  This paper calculates the spatial distribution of the plasma responsible for
radar head echoes by applying the kinetic theory developed in the companion
paper (Dimant and Oppenheim, arXiv:1608.08524). This results in a set of
analytic expressions for the plasma density as a function of distance from the
meteoroid. It shows that, at distances less than a collisional mean-free-path
from the meteoroid surface, the plasma density drops in proportion to $1/R$
where $R$ is the distance from the meteoroid center; and, at distances much
longer than the mean-free-path behind the meteoroid, the density diminishes at
a rate proportional to $1/R^{2}$. The results of this paper should be used for
modeling and analysis of radar head echoes.
