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 2013-01-15T23:43:54
2013-01-13T08:10:11 --> 2013-01-13T09:30:35
This may look different from what we normally talk about as EUV waves because no smooth front is seen. However, the movie clearly show outward propagating disturbances from the flare site.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-12T18:44:11
2013-01-12T06:00:03 --> 2013-01-12T06:50:03
Although we do not know at this moment (before STEREO-A images arrive) where this eruption comes from (no reported flare), it clearly produces a large-scale propagation of disturbances. The southward branch is especially noticeable.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-12T18:18:12
2013-01-09T14:20:23 --> 2013-01-09T15:30:23
The propagation stands out in the northern direction. The associated flare is somehow not included in the NOAA list.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-12T17:58:49
2013-01-05T16:15:35 --> 2013-01-05T17:05:35
This is associated with a C1.3 flare. The mostly westward weak propagation seems to be hampered by the presence of an adjacent active region.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-12T17:49:19
2013-01-04T08:20:23 --> 2013-01-04T09:40:23
The propagation is mostly northward, and the associated eruption appears to be absorbed into a northern active region.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2013-01-10T02:54:04
2013-01-09T10:03:03 --> 2013-01-09T16:33:03
A rapid eruption, best seen in 171A, unleashes a sall coronal wave (211A). At the same time, there is a slow prominence eruption (annotated earlier) in where the wave passed by. It is not clear whether these two events are connected or influence one another.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2013-01-10T02:26:02
2013-01-09T01:00:03 --> 2013-01-09T08:12:03
A massive prominence lifts off on the SW limb. Most of it falls to a distant location as coronal rain, and there is a small blob which leaves the field of view in the SW direction. I am not sure whether to classify this event as a filament activation or a minor eruption so I mark it as both. It is definitely a beautiful event.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2013-01-10T02:07:43
2013-01-08T00:00:03 --> 2013-01-08T15:00:03
A prominence lifts and slowly swirls across the N limb, losing some material to the interplanetry space.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2013-01-09T02:36:29
2013-01-07T22:15:03 --> 2013-01-08T00:00:03
A small sigmoid on the N disk tries to erupt but does not go far.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2013-01-09T01:47:04
2013-01-07T07:57:03 --> 2013-01-07T09:51:03
Spray surge following a the C-class flare. Note that only its top part is lit in 304A channel. It is uncler whether this eruption is copmplete or if all the material falls back to the surface.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2013-01-09T00:10:40
2012-12-20T00:54:03 --> 2012-12-20T05:18:03
Eruption of a faint filament in the QS area. Notice the prior surge and darkening in the AR immediately to the S of this filament
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-04T21:36:28
2013-01-01T06:50:23 --> 2013-01-01T08:20:23
This event may be a confined (failed) eruption but there is at least some dimming high in the corona.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-04T21:25:54
2012-12-26T00:10:11 --> 2013-01-03T21:10:11
This cavity should be located at very high latitudes since it (and the associated prominence) does not seem to move substantially with solar rotation over the 9-day period or at least for the last 7 days.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-04T20:50:05
2013-01-03T01:10:11 --> 2013-01-03T02:10:11
This may at first look like another backside event. However, a small eruption is found on the visible side to precede the dimming at high altitudes.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-04T20:30:45
2013-01-03T09:00:03 --> 2013-01-03T10:30:03
Material is injected from the southern leg, apparently moving the northern leg of a cus-like loop system.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-04T19:41:00
2013-01-02T17:00:03 --> 2013-01-02T18:20:03
The filament material largely falls back as seen in 304 A images, but the higher corona seems to be partly opened up by the eruption. The associated CME is marginal.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-04T19:27:32
2013-01-02T06:00:03 --> 2013-01-02T08:00:03
Perhaps the prominence started to be activated a little earlier, but the movie captures its rotating motions projected on the plane of the sky. The corona at higher altitudes slightly dimmed as the prominence gets accelerated.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-04T17:40:15
2013-01-01T01:45:35 --> 2013-01-01T03:05:35
Another jet from a high-latitude region in the northern hemisphere. The region appears to be just on the limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-04T16:03:42
2012-12-31T16:00:04 --> 2012-12-31T18:30:04
Although much of the erupted material seems to fall back, the erution makes it into the interplanetary space as a minor CME. The eruption is associated with a B-class flare not registered in the NOAA flare list.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2013-01-04T08:05:52
2012-12-30T19:00:03 --> 2012-12-30T21:00:03
Although the source region appears to be not deeply occulted, the eruption is not spectacular in these images. The associated CME is also marginal.