A mathematical model of solar wind flow.

Details A mathematical model of solar wind flow. A mathematical model of solar wind flow.

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995jmps...29..253m&link_type=abstract

Journal of Mathematical Physics Sci., Vol. 29, No. 6, p. 253 - 261

Mathematics

Mathematical Physics

Solar Wind: Models

Scientific paper

In order to study the continuous emission of the solar corona, the fluid dynamical models of a spherically symmetric, expanding and heat conducting gas under gravity is considered. On the basis of certain simplifying postulates, the fluid equations of continuity, momentum, energy and a thermodynamic relation that involve entropy, are obtained and solved analytically. The topology of the results shows the existence of two critical solutions (one increasing and the other decreasing) passing through their bifurcation point.

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