The behavior of the meteoric O I 5577 A emission

Details The behavior of the meteoric O I 5577 A emission The behavior of the meteoric O I 5577 A emission

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977cajph..55.1379b&link_type=abstract

Canadian Journal of Physics, vol. 55, Aug. 1, 1977, p. 1379-1383.

Physics

Atomic Excitations, Forbidden Transitions, Light Emission, Meteor Trails, Oxygen Ions, Plasma Radiation, Abundance, Atmospheric Ionization, Ion Concentration, Ionic Collisions, Mathematical Models

Scientific paper

A better understanding of the mechanisms important in the production of the forbidden O I green line feature in meteor wakes may result from a theoretical approach to the relevant dynamic and reaction processes in a plasma column. A model is developed in which the rates of excitation and removal of metastable atoms permit a description of the resulting 5577 A emission.

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