On the use of an asymmetric model in the theory of radio echo from meteor trails

Details On the use of an asymmetric model in the theory of radio echo from meteor trails On the use of an asymmetric model in the theory of radio echo from meteor trails

Mar 1963

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1963jatp...25..151k&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 25, no. 3, pp. 151-161

Physics

Scientific paper

The scattering of short radio waves from an underdense meteor trail is considered in the context of the first-order echo theory. The essentially asymmetric nature of the trail formed in the earth's atmosphere is recognized and an attempt is made to assess its effects on observables such as the echo power, energy and duration. Tentative but specific results are derived for the case of specular scattering. These results permit the evaluation of the echo as a function of time; their dependence on the separation of the trail's terminus from the specular point and on the axial density distribution is discussed.

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