The estimation of the optical thicknesses of two-condensate cloud cover in the atmospheres of Jupiter and Saturn

Details The estimation of the optical thicknesses of two-condensate cloud cover in the atmospheres of Jupiter and Saturn The estimation of the optical thicknesses of two-condensate cloud cover in the atmospheres of Jupiter and Saturn

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987avest..21..189i&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 21, Apr.-June 1987, p. 189-191. In Russian.

Astronomy and Astrophysics

Astronomy

Cloud Cover, Jupiter Atmosphere, Light Scattering, Optical Thickness, Saturn Atmosphere

Scientific paper

The volumetric light scattering coefficients and optical thicknesses of the multilayer cloud structures of Jupiter and Saturn are determined. Khrgian-Mazin formulas for the description of the particle size distribution function are used. The optical thickness can be in the range of fractions of a unit to 1000 for Jupiter and several units to 1000 for Saturn.

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