Radiative transfer in spherical shell atmospheres. III. Application to Venus
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference15 articles.
1. Radiative transfer in spherical shell atmospheres. I. Rayleigh Scattering;Adams;Icarus,1978
2. The atmosphere of Venus near her cloud tops;Chamberlain;Astrophys. J.,1965
3. Relative intensity calculations for carbon dioxide. III. Relative line intensities of transitions from the vibrational ground state for temperatures from 160° to 280°K;Gray;J. Quant. Spectrosc. Radiat. Transfer,1967
4. Interpretation of the polarization of venus;Hansen;J. Atmos. Sci.,1974
5. Radiative transfer in spherical shell atmospheres. II. Asymmetric phase function;Kattawar;Icarus,1978
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1. Revised and extended benchmark results for Rayleigh scattering of sunlight in spherical atmospheres;Journal of Quantitative Spectroscopy and Radiative Transfer;2020-10
2. Comparison of numerical models for computing underwater light fields;Applied Optics;1993-12-20
3. Light scattering in a spherical, exponential atmosphere, with applications to Venus;Icarus;1985-09
4. A reconsideration of the effective depth of line formation in planetary atmospheres;Earth, Moon and Planets;1984-04
5. Effective depth of spectral line formation in planetary atmospheres;Icarus;1980-12
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