Jovian atmosphere and total reflection

Details Jovian atmosphere and total reflection Jovian atmosphere and total reflection

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..821l&link_type=abstract

(Società Astronomica Italiana, Riunione, 21st, Bologna, Italy, Oct. 20-23, 1977.) Società Astronomica Italiana, Memorie, vol. 48

Physics

Optics

Atmospheric Density, Atmospheric Optics, Jupiter Atmosphere, Optical Reflection, Planetary Radiation, Stellar Occultation, Atmospheric Models, Incident Radiation, Light Transmission, Venus Atmosphere

Scientific paper

Link's theory of eclipse phenomena (1969) is used to develop a simple model for the density of the Jovian atmosphere. The model involves the numerical calculation of conditions under which a light ray, emitted from the Jovian solid surface, is subject to total reflection in the atmosphere. The present method may also have application to the Venusian atmosphere.

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