Single-Fluid Models for Astrophysical Plasma
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.
KeywordsElectric Resistivity Solar Corona Magnetic Reynolds Number Pressure Tensor Astrophysical Plasma
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