Recent Events Reported by Observers
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Detected by Charles Kankelborg, Submitted at 2017-05-16T06:41:32
2017-05-15T08:50:10 --> 2017-05-15T09:16:59
Small failed eruption in new region AR 12656. After the event there is also some nearby microflaring.
Detected by Charles Kankelborg, Submitted at 2017-05-16T06:09:23
2017-05-13T19:50:44 --> 2017-05-13T20:03:33
A cute little macrospicule that missed the slit.
Detected by Charles Kankelborg, Submitted at 2017-05-16T05:28:47
2017-05-12T07:59:48 --> 2017-05-12T13:53:21
SST was looking for solar tornadoes, but targeting a day ahead was difficult. The IRIS slit missed this one.
Detected by Charles Kankelborg, Submitted at 2017-05-16T05:22:17
2017-05-12T12:45:04 --> 2017-05-12T13:06:16
Transition region jet near the limb during SST coordination.
Detected by Charles Kankelborg, Submitted at 2017-05-16T04:34:09
2017-05-10T08:07:51 --> 2017-05-10T12:05:36
Series of homologous microflares in AR 12655
Detected by Charles Kankelborg, Submitted at 2017-05-16T04:13:58
2017-05-10T03:30:20 --> 2017-05-10T03:42:46
Small, rapid eruptive event
Detected by Charles Kankelborg, Submitted at 2017-05-16T03:15:40
2017-05-09T04:25:45 --> 2017-05-09T04:25:45
During routine A1 synoptic, IRIS rastered over an explosive event in a very bright network element.
Detected by Paul Bryans, Submitted at 2017-05-10T14:46:25
2017-05-05T10:23:04 --> 2017-05-05T10:54:15
Microflare (no GOES counterpart) in emerging flux region
Detected by Paul Bryans, Submitted at 2017-05-10T14:43:24
2017-05-02T09:57:41 --> 2017-05-02T11:08:03
Bright point in AR with strong Doppler shifts
Detected by Paul Bryans, Submitted at 2017-05-09T22:58:43
2017-05-04T19:49:39 --> 2017-05-04T20:51:02
Persistent jet in AR
Detected by Paul Bryans, Submitted at 2017-05-09T22:56:55
2017-05-04T18:11:39 --> 2017-05-04T19:13:02
Small jet near penumbra of trailing sunspot of AR
Detected by Paul Bryans, Submitted at 2017-05-09T22:53:42
2017-05-04T00:59:28 --> 2017-05-04T03:00:46
Loops on west limb and coronal rain
Detected by halocme, Submitted at 2017-05-07T07:40:49
2017-05-04T00:00:09 --> 2017-05-05T13:00:09
Although there were magnetic field concentrations, the sunspot was recognized only on 5 May 2017. Since then several B-class flares were produced. It appears that there was an eruption on 5 May 2017, between 08:30 and 10:30, woth notable dimming in 171 A, but no CME was associated.
Detected by halocme, Submitted at 2017-05-07T06:40:55
2017-05-01T15:00:09 --> 2017-05-03T04:00:09
A rapid growth started early on 2 May 2017 due to the new flux to the south of the original bipole. This region did not produce major (e.g. >C1) flares or CMEs.
Detected by halocme, Submitted at 2017-05-07T06:01:59
2017-05-05T22:30:01 --> 2017-05-05T23:30:01
This flare may be called eruptive by some, because a large area to the north seems to have been impacted. But there is no way it was associated with a CME even in the limb view. There may have been disturbances due to MHD waves but it seems that no flux rope was involved, hence no CME.
Detected by halocme, Submitted at 2017-05-07T05:38:19
2017-05-05T03:50:25 --> 2017-05-05T05:30:25
The pre-eruption filament is not clear, but the formation of flare ribbons and loops between them suggests an eruption. An area larger to the south more extended than the ribbons is seen to dim, especially in 171 A.
Detected by halocme, Submitted at 2017-05-07T05:38:18
2017-05-05T03:50:25 --> 2017-05-05T05:30:25
The pre-eruption filament is not clear, but the formation of flare ribbons and loops between them suggests an eruption. An area larger to the south more extended than the ribbons is seen to dim, especially in 171 A.
Detected by halocme, Submitted at 2017-05-07T05:13:34
2017-05-03T19:55:13 --> 2017-05-03T21:31:13
Continued surge-like activities came from two regions near the limb. It is not clear whether the eruptions only delineated closed structures, or how the two regions were linked.
Detected by halocme, Submitted at 2017-05-07T05:03:39
2017-05-02T11:50:25 --> 2017-05-02T15:50:25
The pre-eruption filament was not clearly seen, but a moving dark feature may have been a filament eruption. The event was captured only in 304 A channel, without showing clear flare ribbons or post eruption arcades
Detected by halocme, Submitted at 2017-05-07T05:40:50
2017-05-01T12:55:13 --> 2017-05-01T13:50:25
This eruption was associated with a B3.0 flare from the same region (without NOAA AR number) as the earlier B9.9 flare. The eruption itself was weaker, but the coronal wave is clearly seen to propagate counterclockwise along the limb in difference images especially in 193 A channel.
