On the scattering of radio waves from underdense meteor trains

Details On the scattering of radio waves from underdense meteor trains On the scattering of radio waves from underdense meteor trains

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986baicz..37..189n&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 37, July 1986, p. 189-195.

Astronomy and Astrophysics

Astronomy

5

Electron Density (Concentration), Meteor Trails, Plasma-Electromagnetic Interaction, Radio Scattering, Diffusion Coefficient, Fresnel Diffraction

Scientific paper

The paper deals with some problems of radio-wave scattering from underdense meteor trains. The diffusion equation is solved under the assumption that the ionization source terminates its action after the meteor is fully burnt out, which has not been taken into account so far. The finite train initial radius is also considered. The formulas for the electron volume density obtained in this way are compared with those found by Dokuchaev (1960) and are further applied to the construction of the Fresnel characteristics. The model case is also considered, bearing in mind the possible presence of negative ions within the train.

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