Highest Rated Events (only 193 and 304 shown) All AR FE FL
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-05T20:17:56
2014-07-01T12:50:23 --> 2014-07-01T14:00:23
Another example.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-05T20:14:39
2014-07-01T07:25:11 --> 2014-07-01T08:25:11
Something like this was seen many times during 1-2 July. The origin was probably on the far side. Only big ones will be reported.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-05T20:14:38
2014-07-01T07:25:11 --> 2014-07-01T08:25:11
Something like this was seen many times during 1-2 July. The origin was probably on the far side. Only big ones will be reported.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-05T19:42:05
2014-07-01T23:00:03 --> 2014-07-01T23:58:03
The source region seems to be less than 20 degrees behind the limb. The prominence appears in emission in all of the 304, 211 and 171 channels.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-05T19:35:32
2014-07-01T09:50:23 --> 2014-07-01T12:20:23
This movie contains two flares in AR 12106. The first one is C6.0 and it is characterized by a large-scale coronal propagating front (LCPF) and the second one, M1.4, by an eruption in the radial direction. The first flare may be considered to have set the stage for the main eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-05T19:35:31
2014-07-01T09:50:23 --> 2014-07-01T12:20:23
This movie contains two flares in AR 12106. The first one is C6.0 and it is characterized by a large-scale coronal propagating front (LCPF) and the second one, M1.4, by an eruption in the radial direction. The first flare may be considered to have set the stage for the main eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-05T19:35:29
2014-07-01T09:50:23 --> 2014-07-01T12:20:23
This movie contains two flares in AR 12106. The first one is C6.0 and it is characterized by a large-scale coronal propagating front (LCPF) and the second one, M1.4, by an eruption in the radial direction. The first flare may be considered to have set the stage for the main eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-03T23:53:13
2014-06-30T17:00:03 --> 2014-06-30T19:00:03
This eruption occurred in what used to be AR 12093. It started as the northern part opened up.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-03T23:53:12
2014-06-30T17:00:03 --> 2014-06-30T19:00:03
This eruption occurred in what used to be AR 12093. It started as the northern part opened up.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-03T23:01:54
2014-06-30T16:40:11 --> 2014-06-30T17:56:11
This is from a sizable eruption from the backside. The source region may be ~30 degrees behind the limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-03T22:38:08
2014-06-30T06:00:03 --> 2014-06-30T07:20:03
This eruption was responsible for a diffuse but fast CME observed by LASCO. No clear systematic pre-eruption activity is found, but based on the complex foot-point structure multiple small bipoles may have been involved.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-03T22:03:04
2014-06-30T02:40:11 --> 2014-06-30T03:30:11
The eruption assumes a kink-like appearance as is often the case with failed eruptions. As expected, no CME is associated with this solar event.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-07-03T21:34:39
2014-06-30T01:55:11 --> 2014-06-30T02:31:11
The jet itself is so diffuse that it can escape detection, but reconnection at the footpoints may be consistent with a jet model.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-07-03T21:05:34
2014-06-22T19:20:03 --> 2014-06-22T21:00:03
Most of the chromospheric (304) material seems to drain back down following the surge.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-07-03T21:01:13
2014-06-21T18:10:03 --> 2014-06-21T22:20:03
Simultaneous events: 1. Filament activation in northwest limb 2. Puffing loops (eruption?) in northeast limb 3. Eruption in AR 12093
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-07-03T21:00:32
2014-06-21T18:10:03 --> 2014-06-21T22:20:03
Simultaneous events: 1. Filament activation in northwest limb 2. Puffing loops (eruption?) in northeast limb 3. Eruption in AR 12093
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by cheung, Submitted at 2014-07-03T20:59:44
2014-06-21T18:10:03 --> 2014-06-21T22:20:03
Simultaneous events: 1. Filament activation in northwest limb 2. Puffing loops (eruption?) in northeast limb 3. Eruption in AR 12093
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2014-06-17T01:07:22
2014-06-14T00:00:03 --> 2014-06-15T00:00:03
A remarkably unremarkable existence of a prominence as large as this one.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2014-06-16T23:18:44
2014-06-13T00:00:03 --> 2014-06-13T02:36:03
Two nearby regions brighten up at the same time; one produces a large spray surge and the other one appears to produce an incomplete eruption. The 211A images show some connectivity between the two regions and so these two eruptions coule, in fact, be two footpoints of the same larger-scale eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-06-16T07:46:01
2014-06-11T20:30:35 --> 2014-06-11T21:40:11
Like the previous X2.2, M3.1 and X1.0 flares (not the X1.5, which was special in terms of a powerful eruption), this flare was associated with a minor eruption and loop oscillations at higher altitudes. The eruption looks falling back, but at least an unimpressive CME has resulted from it.
