Abstract
The laws of evolution of spherically symmetrical explosions with a high initial energy concentration in the atmosphere at heights from 0 to 90 km are investigated. The processes of initial energy release are ignored, and the explosion is assumed to be massless, i.e., the initial data are specified in the form of a uniformly heated sphere with a constant air density. The results are obtained by radiative gasdynamic numerical calculations in the range of explosive energies from 4.2·1012 J to 4.2·1016. J.
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