Theoretical studies of important processes in planetary and comet atmospheres. Renewel request

Details Theoretical studies of important processes in planetary and comet atmospheres. Renewel request Theoretical studies of important processes in planetary and comet atmospheres. Renewel request

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989isrl.rept.....g&link_type=abstract

Progress Report, 1 Sep. 1989 - 31 Oct. 1990 Institute for Scientific Research, Lexington, MA.

Physics

Atmospheric Models, Cometary Atmospheres, Gas Dissociation, Oxygen, Planetary Ionospheres, Recombination Reactions, Atomic Structure, Electron Energy, Kinetic Energy, Molecular Excitation, Quantum Chemistry, Vibration

Scientific paper

Current efforts have focused on the dissociative recombination (DR) of O2(+), a process of great importance in planetary atmospheres. This process is difficult to study experimentally because of the need to determine the dependence of the product electronic states and kinetic energies upon the vibrational distribution of the ion and electron temperature. The knowledge of these characteristics of DR is needed to accurately model planetary ionospheres. Using a theoretical quantum chemical approach, the generation of O(1S) from DR was studied in detail.

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