On the basis of experimental data both published and obtained by the author
s on radiation excited in CO2-N-2-Ar mixtures by shock waves, a physicochem
ical model of such mixtures is developed that can be recommended for calcul
ating the heat exchange and radiation of vehicles descending in the Martian
atmosphere. It is shown that the usually adopted assumption of the locally
equilibrium population of the electron-exited states is invalid. This make
s it necessary to consider each electron-excited state separately. The rate
constants of the excitation processes of electron states CN(A(2)Pi), CN(B(
2)Sigma (+)), and C-2(d(3)Pi (g)) produced as a result of collisions with h
eavy particles are determined. (C) 2001 MAIK "Nauka/Interperiodica"..