Recent Events Reported by Observers
Previous NextDetected by schryver, Submitted at 2013-10-18T00:12:59
2013-10-16T05:04:03 --> 2013-10-16T08:48:03
W-limb eruption
Detected by schryver, Submitted at 2013-10-16T23:14:42
2013-10-15T00:00:03 --> 2013-10-16T03:00:03
Smallish active regions and their surroundings exhibit multiple eruptions and flares (high-C and low-M) as activity couples from one region into another, including high over the SW limb.
Detected by schryver, Submitted at 2013-10-16T23:14:41
2013-10-15T00:00:03 --> 2013-10-16T03:00:03
Smallish active regions and their surroundings exhibit multiple eruptions and flares (high-C and low-M) as activity couples from one region into another, including high over the SW limb.
Detected by schryver, Submitted at 2013-10-16T23:14:41
2013-10-15T00:00:03 --> 2013-10-16T03:00:03
Smallish active regions and their surroundings exhibit multiple eruptions and flares (high-C and low-M) as activity couples from one region into another, including high over the SW limb.
Detected by halocme, Submitted at 2013-10-16T02:55:35
2013-10-13T00:00:03 --> 2013-10-13T02:30:03
The M1.7 flare associated with a halo CME and large-scale coronal propagating front is accompanied by activities in other regions. Four regions are seen to flare or erupt. Let's call them 1, 2, 3 and 4 from east to west. Obviously region 3 was the first (C1.2 flare minutes before the M1.7 flare), but regions 1, 2 and 4 seem to nearly simultaneously erupt. The apparent halo may be contributed by more than region 2, responsible for the M1.7 flare.
Detected by halocme, Submitted at 2013-10-16T02:55:36
2013-10-13T00:00:03 --> 2013-10-13T02:30:03
The M1.7 flare associated with a halo CME and large-scale coronal propagating front is accompanied by activities in other regions. Four regions are seen to flare or erupt. Let's call them 1, 2, 3 and 4 from east to west. Obviously region 3 was the first (C1.2 flare minutes before the M1.7 flare), but regions 1, 2 and 4 seem to nearly simultaneously erupt. The apparent halo may be contributed by more than region 2, responsible for the M1.7 flare.
Detected by halocme, Submitted at 2013-10-16T02:45:07
2013-10-13T00:00:03 --> 2013-10-13T02:30:03
This eruption is associated with a halo CME observed by LASCO. The front does not appear sharp, and it becomes clear only far from the flare location.
Detected by halocme, Submitted at 2013-10-16T02:45:07
2013-10-13T00:00:03 --> 2013-10-13T02:30:03
This eruption is associated with a halo CME observed by LASCO. The front does not appear sharp, and it becomes clear only far from the flare location.
Detected by halocme, Submitted at 2013-10-16T02:45:06
2013-10-13T00:00:03 --> 2013-10-13T02:30:03
This eruption is associated with a halo CME observed by LASCO. The front does not appear sharp, and it becomes clear only far from the flare location.
Detected by halocme, Submitted at 2013-10-16T02:36:28
2013-10-13T10:30:35 --> 2013-10-13T16:00:35
This prominence seems to gradually collapse down. The overlying corona is seen to dim slowly. This may be the origin of the slow, diffuse and structured CME, whose first appearance in LASCO data is not well defined.
Detected by halocme, Submitted at 2013-10-16T02:36:28
2013-10-13T10:30:35 --> 2013-10-13T16:00:35
This prominence seems to gradually collapse down. The overlying corona is seen to dim slowly. This may be the origin of the slow, diffuse and structured CME, whose first appearance in LASCO data is not well defined.
Detected by halocme, Submitted at 2013-10-16T02:36:27
2013-10-13T10:30:35 --> 2013-10-13T16:00:35
This prominence seems to gradually collapse down. The overlying corona is seen to dim slowly. This may be the origin of the slow, diffuse and structured CME, whose first appearance in LASCO data is not well defined.
Detected by halocme, Submitted at 2013-10-16T02:28:55
2013-10-13T10:30:35 --> 2013-10-13T16:00:35
Mass is seen to move from one leg to another of the prominence. These motions may underlie an eruption. But the overlying corona does not seem to be affected. The possibly associated CME is narrow.
Detected by halocme, Submitted at 2013-10-16T02:28:55
2013-10-13T10:30:35 --> 2013-10-13T16:00:35
Mass is seen to move from one leg to another of the prominence. These motions may underlie an eruption. But the overlying corona does not seem to be affected. The possibly associated CME is narrow.
Detected by halocme, Submitted at 2013-10-16T02:14:54
2013-10-13T08:00:03 --> 2013-10-13T09:00:03
Although flare ribbons and dimming are seen, this seems to be a failed eruption.
Detected by halocme, Submitted at 2013-10-16T02:14:53
2013-10-13T08:00:03 --> 2013-10-13T09:00:03
Although flare ribbons and dimming are seen, this seems to be a failed eruption.
Detected by halocme, Submitted at 2013-10-16T02:08:49
2013-10-13T06:45:35 --> 2013-10-13T08:25:11
The bright prominence is seen to push overlying structures into a large eruption, although CME association is unclear due to LASCO data gap and to a prior halo event. STEREO-B data show that the source region is about 10 degrees behind the limb and that it is not an active region.
Detected by halocme, Submitted at 2013-10-16T02:08:49
2013-10-13T06:45:35 --> 2013-10-13T08:25:11
The bright prominence is seen to push overlying structures into a large eruption, although CME association is unclear due to LASCO data gap and to a prior halo event. STEREO-B data show that the source region is about 10 degrees behind the limb and that it is not an active region.
Detected by halocme, Submitted at 2013-10-16T02:08:48
2013-10-13T06:45:35 --> 2013-10-13T08:25:11
The bright prominence is seen to push overlying structures into a large eruption, although CME association is unclear due to LASCO data gap and to a prior halo event. STEREO-B data show that the source region is about 10 degrees behind the limb and that it is not an active region.
Detected by halocme, Submitted at 2013-10-16T01:37:57
2013-10-13T04:50:23 --> 2013-10-13T06:20:23
The loops that encompass the whole active region erupted, followed by another eruption of loops in the western part. Neither of them leaves traces in coronagraph data.