Calculation of the incident flux density of meteors by numerical integration: Improved geometrical approach

Details Calculation of the incident flux density of meteors by numerical integration: Improved geometrical approach Calculation of the incident flux density of meteors by numerical integration: Improved geometrical approach

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jastp..73..901v&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 73, Issue 9, p. 901-903.

Physics

Scientific paper

As meteoroid flux density is an objective parameter which measures meteoroid abundance in the vicinity of the Earth's orbit, accurate determination of this parameter by radar and other observations is essential in order to compare results of radars in a network. A numerical technique for calculation of the incident meteoroid flux density from specular radar and forward scatter observations of meteor trails was published in Ryabova (2008, 2009). The present paper modifies this numerical method to remove the lower mass limit mismatch effect and features a more accurate geometrical representation.

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