Recent Events Reported by Observers
Previous Next
Detected by gchintzo, Submitted at 2018-08-21T23:14:16
2018-08-18T16:30:09 --> 2018-08-19T04:10:09
A filament seen along its axis surrounded by a cavity. This eruption was captured by LASCO and produced a CME of 480 km/s (see http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20180819.074807.w010.v0489.p217&frame=3&r)
Detected by gchintzo, Submitted at 2018-08-21T23:08:54
2018-08-18T20:50:09 --> 2018-08-19T19:10:09
A long north-south oriented filament on the north hemisphere of the sun. The filament forms along the neutral line (between positive (green) and negative (red) polarities)
Detected by gchintzo, Submitted at 2018-08-21T23:04:22
2018-08-18T20:50:09 --> 2018-08-19T19:10:09
Four consecutive eruptions seen at the east limb. These eruptions showed no imprints in the LASCO coronagraphic data, thus they were failed eruptions.
Detected by jinmeng, Submitted at 2018-08-21T01:45:10
2018-06-24T06:30:09 --> 2018-06-24T15:42:09
An eruption observed at the limb.
Detected by jinmeng, Submitted at 2018-08-21T01:07:07
2018-08-16T08:10:09 --> 2018-08-16T16:30:09
An eruption from AR 12718.
Detected by jinmeng, Submitted at 2018-08-21T00:41:03
2018-07-31T01:20:09 --> 2018-07-31T12:10:09
A filament eruption was observed near the equator. It seems that majority of the filament material falls back to the Sun showing multiple brightenings.
Detected by jinmeng, Submitted at 2018-08-21T00:25:14
2018-06-09T00:00:09 --> 2018-06-09T05:30:09
A large quiet-Sun filament eruption was observed in the northern hemisphere.
Detected by jinmeng, Submitted at 2018-08-20T23:16:13
2018-06-07T05:30:09 --> 2018-06-07T10:40:09
Small eruption from a bipolar region. The eruption influenced a larger area around the source region (showing temporary dimming).
Detected by Patricia Jibben, Submitted at 2018-08-20T14:25:23
2018-05-19T08:01:35 --> 2018-05-19T08:37:49
This movie does not show the feature. It exists in the wings of Mg II and can be observed by clicking on the MgII_raster on the IRIS observation page. Counter streaming is easily observed almost perpendicular to the IRIS slit.
Detected by Patricia Jibben, Submitted at 2018-08-20T14:15:38
2018-05-17T13:53:16 --> 2018-05-17T14:42:04
This Flare does not have a corresponding GOES event. The IRIS slit crosses the event near the beginning and end.
Detected by Lijia Guo, Submitted at 2018-08-14T21:51:07
2018-08-07T05:57:55 --> 2018-08-07T06:01:10
The IRIS slit raster across a bright point in the middle of AR 12717 around 05:58:00, at the same time enhancement of continuum are observed in Si IV, C II and Mg II h&k.
Detected by Lijia Guo, Submitted at 2018-08-14T21:37:48
2018-08-07T05:07:09 --> 2018-08-07T05:10:23
The IRIS slit raster across a bright arc at the north end of AR 12717 around 05:08:00 and extensively widened wings are observed in Si IV, C II and Mg II h&k.
Detected by gchintzo, Submitted at 2018-08-10T18:19:38
2018-08-06T20:40:09 --> 2018-08-07T19:20:09
Cool material (yellow: 304A channel; 50,000 K) is seen to move along the north south direction filling magnetic field structures above the west solar limb.
Detected by Milan Gosic, Submitted at 2018-08-07T23:20:42
2018-05-03T19:18:51 --> 2018-05-03T20:32:00
Spray surges on the east limb, covered by the slit.
Detected by Milan Gosic, Submitted at 2018-08-07T22:59:10
2018-05-06T14:01:58 --> 2018-05-06T20:35:04
On 6-May-2018 IRIS captured a prominence at the E solar limb. This observational run gives a quite rare opportunity to see how prominences are formed. Around the prominence there are also some loop-like structures, partially located under the slit.
Detected by gchintzo, Submitted at 2018-08-07T22:43:26
2018-08-03T04:20:09 --> 2018-08-05T00:00:09
A coronal cavity becoming more prominent when solar rotation brings a filament channel in a view along its axis.
Detected by gchintzo, Submitted at 2018-08-07T22:33:12
2018-08-02T00:00:09 --> 2018-08-05T00:00:09
A prominence north of a large loop system rotating into view. Note the continuous swaying motions of the cool prominence material.
Detected by gchintzo, Submitted at 2018-08-07T22:27:12
2018-08-02T00:00:09 --> 2018-08-05T00:00:09
NOAA AR12717 transiting the solar disk. No sunspots are visible in this Active Region due to the incoherence of its magnetic flux concentrations (green positive, red negative)
Detected by gchintzo, Submitted at 2018-08-07T21:46:58
2018-08-02T00:00:09 --> 2018-08-02T18:50:09
An eruption exhibiting the characteristic CME bubble structure. Associated CME speed is unkown; SEEDS is currently offline.
Detected by Paul Bryans, Submitted at 2018-08-03T21:19:23
2018-07-10T02:33:03 --> 2018-07-10T03:43:57
Interesting brightening events that appear as several small bright points clustered close together. Seen in 1330, 1400 and 2796 SJIs. 2832 also shows some activity that resembles flux emergence.
