Some features of formation of details of raman scattering in a non-isothermal atmosphere

Details Some features of formation of details of raman scattering in a non-isothermal atmosphere Some features of formation of details of raman scattering in a non-isothermal atmosphere

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005kfnt...21..114m&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 21, no. 2, p. 114-120

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Scientific paper

The influence of non-isothermal atmosphere on the intensity of details of the Raman scattering is computed for a spectrum of Neptune. The following inferences are made: the intensity of this scattering depends on the depth of the level of its formation in an optical homogeneous non-isothermal atmosphere; neglect of real temperature profiles during the analysis of observation data leads to large errors in the parameters of the atmosphere upper levels.

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