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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 4.

Dynamic spectrum associated with the 1997 November 4 CME from Wind. The vertical dashed line indicates the shock arrival time at the Earth. The white arrows indicate the observed type II radio bands. The black dotted curve is obtained from the simple analytical model, which simulates the frequency drift of the observed type II radio burst at the harmonic plasma frequency. The white dotted curve is derived by dividing the harmonic curve by a factor of 2.

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