Quantifying the Propagation of Fast Coronal Mass Ejections from the Sun to Interplanetary Space by Combining Remote Sensing and Multi-point In Situ Observations
Authors: Xiaowei Zhao, Ying D. Liu, Huidong Hu, and Rui Wang
2019 The Astrophysical Journal882122.
Provider: AAS Journals
Caption: Figure 10.
Similar to Figure 5, but for the overall propagation profile of the 2000 June 6 CME-driven shock from the Sun far into interplanetary space. Large blue dots show shock arrival times at 1.5, 2.0, 2.5, 3.0, and 3.34 au (Ulysses) predicted by the MHD model.