Raman effects in the atmospheres of the major planets

Details Raman effects in the atmospheres of the major planets Raman effects in the atmospheres of the major planets

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..10e..37k&link_type=abstract

Progress in Planetary Exploration Missions, 26th meeting of the IAU, Joint Discussion 10, 21-22 August 2006, Prague, Czech Repub

Computer Science

Scientific paper

The results of research for high-resolution spectra of solar system major planet atmospheres in visible range are presented in this paper. Investigations are realized taking into account Raman light scattering by H[2]. Approximate calculations of the reflected intensities of the various frequency-shifted Raman components by observation data are presented. Spectral brightness factors of cloudy surface regions for Jupiter and Saturn and geometric albedos for Uranus and Neptune discs are calculated. There are obtaned their veritable significances after subtract of Raman scattering. There are rated some optical parameters of major planet atmospheres describing vertical structure of atmospheres with using intensities of Raman components.

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