Elastic radiative transfer equations have recently been derived to des
cribe the evolution of seismic energy in the dust of the earth (Ryzhik
et al., 1996), These equations are derived from a rigorous statistica
l treatment of the elastic-wave equation and include both shear polari
zations and mode conversion between the P and S modes. Calculations of
attenuations ratios and diffusion constants based upon these theories
are made and compared with values used in the literature, Equivalent
elastic radiative transfer equations have also been previously derived
for ultrasonic materials characterization purposes using a different
method, Observations made from numerical solutions of these ultrasonic
radiative transfer equations are discussed with application to seismo
logy, Both the steady-state and time-dependent solutions have been exa
mined including effects from boundaries, depolarization of S waves app
roach to isotropy of energy, and validity of the diffusion approximati
on, Similar results are expected for seismology.