A 3D Parametric Venusian Bow Shock Model with the Effects of Mach Number and Interplanetary Magnetic Field

A 3D Parametric Venusian Bow Shock Model with the Effects of Mach Number and Interplanetary Magnetic Field

Using global magnetohydrodynamics simulations, we have developed a three-dimensional parametric model for the Venusian bow shock based on a generalized conic section function defined by six parameters, with the effects of the solar wind magnetosonic Mach number ( M _MS ) and the interplanetary magne...

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Bibliographic Details
Main Authors: Ming Wang, Qi Xu, Lianghai Xie, Lei Li, Xiaojun Xu
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astronomical Journal
Subjects:
Magnetohydrodynamics
Planetary bow shocks
Solar-planetary interactions
Venus
Online Access:https://doi.org/10.3847/1538-3881/ad192d

Internet

https://doi.org/10.3847/1538-3881/ad192d

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