Recent Events Reported by Observers
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Detected by Tiago Pereira, Submitted at 2017-07-18T15:52:19
2017-06-22T05:10:59 --> 2017-06-22T05:47:35
Dark absorption fibrils appear, perhaps a small filament, appear in the 2796 SJI.
Detected by Tiago Pereira, Submitted at 2017-07-18T15:44:57
2017-06-21T09:44:02 --> 2017-06-21T09:57:40
Eruption in AR plage, probably a small flare. Slit partially covers the event (late stages, one footpoint).
Detected by Tiago Pereira, Submitted at 2017-07-18T15:40:59
2017-06-20T22:26:04 --> 2017-06-20T22:40:44
A reverse-Y (anemone type) jet associated with magnetic reconnection erupts violently.
Detected by jinmeng, Submitted at 2017-07-13T23:40:54
2017-06-28T09:10:09 --> 2017-06-29T00:00:09
The eruption on Jun 28 toward the Earth. It seems the filament is located to the north of the active region. This CME event looks big in the white light observation (https://twitter.com/halocme/status/880334481479139329). The CME-driven shock was arrived Earth around 16:00 UT July 1 (https://twitter.com/halocme/status/881233848255864833).
Detected by jinmeng, Submitted at 2017-07-13T23:40:53
2017-06-28T09:10:09 --> 2017-06-29T00:00:09
The eruption on Jun 28 toward the Earth. It seems the filament is located to the north of the active region. This CME event looks big in the white light observation (https://twitter.com/halocme/status/880334481479139329). The CME-driven shock was arrived Earth around 16:00 UT July 1 (https://twitter.com/halocme/status/881233848255864833).
Detected by jinmeng, Submitted at 2017-07-13T23:40:48
2017-06-28T09:50:09 --> 2017-06-29T00:00:09
Transiant coronal dimming was observed near an active region. Might be related to a QR filament eruption.
Detected by jinmeng, Submitted at 2017-07-13T22:32:42
2017-06-28T13:56:09 --> 2017-06-28T16:38:09
A small eruption was observed at the east limb.
Detected by jinmeng, Submitted at 2017-07-13T22:41:38
2017-06-27T15:40:09 --> 2017-06-27T23:50:09
Two distant filaments at the east limb were observed exchanging material.
Detected by jinmeng, Submitted at 2017-07-13T22:11:25
2017-06-26T06:10:09 --> 2017-06-26T14:30:09
Filament material was observed draining back to the Sun to both north and south directions.
Detected by jinmeng, Submitted at 2017-07-13T22:00:18
2017-06-25T11:57:09 --> 2017-06-25T12:40:09
A very small-scale (minifilament?) eruption was observed in the south polar region.
Detected by jinmeng, Submitted at 2017-07-13T22:41:39
2017-06-25T08:46:09 --> 2017-06-25T09:59:09
Two minifilaments were observed erupting around the same time.
Detected by jinmeng, Submitted at 2017-07-13T21:40:01
2017-06-24T11:40:09 --> 2017-06-24T13:43:21
A coronal jet/surge was observed from AR 12664. The surge seems to be associated with multiple activities around the active region indicating the magnetic connectivities among them.
Detected by jinmeng, Submitted at 2017-07-13T21:40:01
2017-06-24T11:40:09 --> 2017-06-24T13:43:21
A coronal jet/surge was observed from AR 12664. The surge seems to be associated with multiple activities around the active region indicating the magnetic connectivities among them.
Detected by jinmeng, Submitted at 2017-07-13T21:29:02
2017-06-23T13:50:09 --> 2017-06-23T21:50:09
A failed filament eruption was observed near the west limb. At certain time, large-scale overlaying coronal loop can be seen above the filament channel.
Detected by halocme, Submitted at 2017-07-06T06:41:42
2017-07-04T08:15:01 --> 2017-07-04T09:51:01
It appeared to come from slightly behind the limb. Some dimming was seen. As expected, there was a CME.
Detected by halocme, Submitted at 2017-07-06T06:16:16
2017-07-04T03:00:09 --> 2017-07-04T11:00:09
Repeated small-scale activities seen in 304 A images appear to lead to ouflows on larger scales. They may contribute to long-lasting outflows in LASCO data. They were from the new region without NOAA number that produced the M1.3 flare on 3 July.
Detected by halocme, Submitted at 2017-07-06T02:06:53
2017-07-03T15:30:01 --> 2017-07-03T18:00:01
I forgot to mention in the last annotation that the M1.3 flare (newly emerged non-numbered region) was not homologous to the B1.3 flare (AR 12644). This wave is slightly more pronounced in the clockwise direction.
Detected by halocme, Submitted at 2017-07-06T02:06:52
2017-07-03T15:30:01 --> 2017-07-03T18:00:01
I forgot to mention in the last annotation that the M1.3 flare (newly emerged non-numbered region) was not homologous to the B1.3 flare (AR 12644). This wave is slightly more pronounced in the clockwise direction.
Detected by halocme, Submitted at 2017-07-06T01:36:54
2017-07-03T15:30:01 --> 2017-07-03T18:00:01
More energetic version of the B1.3 flare on 2 July 2017. Cool prominence matrial is more clearly seen. However, supra-arcade downflows, often seen in eruptive flares, seem to be missing.
Detected by halocme, Submitted at 2017-07-06T01:36:54
2017-07-03T15:30:01 --> 2017-07-03T18:00:01
More energetic version of the B1.3 flare on 2 July 2017. Cool prominence matrial is more clearly seen. However, supra-arcade downflows, often seen in eruptive flares, seem to be missing.