Viscous solutions of the two-fluid solar wind equations

Details Viscous solutions of the two-fluid solar wind equations Viscous solutions of the two-fluid solar wind equations

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976p%26ss...24..799s&link_type=abstract

Planetary and Space Science, vol. 24, Aug. 1976, p. 799, 800. Science Research Council

Physics

Magnetohydrodynamic Flow, Solar Wind, Two Fluid Models, Viscous Flow, Differential Equations, Ideal Fluids, Steady Flow, Supersonic Flow

Scientific paper

The two-fluid equations describing the ideal, steady, viscous solar wind
are examined, and supersonic solutions are sought in which the electron
and ion temperatures vary as inverse powers of the radial distance from
the sun. Just two solutions are found, and these are analogous to those
found by Whang et al. (1966) and Dahlberg (1970) in one-fluid theory.

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