The Spatial Distribution of Potential Forward Scatter Reflection Points

Details The Spatial Distribution of Potential Forward Scatter Reflection Points The Spatial Distribution of Potential Forward Scatter Reflection Points

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995jimo...23..236v&link_type=abstract

WGN, Journal of the International Meteor Organization, vol. 23, no. 6, p. 236-243

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Scientific paper

A forward scatter set-up can only detect those meteors which lie above the Earth's tangent planes (i.e., horizon) in transmitter and receiver. For other meteors, the transmitted signal will not reach the meteor or the reflected signal will not reach the receiver. The present paper determines the explicit shape of the potential reflection zone of points satisfying the above condition, as well theoretically as in some numeric instances.

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