Meteor Trajectory from Multiple Station Head Echo Doppler Observations

Details Meteor Trajectory from Multiple Station Head Echo Doppler Observations Meteor Trajectory from Multiple Station Head Echo Doppler Observations

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jimo...38..123s&link_type=abstract

WGN, Journal of the International Meteor Organization, vol. 38, no. 4, p. 123-129

Statistics

Methodology

Scientific paper

An improved method for determining a meteor's trajectory from its head echo Doppler signature is presented. This methodology is derived from pioneering work from over half a century ago. The new analytical technique employs head echo data that was simultaneously captured by multiple receiving stations located around a low power beacon. In addition to the geometrical data, Monte Carlo simulations of timing errors were generated and reviewed. The method shows great potential, especially if tighter constraints in the inter-station timing can be achieved.

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