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Plasma Astrophysics, Part I pp 237–262Cite as

Single-Fluid Models for Astrophysical Plasma

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 391))

Abstract

Single-fluid models are the simplest but sufficient approximation to describe many large-scale low-frequency phenomena in astrophysical plasma: regular and turbulent dynamo, plasma motions driven by strong magnetic fields, accretion disks, and relativistic jets.

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Somov, B.V. (2013). Single-Fluid Models for Astrophysical Plasma. In: Plasma Astrophysics, Part I. Astrophysics and Space Science Library, vol 391. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-4283-7_12

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