Elementary process and meteor train spectra

Details Elementary process and meteor train spectra Elementary process and meteor train spectra

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987maph...25...11o&link_type=abstract

In International Council of Scientific Unions, Middle Atmosphere Program. Handbook for MAP, Volume 25 p 11-21 (SEE N88-14502 06-

Astronomy and Astrophysics

Astrophysics

Atmospheric Ionization, Meteor Trails, Meteoroid Showers, Radiation Spectra, Astrophysics, Charge Exchange, Charged Particles, Earth Atmosphere, Ion Recombination, Line Spectra, Oxidation

Scientific paper

Mechanisms of excitation of individual spectral line radiation were studied experimentally and theoretically and it was demonstrated that such processes as oxidation, resonant charge exchange, dissociative recombination and others play an important part in the chemistry of excited particles. The foundation was laid toward simulating the elementary processes of meteor physics. Having a number of advantages and possibilities, this method is sure to find a wide use in the future.

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