Numerical study of the propagation characteristics of coronal mass ejections in a structured ambient solar wind-Reference-Cited by-同舟云学术

Numerical study of the propagation characteristics of coronal mass ejections in a structured ambient solar wind

Published:2017-02 Issue:2 Volume:122 Page:1451-1462
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Zhou Yufen¹²^ORCID,Feng Xueshang¹

Affiliation:

1. SIGMA Weather Group, State Key Laboratory of Space WeatherNational Space Science Center, Chinese Academy of Science Beijing China

2. CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary SciencesUniversity of Science and Technology of China Hefei China

Funder

National Natural Science Foundation of China

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016JA023053

Reference41 articles.

1. Solar wind helium and hydrogen structure near the heliospheric current sheet: A signal of coronal streamers at 1 AU

2. Propagation of an Earth-directed coronal mass ejection in three dimensions

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