PHSCS 645

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Magnetohydrodynamic Theory of Plasmas

Physics and Astronomy College of Computational, Mathematical, & Physical Sciences

Course Description

Plasma equilibrium and dynamics using magnetohydrodynamic theory with application to fusion and astrophysical plasmas.

When Taught

Contact Department

Min

3

Fixed/Max

3

Fixed

3

Fixed

0

Title

Divergence, Gradient, Curl, and Fluids

Learning Outcome

Be able to explain what the gradient, the directional derivative, divergence, and curl mean in fluid dynamics. Also be able to explain how these concepts are involved in cases of simple gas and fluid flow.

Title

Equilbrium and Stability

Learning Outcome

Demonstrate the ability to use the energy principle to predict whether MHD equilibria are stable or unstable.

Title

Applications

Learning Outcome

Be able to explain the physical origins and properties of the MHD instabilities and waves that are involved in magnetic fusion plasmas and astrophysical plasmas.

Title

MHD Equations

Learning Outcome

Be able to write down from memory the ideal MHD equations and be able to explain the physical meaning of the terms in these equations.

Title

Resistive Instabilities

Learning Outcome

Be able to explain the physical origin of resistive instabilities in non-ideal MHD.