Radiative transfer in scattering stochastic atmospheres
  Many stars, active galactic nuclei, accretion discs etc. are affected by the
stochastic variations of temperature, turbulent gas motions, magnetic fields,
number densities of atoms and dust grains. These stochastic variations
influence on the extinction factors, Doppler widths of lines and so on. The
presence of many reasons for fluctuations gives rise to Gaussian distribution
of fluctuations. The usual models leave out of account the fluctuations. In
many cases the consideration of fluctuations improves the coincidence of
theoretical values with the observed data. The objective of this paper is the
investigation of the influence of the number density fluctuations on the form
of radiative transfer equations. We consider non-magnetized atmosphere in
continuum.
