Phase function in the scattering in arbitrary higher order

Details Phase function in the scattering in arbitrary higher order Phase function in the scattering in arbitrary higher order

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mesjj..60.1175s&link_type=abstract

Meteorological Society of Japan, Journal, vol. 60, Oct. 1982, p. 1175-1187.

Physics

Optics

Atmospheric Optics, Light Scattering, Planetary Atmospheres, Infrared Radiation, Mars Atmosphere, Transformations (Mathematics), Venus Atmosphere, Wavelengths

Scientific paper

A theory of higher order scattering of light by atmospheric particles is developed for a spherically stratified atmosphere. The phase function for scattering at higher-than-tertiary orders is defined, with consideration given to 12 wavelengths ranging from 3572-25,356 A. Calculations are presented for the intensity of n-th order scattering, and adaptations for a computer code are defined. The contributions of primary, secondary, and tertiary scattering of sunlight in the atmospheres of the earth, Mars, and Venus are calculated up to third order.

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