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B.d.iii. Solar radiation of dust
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The solar radiative transfer equations of dust
(A.31),
(A.32),
which are described in Appendix A.d.iii,
are discretized as follows.
When
Equations
(B.49),
(B.50)
can be formally represented in matrix form as follows.
Equations
(B.51),
(B.52)
are solved by an iteration method.
The elements of the these matrixes are represented as follows
(where
 ).
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