Numerical results for internal intensities in atmospheres illuminated by isotropic sources

by H. H. Natsuyama

Publisher: Rand Corporation in Santa Monica, Calif

Written in English
Published: Pages: 138 Downloads: 501
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  • Radiative transfer.,
  • Transport theory.

Edition Notes

Bibliography: p. 138.

StatementH.H. Kagiwada and R.E. Kalaba.
SeriesMemorandum -- RM-4958-PR, Research memorandum (Rand Corporation) -- RM-4958-PR..
ContributionsKalaba, Robert E.
The Physical Object
Paginationvii, 138 p. :
Number of Pages138
ID Numbers
Open LibraryOL17985034M

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Numerical results for internal intensities in atmospheres illuminated by isotropic sources by H. H. Natsuyama Download PDF EPUB FB2

Kagiwada and R. Kalaba, “Numerical Results for Internal Intensities in Atmospheres Illuminated by Isotropic Sources,” The Rand Corporation, RMPR, Google Scholar Author: Harriet H. Natsuyama, Sueo Ueno, Alan P. Wang. Radiation field of an optically finite homogeneous atmosphere with internal sources Article in Journal of Quantitative Spectroscopy and Radiative Transfer (10) · July with 3 Reads.

The Stokes parameters of the polarized radiation in a plane-parallel homogeneous atmosphere, which is solely illuminated by homogeneously distributed, isotropically radiating internal sources, are.

ICARUS 25, () Multiple Scattering in Planetary Atmospheres' WILLIAM M. IRVINE Department of Physics and Astronomy, University of Massachusetts, Amherst, Massachusetts Received December 11, Methods for solving radiative transfer problems within the extended visible spectrum in planetary atmospheres are reviewed for use by the by: A two-component method for solving multislab problems in radiative transfer.

for solving slab-geometry S N neutron transport problems with anisotropic scattering up to the first order and with isotropic constant internal sources. Numerical results for the diffuse component of the by: The numerical results show that for an atmosphere with uniformly distributed primary sources of partially polarized radiation, the matrix Eddington - Barbier relation holds: I(μ)=~S(τ=μ), where S(τ) is the matrix source function corresponding to this problem.

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na = nc + n s 1 − (1) Rs Rs To calculate characteristics of scattering for a separate concentric two-layered particle we used the algorithms described in [4].

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Eddy diffusion in the atmosphere is the process of transport of gases due to turbulent mixing in the presence of a composition gradient.

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