Hypersonic flow of a viscous radiating gas over blunted cones

Radiation gas dynamics of Martian space vehicles

“…In [1][2][3][4][5][6], important data on the features of the radiation convective heat exchange of SVs in atmo spheres composed of CO 2 and N 2 (atmospheres of Mars and Venus, in different percentage ratios) were obtained in the computational theoretical way. Papers [5,[8][9][10][11] can be mentioned as examples of the analy sis of the convective and radiation heating of the whole surface of a SV of a complex shape.…”

“…With respect to the atmo spheres of Mars and Venus, problems of the radiation convective heat exchange of descent SVs were solved earlier (starting from the 1960s) only for the frontal surface [1][2][3][4] using simplified equations of the dynamics of the radiative gas. The need for obtaining and analyzing new calculation data for the whole sur face of SVs is dictated by the heightened requirements for the aerothermodynamic design of descent SVs at present.…”