Nonisothermicity of meteor trails

Details Nonisothermicity of meteor trails Nonisothermicity of meteor trails

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976avest...9..232d&link_type=abstract

(Astronomicheskii Vestnik, vol. 9, Oct.-Dec. 1975, p. 232-236.) Solar System Research, vol. 9, no. 4, Apr. 1976, p. 191-194. Tra

Physics

Fresnel Region, Meteor Trails, Meteoroid Concentration, Radio Meteors, Atmospheric Physics, Diffusion Coefficient, Radio Echoes, Radio Probing, Time Dependence, Upper Atmosphere

Scientific paper

On the basis of experimental data it has been shown that the diffusion coefficient of meteoric trail D changes considerably during the existence of radio-echo recorded from an unsaturated meteoric trail. A law of the change of value D in time has been established. It has been shown that the decrease of D ceases approximately in 0.17 sec after the formation of the first Fresnel zone.

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