Reflection and transmission of thin layers
Starting the adding-doubling method requires knowledge of the reflection and
transmission operators for a thin slab. Several methods exist for obtaining these
operators: diamond initialization [66], infinitesimal generator
[20], and successive scattering [28]. The first two methods
have been compared by Wiscombe who found that the more complicated diamond
initialization technique was better about two-thirds of the time [67].
The successive scattering technique was the first method used for calculating the
reflection and transmission operators of a thin slab [63].
With this method initial optical depths up to
are possible although
Hansen and Travis indicate that an optical thickness of
is optimal for this
starting method [24]. The infinitesimal generator technique
assumes that the tissue is sufficiently thin that single scattering accurately estimates
the reflection and transmission for the slab. This is the method implemented for
calculations in this chapter because of its simplicity.
Single scattering equations for the reflection and transmission functions are
given by van de Hulst for isotropic scattering [60]. For azimuthally
independent anisotropic scattering the redistribution function must be included. The
single scattering reflection function for thin layers is
![\begin{displaymath}
R(a,\tau,\mu,\mu_0) = {a \pi h(\mu,-\mu_0) \over \mu+\mu_0}
...
...ft[1-\exp\left(-{\tau\over\mu}-{\tau\over\mu_0}\right) \right]
\end{displaymath}](img162.gif) |
(3.30) |
The slight difference from van de Hulst results from differences in phase function
normalization. At grazing angles ( ), the reflection has a singularity
 |
(3.31) |
When the angle of incidence is not equal to the angle of transmission ( ),
then the transmission function is given by
![\begin{displaymath}
T(a,\tau,\mu,\mu_0) = {a \pi h(\mu,-\mu_0) \over \mu_0-\mu}
...
...u\over\mu_0}\right)
-\exp\left(-{\tau\over\mu}\right) \right]
\end{displaymath}](img166.gif) |
(3.32) |
When
then the primary beam (with an incident cone of )
must be included,
 |
(3.33) |
The factor of
in the unscattered beam results from the use of star multiplication.
Finally, for grazing incidence (
), the transmission is zero
 |
(3.34) |
|