although no obvious filament appears in the SJI, Mg II h and k shows absorption in the line core that is spatially coincident with a bright network element. The absorption becomes visible at 19:05:29 near the center of the Mg II spectrum. The absorption then dynamically proceeds to the spectrum's most northern extent.

Detected by Jakub Prchlik, Submitted at 2017-01-19T20:52:59

2017-01-10T22:18:39 --> 2017-01-10T22:30:43

Although no obvious filament appears in the SJI, Mg II h and k shows absorption in the line core that is spatially coincident with a faint network element. The absorption becomes visible at 22:17:27 near the top of the Mg II spectrum.

Detected by Jakub Prchlik, Submitted at 2017-01-19T18:24:59

2017-01-16T17:39:55 --> 2017-01-16T17:54:33

IRIS observes a GOES B1.3 flare in AR 12626. The left flare ribbon forms between two sunspots and expands into both sunspots. However, expansion into the southern sunspot slows, while expansion into the northern sunspot remains constant. Once the northern expansion stops, the flare brightens to maximum intensity.

Detected by Jakub Prchlik, Submitted at 2017-01-19T18:05:56

2017-01-14T10:17:10 --> 2017-01-14T10:26:05

IRIS observes a microflare in AR 12626. The microflare stems from two footpoints on opposite sides of a circular bright region. After peak flux, we see heated material suspended above the flare. Although the slit crosses the event, the slit does not obtain a spectrum near peak intensity.

Detected by Jakub Prchlik, Submitted at 2017-01-19T17:30:11

2017-01-15T17:15:55 --> 2017-01-15T17:26:59

IRIS observes a microflare in AR 12626. The microflare produces a visible flare loop; however, only one flare footpoint is visible.

Detected by Jakub Prchlik, Submitted at 2017-01-19T17:18:12

2017-01-13T09:38:32 --> 2017-01-13T10:01:01

IRIS observes a UV burst in AR 12626 near the east limb.