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 2014-03-07T00:23:33
2014-03-04T20:35:23 --> 2014-03-04T22:25:47
This eruption starts at a region without spots, but it produces two-ribbon emission and a post-eruption arcade.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-07T00:16:35
2014-03-04T20:08:23 --> 2014-03-04T21:50:23
The outflow over the limb signify an eruption from the far side that was contemporaneous with another eruption on the east limb.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-07T00:09:19
2014-03-04T17:35:23 --> 2014-03-04T19:16:11
This eruption seems to preceded by downflows in the surrouding area. The expansion of the core field is seen in all the three channels in this movie. The event is associated with a gradual C5.5 flare.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-07T00:09:18
2014-03-04T17:35:23 --> 2014-03-04T19:16:11
This eruption seems to preceded by downflows in the surrouding area. The expansion of the core field is seen in all the three channels in this movie. The event is associated with a gradual C5.5 flare.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-07T00:01:22
2014-03-04T10:50:23 --> 2014-03-04T12:20:23
This appears to be triggered by foot-point dynamics possibly flux emergence, reminiscent of the prevalent model of coronal jets. But the coronal response seems to be broader than what is considered to be a jet.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T23:53:50
2014-03-04T03:10:11 --> 2014-03-04T04:10:11
This outflow or eruption is very diffuse, but it is seen to follow a cusp-like structure.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T23:46:19
2014-03-03T23:50:23 --> 2014-03-04T01:20:23
The ejection is seen in 304 A, 211 A and 171 A images in emission. The source region is likely to be occulted, and the closed structure on the limb is not affected by this ejection.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T23:37:54
2014-03-03T18:20:23 --> 2014-03-03T20:20:23
Collimated eruptions are seen for more than two hours. It is hard to know exactly when and how this activity started.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T23:27:03
2014-03-03T11:00:03 --> 2014-03-03T13:30:03
Coronal loops over an active region are seen to expand in a sequence. We note four steps in this movie. They do not reflect in GOES X-ray light curves.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T23:17:42
2014-03-02T09:00:03 --> 2014-03-03T04:00:03
It took almost a day for this prominence to lift off - quietly. No related signatures are seen in 211 A or 171 A. The relation with the on-disk filament is also unclear.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T23:08:01
2014-03-02T16:10:11 --> 2014-03-02T19:00:11
This looks more like a rearrangement of coronal structures than an eruption. It may be due to changes in the photospheric field as suggested by frequent compact brightenings.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T23:00:50
2014-03-02T15:40:11 --> 2014-03-02T17:00:11
This jet-like outflow is again seen only in 304 A images indicating its low temperature.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T22:51:24
2014-03-02T08:00:03 --> 2014-03-02T13:00:03
These may not be distinguishable from prominences in the low latitude regions.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T22:29:31
2014-03-02T02:50:23 --> 2014-03-02T06:30:23
These outflows are seen only in 304 A images. They may be of backside origin. The closed structures and their dynamics including oscillations may happen to be in the same line of sight and are not related.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T22:19:35
2014-03-02T02:20:23 --> 2014-03-02T03:30:23
The compact eruption in the south at first looks like starting earlier than the more extended one in the north (with apparent dimming). But on a closer look they seem to start around the same time.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by halocme, Submitted at 2014-03-06T22:19:34
2014-03-02T02:20:23 --> 2014-03-02T03:30:23
The compact eruption in the south at first looks like starting earlier than the more extended one in the north (with apparent dimming). But on a closer look they seem to start around the same time.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by weiliu, Submitted at 2014-03-06T19:15:08
2014-03-06T09:10:03 --> 2014-03-06T16:00:03
A filament erupts, procuding two curved flare ribbons. Note a surge occurs in the nearby active region (to the north of the filament) during the filmament eruption.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by weiliu, Submitted at 2014-03-05T19:03:44
2014-03-04T20:00:03 --> 2014-03-05T02:00:03
Three eruptions one after another: the first one is a large, diffuse prominence eruption apparently from the south pole, then another prominence on the southwest limb lifts off and erupts, followed by another eruption next to it in the north evidently in the 171 channel like a puff.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2014-03-05T00:39:16
2014-03-01T11:54:03 --> 2014-03-01T14:44:03
Rather than emerging bubble, this event looks like a rapid "unzipping" of the background corona and rapid "zipping" back up.
Rating:
3.0 (0=lowest, 5=highest)
Num Ratings:1
Detected by anny, Submitted at 2014-03-05T00:22:09
2014-03-01T04:20:03 --> 2014-03-01T11:40:03
An eruption of a thin filament on the E limb.
