Processing of radar observations 2: Determination of the meteoroid flux density

Details Processing of radar observations 2: Determination of the meteoroid flux density Processing of radar observations 2: Determination of the meteoroid flux density

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006prms.conf...38b&link_type=abstract

Proceedings of the Radio Meteor School, Oostmalle, Belgium, 10-14 September, 2005 Eds.: Verbeeck, C., Wislez, J.-M., Internation

Physics

1

Scientific paper

Two methods are described for determining the meteoroid flux density Q(m_0) of a meteor stream. In the first method, all observed stream meteors are considered, and the problem is solved by calculating the collecting area of a typical sector in the echo plane, reducing the flux density in this sector to mass m_0, and integrating over all directions in the echo plane. The second method uses the number of observed overdense meteors with an echo duration longer than 1 second.

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