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Numerical Computation in Magneto Fluid Dynamics
Numerical Computation in Magneto Fluid Dynamics
By Professor Robert W. MacCormack
Professor
Department of Aeronautics and Astronautics, Stanford University
Thu, Oct 9, 2008 2:30 PM
Location: Lopata Hall Room 101
This talk presents a numerical method for solving the Navier-Stokes equations coupled to Maxwell’s equations describing ionized flows within strong electric and magnetic fields. This set is difficult to solve because the characteristic speeds vary from the speed of sound to the speed of light. An algorithm and boundary condition procedures are presented for solving these equations. A scaling of the Maxwell flux vectors is used to control the numerical dissipation inherent in the Modified-Steger-Warming method used to solve the governing equations. This novel scaling procedure enabled both stable and accurate solutions to be found for these equations. This fully implicit numerical method is tested first on the Hartmann flow problem and then by simulating the flow within an MFD accelerator, generator and simplified scramjet engine (to be presented).
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Mechanical, Aerospace & Structural Engineering, Washington University in St. Louis
One Brookings Drive, Box 1185, St. Louis, Missouri 63130
Office Location: 305 Jolley Hall, Phone: (314) 935-6047, Fax: (314) 935-4014 |
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