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In t h i s paper we consider an inviscid, thermal conductive, spherically symmetric model of the solar wind.The equations of mass, momentum and energy conservation are integrated simultaneously to give a unique solution for t h i s solar wind model.The solution obtained smoothly passes through the critical radius and satisfies the condition T = o as r-roo.The quantitative physical implication of the solution i s discussed.
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Whang et al. (1965) studied this question.
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