The calculation of meteor motion parameters based on the single station TV observations

Details The calculation of meteor motion parameters based on the single station TV observations The calculation of meteor motion parameters based on the single station TV observations

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010sosyr..44..327b&link_type=abstract

Solar System Research, Volume 44, Issue 4, pp.327-333

Mathematics

Scientific paper

Recently, television observations of meteors have steadily replaced photographic observations. Television recording with short exposures is a close analog of a photographic survey with a rotary shutter in the form of a system of set time marks on the meteor track. Each meteoric event is a series of recordings of separate phases of the motion of a meteor. This allows for the use of the geometric method for the determination of the motion parameters of meteors. In this work, a critique is given regarding the concept proposed by K.P. Stanyukovich in 1932-1939, and a mathematical justification of the geometric method of the analysis of the television images of meteors is given.

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