Figure 10 from Quantifying the Propagation of Fast Coronal Mass Ejections from the Sun to Interplanetary Space by Combining Remote Sensing and Multi-point In Situ Observations

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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 Journal 882 122.

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.

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