PTYS558
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PTYS558 - Plasma Physics with Astrophysical and Solar System Applications
Course ID
029006
Course Description
The goal of this course is to present an introduction to fundamental plasma physics and magnetohydrodymics, beginning with kinetic theory. The various important limits including the vlasov equation and magnetohydrodynamics will be derived. Applications will be mostly from astrophysics and the solar system. These will include the main dynamical processes in the solar atmosphere, interplanetary medium, magnetospheres, interstellar medium, blast waves, accretion disks, etc. The emphasis throughout will be on basic physical processes and the various approximations used in their application to concrete problems.
Min Units
3
Max Units
3
Repeatable for Credit
No
Grading Basis
GRD - Regular Grades A, B, C, D, E
Career
Graduate
Course Attributes
CE - CL (Cross Listed)
Course Requisites
Cross Listed Courses
May be convened with
Component
Lecture
Optional Component
No