Radiation intensity in meteor spectra

Details Radiation intensity in meteor spectra Radiation intensity in meteor spectra

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992avest..26..116s&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 26, no. 2, Mar.-Apr. 1992, p. 116-120. In Russian.

Astronomy and Astrophysics

Astronomy

Earth Atmosphere, Meteor Trails, Plasma Interactions, Radiation Spectra, Space Plasmas, Spectral Energy Distribution, Kinetic Equations, Line Spectra, Plasma Spectra, Stony Meteorites

Scientific paper

Various mechanisms responsible for spectral-line radiation in meteor spectra are considered. Theoretical intensities of the meteor spectral lines are compared with experimental intensity values. The effect of different external physical conditions on the radiation in the meteor spectrum formation process is evaluated. The solution of the kinetic equation as applied to the problem of the dispersion of a meteor plasma cluster is considered.

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