The stellar atmosphere physical system II. An operative sequential algorithm to solve the stellar atmosphere problem
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In this paper, the second and the last of the series, we present a sequential algorithm to solve the stellar atmosphere problem that may serve as a paradigm for the solution of more general non-linear and non-local problems. The Iteration Factors (IF) Method is applied to achieve a solution of the radiative transfer equations, consistent with the radiative equilibrium constraint.
1992 ◽
Vol 47
(2)
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pp. 121-126
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2020 ◽
Vol 80
(6)
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pp. 1650-1667
1987 ◽
Vol 16
(4-6)
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pp. 637-652
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2019 ◽
Vol 48
(5)
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pp. 180-199
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