Based on maximum speed (in-situ observation) of 720 km/s, the search window starts from 2013/03/14 20:16 UT
2013/03/14
Narrow front side moving CME appearing at LASCO FOV at 20:12 UT. It was moving with linear velocity of 206 km/s.
Unlikely to be related to the disturbance of 2013/03/17, based on the initial speed and maximum speed.
2013/03/15
Halo and front side moving, with linear velocity of 1063 km/s, CME at 07:12 UT.
Likely to be related to the disturbance of 2013/03/17
SS: M1.1 flare from NOAA AR 1692 (N09E06). AIA data gap during the flare, most probably due to AIA eclipse. GMU's ENLIL model run shows that this CME could produce disturbance on 2013/03/16 ~ 20:00 UT.
2013/03/16
Partial halo and front side moving CME appearing at 14:48 UT. It was moving with linear velocity of 786 km/s.
Unlikely to be related to the the disturbance of 2013/03/17, based on the starting time of disturbance and CME appearing time and propagating velocity.
2013/03/17
No CME seem to be related to the disturbance of 2013/03/17
Curators: Jie Zhang (jzhang7 AT gmu.edu); Suman Dhakal (sdhakal2 AT masonlive.gmu.edu);
Last updated:
2022/01