ANALYTICAL MODEL OF THE PLANETARY BOW SHOCK FOR VARIOUS MAGNETIC FIELD DIRECTIONS BASED ON MHD CALCULATIONS

Study of physical processes in plasma near planets often requires knowledge of the position and shape of the planetary bow shock. Empirical models are usually used since theoretical MHD and kinetic models consume too much computer time and cannot be used to track fast processes. M.I. Verigin propose...

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Bibliographic Details
Main Authors: G.A. Kotova, M.I. Verigin, T. Gombosi, K. Kabin
Format: Article
Language:English
Published: INFRA-M 2020-12-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/en/nauka/article/41326/view