Calculating the meteoroid flux density of a meteor shower from radio forward scatter observations

Details Calculating the meteoroid flux density of a meteor shower from radio forward scatter observations Calculating the meteoroid flux density of a meteor shower from radio forward scatter observations

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007pimo.conf..162s&link_type=abstract

Proceedings of the International Meteor Conference, Roden, The Netherlands, 14-17 September, 2006 Eds.: Bettonvil, F., Kac, J. I

Physics

Scientific paper

A practical method is presented for calculating the meteoroid flux density Q(mo) of a meteor shower based on echo count s from a forward scatter set-up. The current paper aims at providing a ready-to use method, while more physical explanations can be found in the Radio Meteor School lectures by Oleg Belkovich (Verbeeck & Wislez, 2006). This method was already used to process real data from Perseid observations (Belkovich & Suleymanova, 1999).

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