Single-Fluid Models for Astrophysical Plasma

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


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.


Electric Resistivity Solar Corona Magnetic Reynolds Number Pressure Tensor Astrophysical Plasma 
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Copyright information

© Springer Science+Business Media, LLC 2006

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