Based on maximum speed of 380 km/s, the search window starts from 2011/09/30 12:00 UT
2011/09/30
==> Partial Halo CME aat 20:00 UT (angular width 183), moving with 337 km/s
small CME in both COR2-A and COR2-B FOV, frontside moving CME
Eruption from AR 11305 (N08E06), associated with M1.0 flare (onset 18:55)
could be the source of disturbance
2011/10/01
==> Partial Halo CME at 01:25 UT (angular width 241), moving with 745 km/s
backside event COR2-A and COR2-B FOV, frontside moving CME
==> Partial Halo CME at 09:36 UT (angular width 203), moving with 448 km/s
Major CME in both COR2-A and COR2-B FOV, frontside moving CME
Eruption from AR 11305 (N09W04), associated with M1.2 flare (onset 08:56)
could be the source of disturbance
==> Halo CME at 20:48 UT, moving with 1238 km/s
Halo CME in both COR2-A and COR2-B FOV
backside eruption
2011/10/02
==> CME at 02:00 UT (angular width 103), moving with 259 km/s
Moderate CME in both COR2-A and COR2-B FOV, frontside moving CME
Eruption from AR 11305 (N09W12), associated with M3.9 flare (onset 00:37)
could be the source of disturbance
==> CME at 22:12 UT (angular width 66), moving with 386 km/s
small CME in both COR2-A and COR2-B FOV, frontside moving CME
Eruption from AR 11305 (N09W25), associated with C7.6 flare (onset 21:20)
likely the source of disturbance
2011/10/03
==> CME around 02:00 UT, not in CDAW catalog
Major CME in both COR2-A an COR2-B FOV, frontside moving CME
eruption from NW limb
less likely the source of disturbance due to the location of eruption
2011/10/04
==> CME at 12:12 UT (angular width 124), moving with 393 km/s
small CME in both COR2-A and COR2-B FOV, frontside moving CME
Eruption from AR 11310 (~S33E19), not associated with any major flare
less likely the source of disturbance due to the location of eruption
==> Halo CME at 13:25 UT, moving with 1101 km/s
backside eruption
==> CME at 17:24 UT (angular width 109), moving with 295 km/s
major CME in both COR2-A and COR2-B FOV, frontside moving CME
Filament eruption from ~S29W52, not associated with any major flare
less likely the source of disturbance due to the time of eruption
2011/10/05
No CMEs on this day seem To be related to the disturbance
Curators: Jie Zhang (jzhang7 AT gmu.edu); Suman Dhakal (sdhakal2 AT masonlive.gmu.edu);
Last updated:
2022/01