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The asymptotic behavior of the supersonic solutions of the two-fluid solar wind equations
Authors:I W Roxburgh
Institution:(1) Advanced Study Program, National Center for Atmospheric Research, Boulder, Colo., U.S.A.;(2) Queen Mary College, University of London, London, England
Abstract:Three different asymptotic branches of the two-fluid equations are found with tau e agrlambda m , tau p agrlambda n , where, lambda is the inverse distance from the Sun, with (m, n) = (2/7, 2/7), (2/7, 6/7), (4/3, 4/3); other special solutions are also found but they correspond to special choices of density and temperature at the corona. In all the (4/3, 4/3) solutions, the electron and proton temperatures tend to equality at large distances.The National Center for Atmospheric Research is sponsored by the National Science Foundation.
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