Light scattering by an optically thin inhomogeneous, spherically-symmetric planetary atmosphere - Brightness at the zenith near the terminator

Details Light scattering by an optically thin inhomogeneous, spherically-symmetric planetary atmosphere - Brightness at the zenith near the terminator Light scattering by an optically thin inhomogeneous, spherically-symmetric planetary atmosphere - Brightness at the zenith near the terminator

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..71..405w&link_type=abstract

Astrophysics and Space Science, vol. 71, no. 2, Aug. 1980, p. 405-410.

Physics

Optics

2

Atmospheric Optics, Light Scattering, Planetary Atmospheres, Terminator Lines, Atmospheric Scattering, Brightness, Optical Thickness, Zenith

Scientific paper

The approximate method of representing the intensity by a three-stream angular division is used to compute the brightness at the zenith near the terminator of an optically thin, spherically-symmetric planetary atmosphere illuminated by parallel solar radiation. The results are compared with those of Sobolev obtained under classical Eddington approximation

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