Radiative transfer model for a spherical atmosphere.
A new model for computing radiative transfer in a spherically symmetric atmosphere has been developed which uses a Gauss-Sidel iteration similar to Herman(1963). To account for inhomogeneities in the horizontal intensity field, the current work introduces a conical boundary on which solutions are fo...
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| Language: | en |
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The University of Arizona.
1990
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| Online Access: | http://hdl.handle.net/10150/185288 |