The optimal forms of slender bodies with minimum aerodynamic heat moving in the atmospheres of planets of the Solar system.

Details The optimal forms of slender bodies with minimum aerodynamic heat moving in the atmospheres of planets of the Solar system. The optimal forms of slender bodies with minimum aerodynamic heat moving in the atmospheres of planets of the Solar system.

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kosis..29..397k&link_type=abstract

Kosmicheskie Issledovaniia, Tom 29, Vyp. 3, p. 397 - 403

Computer Science

Scientific paper

The paper describes the results of a numerical solution of the variational problems of a flat or axisymmetric body form determination from the condition of the minimum summary (convective and radiation) aerodynamic heat of its surface along the trajectory of motion in a planet's atmosphere. The solution is derived by the local variation method in the slender bodies class for various isoperimetric and boundary conditions. A comparison of optimal flat and axisymmetric bodies forms is realized. The authors calculate the convective and radiation heat coefficients, wave and friction drags and compare the characteristics of optimal bodies with cones and wedges.

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