Radiation characteristics of nonequilibrium meteor plasma

Details Radiation characteristics of nonequilibrium meteor plasma Radiation characteristics of nonequilibrium meteor plasma

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979avest..12..199k&link_type=abstract

(Astronomicheskii Vestnik, vol. 12, Oct.-Dec. 1978, p. 199-205.) Solar System Research, vol. 12, no. 4, Apr. 1979, p. 167-173. T

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Atomic Excitations, Electron Transitions, Meteor Trails, Nonequilibrium Plasmas, Plasma Radiation, Chemical Elements, Deactivation, Inelastic Collisions, Transition Probabilities

Scientific paper

A method of classical analysis of meteor radiation is presented taking into account nonradiative transitions from the excitation levels of the meteor plasma. It is shown that deactivation and reactivation of the excited levels of the meteor atoms induced by inelastic collisions of the second type are characterized by the corresponding changes of the relative intensities of lines along the meteor path.

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