Calculation of the incident flux density of meteors by numerical integration I

Details Calculation of the incident flux density of meteors by numerical integration I Calculation of the incident flux density of meteors by numerical integration I

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jimo...36..120r&link_type=abstract

WGN, Journal of the International Meteor Organization, vol. 36, no. 6, p. 120-123

Physics

3

Scientific paper

A method for calculation of the flux density of meteors from backscatter
radar observations is proposed. The method is a modification of the
Kaiser-Belkovich method, aimed at performing direct numerical
calculations instead of approximations. It allows one to work with
physical models of a user's choice.

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