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Single-Fluid Models for Astrophysical Plasma

Part of the Astrophysics and Space Science Library book series (ASSL, volume 341)

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, accreation disks, and relativistic jets.

Keywords

Electric Resistivity Solar Corona Magnetic Reynolds Number Pressure Tensor Astrophysical Plasma 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media, LLC 2006

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