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 2016-01-20T19:52:49
2016-01-19T17:00:06 --> 2016-01-20T00:00:06
An active region surge through nearby filament channel.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2016-01-20T19:19:48
2016-01-19T00:00:06 --> 2016-01-19T09:20:06
Quiet sun filament eruption. The eruption also causes synchronous activity of another filament to the north.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by jinmeng, Submitted at 2016-01-20T19:19:48
2016-01-19T00:00:06 --> 2016-01-19T09:20:06
Quiet sun filament eruption. The eruption also causes synchronous activity of another filament to the north.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-19T23:21:18
2016-01-18T21:10:10 --> 2016-01-18T22:30:10
Cldearly there was an eruption on the back side, but it did not make it to coronagraph heights.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-19T23:02:24
2016-01-16T17:00:06 --> 2016-01-17T06:00:06
Downflow of cool matrial (as seen in 304 A images) was seen for long time. It traces the lower (closed) part of the coronal structure as seen in 171 A images.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-19T17:08:52
2016-01-15T21:40:10 --> 2016-01-15T23:00:10
This is associated with a C1.1 flare in AR 12480. Most of the ejected material seems to come back. The overlying corona is hardly impacted.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-19T16:46:06
2016-01-15T18:50:22 --> 2016-01-15T19:40:22
This jet-like eruption is most clearly seen in 304 A images. It appears that a straight, horizontal trajectory exists in addition to the one that falls down.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-19T16:38:45
2016-01-15T18:40:10 --> 2016-01-15T21:00:10
Without signs of footpoint brightening, the source region of this eruption should be occulted. The eruption seems to consist of a flux rope, which is consistent with the appearnace of the associated narrow but bright CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-19T16:29:10
2016-01-15T02:20:22 --> 2016-01-15T03:30:22
Minor eruption from AR 12480, triggering loops outside the AR to oscillate. A C2.8 flare was associated.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-19T16:29:09
2016-01-15T02:20:22 --> 2016-01-15T03:30:22
Minor eruption from AR 12480, triggering loops outside the AR to oscillate. A C2.8 flare was associated.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-19T05:43:27
2016-01-17T20:40:10 --> 2016-01-18T00:00:10
This is a subtle eruption that can be easily overlooked.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-19T05:37:45
2016-01-18T14:10:10 --> 2016-01-18T14:40:10
The footpoint seems to be slightly occulted. The jet-like eruption in the polar coronal hole (on the visible side) looks like an independent phenomenon.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-19T02:16:42
2016-01-13T00:00:06 --> 2016-01-13T13:52:06
The northeastern part of the small low-latitude coronal hole became less dark. Is this just projection effect from adjacent close loops?
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by schryver, Submitted at 2016-01-11T19:00:17
2016-01-10T01:58:18 --> 2016-01-10T02:46:18
QS filament activation, with apparent ribbons, but no signs of eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by weiliu, Submitted at 2016-01-09T01:12:50
2015-12-25T17:00:06 --> 2015-12-25T18:30:06
An active region filament kinked and disrupted (but material falls back), causing flaring brightening.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-07T05:48:23
2016-01-06T10:00:06 --> 2016-01-06T13:00:06
A small filament erupted from a quiescent region, showing coronal dimming at high altitudes and formation of two-ribbon flare emission. It resulted in a slow CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-07T05:48:22
2016-01-06T10:00:06 --> 2016-01-06T13:00:06
A small filament erupted from a quiescent region, showing coronal dimming at high altitudes and formation of two-ribbon flare emission. It resulted in a slow CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-07T05:42:31
2016-01-05T02:30:34 --> 2016-01-05T05:30:34
This was likely to be associated with AR 12473, which was already 25-30 degrees behind the limb. The eruption shows helical motions and the overlying corona is seen to dim. It resulted in a narrow CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-07T05:42:30
2016-01-05T02:30:34 --> 2016-01-05T05:30:34
This was likely to be associated with AR 12473, which was already 25-30 degrees behind the limb. The eruption shows helical motions and the overlying corona is seen to dim. It resulted in a narrow CME.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2016-01-07T05:36:27
2016-01-04T10:40:10 --> 2016-01-04T16:00:10
This was a diffuse eruption, but two-ribbon-like emission was clearly seen northwest of the filament.
