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ABOUT CERTAIN APPROXIMATED SOLUTIONS OF GAS DYNAMIC EQUATIONS (O NEKOTORYKH PRIBLIZHENNYKH RESHENIYAKH URAVNENII GAZODINAMIKI),
FOREIGN TECHNOLOGY DIV WRIGHT-PATTERSON AFB OHIO
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Part 1 is a discussion of methods for the study of the dissipation of a shock wave in a stellar atmosphere. Part 2 analyzes the possibility of the extended atmosphere of a star being maintained by periodic shock waves. Part 3 reviews studies of the structure of a shock wave accompanied by radiation. The studies of 29 authors are cited to indicate that the possibilities of solving the three mentioned problems have by no means been exhausted. Author
APPROVED FOR PUBLIC RELEASE