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Raman Scattering in the non-isothermal giant planet atmospheres

Published online by Cambridge University Press:  02 May 2006

Nadyia Kostogryz
Nadyia Kostogryz
Affiliation:
Main Astronomical Observatory of NAS of Ukraine email: kosn@mao.kiev.ua
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Abstract

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The influence of non-isothermal atmosphere on the intensity of details of Raman Scattering is computed for spectra of Uranus and Neptune. It follows that the intensity of this scattering depends on the depth of the level formation in an optically homogeneous non-isothermal atmosphere; neglecting of real temperature profiles during the analysis of observation data leads to large errors in the parameters of the atmosphere upper level.

Keywords

Raman ScatteringPlanetary nonisothermal atmosphere
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Colloquium C200: Direct Imaging of Exoplanets: Science & Techniques , October 2005 , pp. 181 - 184
Copyright
© 2006 International Astronomical Union