Based on maximum speed of 330 km/s, the search window starts from 2012/12/08 02:00 UT
2012/12/08
==> Faint CME at 10:36, moving with 104 km/s.
Distinguishable narrow CME in both COR2-A and COR2-B, it was moving in the front side of the Sun.
SS: Eruption from decayed AR (~S29E28), filament or hot channel structure is not observed.
Could be the source of the disturbance.
2012/12/09
==> Partial halo CME at 18:00 UT.
SS: Eruption near the western limb
Unlikely the source of disturbance due to location of eruption and propagation direction of CME.
2012/12/10
==> Narrow CME (angular width 52) at 08:12 UT, moving with 143 km/s
Hard to identify on COR2-A and COR2-B. Observed in COR1-B (6:26 UT)
SS: Associated with C5.5 (starting at 05:49)flare from AR 11630 (~N19E1).
Could be the source of disturbance.
==> Partial halo CME at 13:36, moving with 226 km/s
SEEDS movie for COR2 is not available during this time. Seen as southward moving CME in COR1-A data (13:15 UT)
SS: Filament eruption from ~S25E62.
Unlikely to be related to the disturbance due to propagation direction of CME.
==> Partial Halo CME at 15:48, moving with 305 km/s
SS: erupted from the backside of the Sun
Unlikely the source of disturbance due to location of eruption
2012/12/11
==> Narrow CME (angular width 60) at 15:36, moving with 380 km/s
Seen as distinguishable narrow CME in both COR2-A and COR2-B, moving in the front side of the Sun.
SS: Filament eruption from ~S21E19 around 14:35 UT, not associated with any major flare.
Could be the source of disturbance.
Curators: Jie Zhang (jzhang7 AT gmu.edu); Suman Dhakal (sdhakal2 AT masonlive.gmu.edu);
Last updated:
2022/01