COMPUTER PROGRAMS AND NUMERICAL RESULTS RELATED TO THE PROBLEM OF THE SOLAR WIND.
Final rept. pt. 2,
AMERICAN SCIENCE AND ENGINEERING INC CAMBRIDGE MASS
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Numerical integrations of the differential equations of several hydrodynamical models of the solar wind have been performed for various sets of initial conditions. The method of integration is described and a summary of the results given together with a listing of the FORTRAN programs used. Also included are tables of various quantities related to the theory of atmospheric evaporation as applied to the solar corona. Author