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The static radiative transfer equation in 3-D may be written
 |
(1) |
where
is the specific intensity at frequency
, position
, in the direction
,
is the emissivity at frequency
and position
, and
is the total
extinction at frequency
and position
. The source function
. Here, we will work in the steady-state so that
, and in Cartesian coordinates so
the
and the direction
is
defined by two angles
at the position
.
Peter Hauschildt
2006-01-09