Flux and polarization reflected from a nonconservative Rayleigh-scattering planetary atmosphere

Details Flux and polarization reflected from a nonconservative Rayleigh-scattering planetary atmosphere Flux and polarization reflected from a nonconservative Rayleigh-scattering planetary atmosphere

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990em%26p...48...41v&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 48, Jan. 1990, p. 41-48.

Physics

1

Planetary Atmospheres, Polarized Electromagnetic Radiation, Rayleigh Scattering, Venus Clouds, Atmospheric Composition, Solar Planetary Interactions, Venus Atmosphere

Scientific paper

The effects associated with the nonconservativeness of the Rayleigh-scattering atmosphere of a planet and the different states of polarization of the incident radiation on the phase curves for both flux and polarization were estimated, assuming that the Rayleigh-scattering atmosphere of a planet is homogeneous and plane-parallel. Results indicate that, in the present model, the effects are rather pronounced, thus making it possible to understand the physical situation in real planetary atmospheres.

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