Structure of discontinuous flows in dispersive hydrodynamics of planetary atmospheres

Details Structure of discontinuous flows in dispersive hydrodynamics of planetary atmospheres Structure of discontinuous flows in dispersive hydrodynamics of planetary atmospheres

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985stoc.iafct....p&link_type=abstract

IAF, International Astronautical Congress, 36th, Stockholm, Sweden, Oct. 7-12, 1985. 8 p.

Statistics

Computation

Collisionless Plasmas, Computational Fluid Dynamics, Hydrodynamics, Planetary Atmospheres, Unsteady Flow, Wave Propagation, Boltzmann Distribution, Electron Density (Concentration), Euler Equations Of Motion, Gas Dynamics, Ion Density (Concentration), One Dimensional Flow, Planetary Ionospheres, Solar Wind, Solitary Waves, Steady Flow

Scientific paper

The use of nondissipative dispersive hydrodynamics to analyze body motion in ionospheres or solar wind flows around planets is reviewed. Results obtained for the problem of unsteady flows in dispersive hydrodynamics are applied to the problem of arbitrary discontinuity evolution in plasma flows around bodies. The piston model of two-dimensional steady high-speed flow around a body is considered for both compression and rarefaction flows.

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