Statistics – Computation
Scientific paper
Jun 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977fpd..confq....c&link_type=abstract
American Institute of Aeronautics and Astronautics, Fluid and Plasmadynamics Conference, 10th, Albuquerque, N. Mex., June 27-29,
Statistics
Computation
Axisymmetric Flow, Blunt Bodies, Solar Wind, Supersonic Flow, Astronomical Models, Euler Equations Of Motion, Hypersonic Flow, Steady Flow
Scientific paper
A recently developed axisymmetric implicit unsteady Euler equation solver has been applied to the calculation of solar wind flows past terrestrial planets. The primary emphasis of this paper is on the application of that computational technique to the calculation of the flow field properties of steady, axisymmetric, supersonic/hypersonic flows past blunt-nosed shapes characteristic of interplanetary solar wind flows past both magnetic and nonmagnetic planets. The purpose is to demonstrate both the accuracy and flexibility of this new technique as well as to present a novel application of such supersonic blunt-body procedures.
Chaussee D. S.
Spreiter John R.
Stahara Stephen S.
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