Highest Rated Events (only 193 and 304 shown) All AR FE FL

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-07-18T18:49:45

2017-07-15T18:56:09 --> 2017-07-15T21:02:09

A confined eruption was observed near the west limb. The coronal loops are pushed to a higher altitude but not opened up.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-07-13T23:31:15

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).

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-07-13T23:31:15

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).

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-07-13T22:43:38

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.

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Detected by jinmeng, Submitted at 2017-07-13T22:32:38

2017-06-28T13:56:09 --> 2017-06-28T16:38:09

A small eruption was observed at the east limb.

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Detected by jinmeng, Submitted at 2017-07-13T22:25:33

2017-06-27T15:40:09 --> 2017-06-27T23:50:09

Two distant filaments at the east limb were observed exchanging material.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-07-13T22:11:22

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.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-07-13T22:00:14

2017-06-25T11:57:09 --> 2017-06-25T12:40:09

A very small-scale (minifilament?) eruption was observed in the south polar region.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-07-13T21:51:53

2017-06-25T08:46:09 --> 2017-06-25T09:59:09

Two minifilaments were observed erupting around the same time.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-07-13T21:39:55

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.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-07-13T21:39:55

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.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by jinmeng, Submitted at 2017-07-13T21:28:57

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.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-07-06T06:41:38

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.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-07-06T06:16:12

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.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-07-06T02:06:25

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.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-07-06T01:36:47

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.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-07-06T01:36:46

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.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-07-06T01:36:46

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.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-07-06T01:11:28

2017-07-03T01:30:01 --> 2017-07-03T08:00:01

This slow eruption or disappearance of a large-scale structure is seen preferentially in 171 A images. It may be responsible for an outflow in LASCO images, which may not be classified as a CME.

Rating: 3.0 (0=lowest, 5=highest)         Num Ratings:1

Detected by halocme, Submitted at 2017-07-06T00:58:31

2017-07-02T11:50:25 --> 2017-07-02T14:20:25

These running difference images reveal the coronal wave more clearly. It is also easier to find the erupting filament. The wave is more pronounced in the counterclockwise direction. It seems to produce a secondary wave as it propagates into large-scale structures.