Formation of the bow shock indentation: MHD simulation results

Simulation results from a global magnetohydrodynamic (MHD) model are used to examine whether the bow shock has an indentation and characterize its formation conditions, as well as its physical mechanism. The bow shock is identified by an increase in plasma density of the solar wind, and the indentat...

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Bibliographic Details
Main Authors: BaoHang Qu, JianYong Lu, Ming Wang, HuanZhi Yuan, Yue Zhou, HanXiao Zhang
Format: Article
Language:English
Published: Science Press 2021-05-01
Series:Earth and Planetary Physics
Subjects:
Online Access:http://www.eppcgs.org/article/doi/10.26464/epp2021033?pageType=en