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B.d.iii. Solar radiation of dust
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The the solar radiative transfer equation of dust
(A.31) and
(A.32)
described in appendix A.d.iii
are discretized as follows.
When  and so on,
(B.49) and
(B.50) can be formally represented in
matrix form as follows.
(B.51) and (B.52) are solved by iteration method.
The elements of the these matrixes are represented as follows
(where 0 ≤ j ≤ J ).
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