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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 3.

Evolution of solar wind speeds from Wind to Ulysses via the 1D MHD model. The solid curves give the solar wind speeds observed at Wind and Ulysses, and the dotted curves represent the predicted speeds at specific distances. The red arrows indicate the progression of the modeled shock. The two red vertical dashed lines mark the observed shock arrival times at Wind and Ulysses, respectively. The same scales are used for all of the panels.

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