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

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

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jimo...37...63r&link_type=abstract

WGN, Journal of the International Meteor Organization, vol. 37, no. 2, p. 63-67

Physics

2

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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