Based on maximum speed of 440 km/s, the search window starts from 2012/08/30 13:46 UT
2012/08/30
==> Partial Halo CME (angular width 130) at 15:12 UT, moving with 480 km/s
mostly moving northward
solar source is hard to identify
2012/08/31
==> Partial Halo CME (angular width 119) at 08:24 UT, moving with 480 km/s
mostly moving northward
solar source is hard to identify
==> CME (angular width 108) at 11:12 UT, moving with 706 km/s
not moving front side of the Sun.
==> Partial Halo CME (angular width 157) at 19:24 UT, moving with 278 km/s
Front side moving CME
Filament eruption from ~N18W46
could be the source of the disturbance.
==> Halo CME at 20:00 UT, moving with 1442 km/s
Halo CME in both COR2-A and COR2-B, frontside moving CME
Filament eruption from ~S27E50
Likely the source of disturbance.
2012/09/01
==> Partial Halo CME at 10:12 UT (angular width 136), moving with 598 km/s.
CME front is not clear in COR2-A and COR2-B, front side moving CME
Solar source is not clear, could be from 11560 (N04W05).
less likely the source of disturbance due to the time of eruption and initial propagation speed.
2012/09/02
No CMEs on this day seem to be related to the disturbance due to the time of origin and the propagation speed.
Curators: Jie Zhang (jzhang7 AT gmu.edu); Suman Dhakal (sdhakal2 AT masonlive.gmu.edu);
Last updated:
2022/01