Abstract
As was shown in the previous section, the system of magnetohydrodynamic equations for an ideal medium in the approximation of strong field and cold plasma is characterized by the only small parameter \( \varepsilon ={{v} \left/ {{{V_A}}} \right.} \):
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© 1994 Springer Science+Business Media Dordrecht
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Somov, B.V. (1994). Plasma Flows in a Strong Magnetic Field. In: Fundamentals of Cosmic Electrodynamics. Astrophysics and Space Science Library, vol 191. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1184-3_8
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DOI: https://doi.org/10.1007/978-94-011-1184-3_8
Publisher Name: Springer, Dordrecht
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