Recent Events Reported by Observers
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Detected by halocme, Submitted at 2013-10-16T01:15:06
2013-10-12T16:00:03 --> 2013-10-12T23:00:03
The prominence slowly rises, and at a certain height it decides to break up into the lower part which clearly goes back to the chromosphere, and the upper part, only small part of which is seen to erupt. Essentially this is a failed eruption and indeed there is hardly a CME in LASCO data.
Detected by halocme, Submitted at 2013-10-16T01:15:06
2013-10-12T16:00:03 --> 2013-10-12T23:00:03
The prominence slowly rises, and at a certain height it decides to break up into the lower part which clearly goes back to the chromosphere, and the upper part, only small part of which is seen to erupt. Essentially this is a failed eruption and indeed there is hardly a CME in LASCO data.
Detected by halocme, Submitted at 2013-10-16T01:15:05
2013-10-12T16:00:03 --> 2013-10-12T23:00:03
The prominence slowly rises, and at a certain height it decides to break up into the lower part which clearly goes back to the chromosphere, and the upper part, only small part of which is seen to erupt. Essentially this is a failed eruption and indeed there is hardly a CME in LASCO data.
Detected by schryver, Submitted at 2013-10-15T23:19:25
2013-10-14T12:40:07 --> 2013-10-14T20:36:07
Two subsequent eruptions occur on a smallish AR in the southern hemisphere, associated ffirst with a high C-class eruptive flare within the AR, then disrupting the field into the leading QS region..
Detected by schryver, Submitted at 2013-10-15T23:19:25
2013-10-14T12:40:07 --> 2013-10-14T20:36:07
Two subsequent eruptions occur on a smallish AR in the southern hemisphere, associated ffirst with a high C-class eruptive flare within the AR, then disrupting the field into the leading QS region..
Detected by schryver, Submitted at 2013-10-15T23:06:55
2013-10-14T00:00:07 --> 2013-10-15T00:00:07
A QS filament approaching the NW limb shows continued activity, often almost surge-like, sometimes extending into the trailing QS region.
Detected by halocme, Submitted at 2013-10-15T22:41:46
2013-10-11T12:00:00 --> 2013-10-11T14:00:00
This flare is highly eruptive, a cusp-like structure is seen at high temperatures as well as coronal dimming.
Detected by halocme, Submitted at 2013-10-15T22:41:46
2013-10-11T12:00:00 --> 2013-10-11T14:00:00
This flare is highly eruptive, a cusp-like structure is seen at high temperatures as well as coronal dimming.
Detected by halocme, Submitted at 2013-10-15T22:41:45
2013-10-11T12:00:00 --> 2013-10-11T14:00:00
This flare is highly eruptive, a cusp-like structure is seen at high temperatures as well as coronal dimming.
Detected by halocme, Submitted at 2013-10-15T21:37:35
2013-10-12T14:00:07 --> 2013-10-12T16:30:07
A local erupting plasma interacted with large-scale field that was highly non-radial. The multiplicity of the jet may reflect interactions with adjacent and similarly oriented field.
Detected by halocme, Submitted at 2013-10-15T04:57:02
2013-10-12T17:30:35 --> 2013-10-12T20:00:35
A small eruption in the same active region that produced a M1.5 flare on 11 October 2013 is highly non-radial, disturbing trans-equatorial loops. An outflow may be seen in LASCO at a barely detectable level, but not a CME.
Detected by halocme, Submitted at 2013-10-15T03:54:25
2013-10-12T15:50:23 --> 2013-10-12T16:20:23
Dark regions in EUV (e.g., 211 A) images may be called coronal holes, but mixed polarity areas exist therein. This example shows a small eruption associated with flux emergence or cancellation within a so-called coronal hole.
Detected by halocme, Submitted at 2013-10-15T03:54:24
2013-10-12T15:50:23 --> 2013-10-12T16:20:23
Dark regions in EUV (e.g., 211 A) images may be called coronal holes, but mixed polarity areas exist therein. This example shows a small eruption associated with flux emergence or cancellation within a so-called coronal hole.
Detected by halocme, Submitted at 2013-10-15T03:19:18
2013-10-12T13:00:03 --> 2013-10-12T16:00:03
The eruption of the bright prominence in 304 A images does not give an impression that it made it to the heliosphere, but at least a real CME with internal structures, although slow, seems to be associated. Closed loops to the south expanded before the prominence eruption, and they hardly reached the LASCO FOV.
Detected by halocme, Submitted at 2013-10-15T03:19:18
2013-10-12T13:00:03 --> 2013-10-12T16:00:03
The eruption of the bright prominence in 304 A images does not give an impression that it made it to the heliosphere, but at least a real CME with internal structures, although slow, seems to be associated. Closed loops to the south expanded before the prominence eruption, and they hardly reached the LASCO FOV.
Detected by halocme, Submitted at 2013-10-14T22:33:06
2013-10-11T15:00:11 --> 2013-10-11T18:00:11
There is no associated feature on the visible disk (such as post-eruption arcades), so this diffuse eruption (found only in difference movies) is probably from the backside.
Detected by anny, Submitted at 2013-10-11T23:25:08
2013-10-07T03:42:35 --> 2013-10-07T18:42:35
Two dipoles are located right next to each other, one above the other, with their axes parallel (but the polarities reversed) and their centers vertically co-aligned. The structure of the 171A loops is suggestive of a coronal null in the middle of the resulting quadrupolar structure. All of a sudden, a coronal dimming in 171A and in 211A explosively develops around the presumed null. This event might be valuable for studies of coronal reconnection, because of its simple geometry, the clearly visible pre- and post- event loops and the proximity of the structure to the disk center.
Detected by anny, Submitted at 2013-10-11T23:25:07
2013-10-07T03:42:35 --> 2013-10-07T18:42:35
Two dipoles are located right next to each other, one above the other, with their axes parallel (but the polarities reversed) and their centers vertically co-aligned. The structure of the 171A loops is suggestive of a coronal null in the middle of the resulting quadrupolar structure. All of a sudden, a coronal dimming in 171A and in 211A explosively develops around the presumed null. This event might be valuable for studies of coronal reconnection, because of its simple geometry, the clearly visible pre- and post- event loops and the proximity of the structure to the disk center.
Detected by anny, Submitted at 2013-10-11T23:25:07
2013-10-07T03:42:35 --> 2013-10-07T18:42:35
Two dipoles are located right next to each other, one above the other, with their axes parallel (but the polarities reversed) and their centers vertically co-aligned. The structure of the 171A loops is suggestive of a coronal null in the middle of the resulting quadrupolar structure. All of a sudden, a coronal dimming in 171A and in 211A explosively develops around the presumed null. This event might be valuable for studies of coronal reconnection, because of its simple geometry, the clearly visible pre- and post- event loops and the proximity of the structure to the disk center.
Detected by anny, Submitted at 2013-10-11T23:40:24
2013-10-07T03:42:35 --> 2013-10-07T18:42:35
Two dipoles are located right next to each other, one above the other, with their axes parallel (but the polarities reversed) and their centers vertically co-aligned. The structure of the 171A loops is suggestive of a coronal null in the middle of the resulting quadrupolar structure. All of a sudden, a coronal dimming in 171A and in 211A explosively develops around the presumed null. This event might be valuable for studies of coronal reconnection, because of its simple geometry, the clearly visible pre- and post- event loops and the proximity of the structure to the disk center.
