The calculation of TV, VT, VV, VV' − rate coefficients for the collisions of the main atmospheric components

The first-order perturbation approximation is applied to calculate the rate coefficients of vibrational energy transfer in collisions involving vibrationally excited molecules in the absence of non-adiabatic transitions. The factors of molecular attraction, oscillator frequency change, anharmoni...

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Bibliographic Details
Main Author: A. S. Kirillov
Format: Article
Language:English
Published: Copernicus Publications 1998-07-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/16/838/1998/angeo-16-838-1998.pdf
Description
Summary:The first-order perturbation approximation is applied to calculate the rate coefficients of vibrational energy transfer in collisions involving vibrationally excited molecules in the absence of non-adiabatic transitions. The factors of molecular attraction, oscillator frequency change, anharmonicity, 3-dimensionality and quasiclassical motion have been taken into account in the approximation. The analytical expressions presented have been normalized on experimental data of VT-relaxation times in N<sub>2</sub> and O<sub>2</sub> to obtain the steric factors and the extent of repulsive exchange potentials in collisions N<sub>2</sub>-N<sub>2</sub> and O<sub>2</sub>-O<sub>2</sub>. The approach was applied to calculate the rate coefficients of vibrational-vibrational energy transfer in the collisions N<sub>2</sub>-N<sub>2</sub>, O<sub>2</sub>-O<sub>2</sub> and N<sub>2</sub>-O<sub>2</sub>. It is shown that there is good agreement between our calculations and experimental data for all cases of energy transfer considered.<br><br><b>Key words.</b> Ionosphere (Auroral ionosphere; ion chemistry and composition). Atmospheric composition and structure (Aciglow and aurora).</p>
ISSN:0992-7689
1432-0576