Fully Correcting for the Spread in Meteor Radiant Positions Due to Gravitational Attraction

Details Fully Correcting for the Spread in Meteor Radiant Positions Due to Gravitational Attraction Fully Correcting for the Spread in Meteor Radiant Positions Due to Gravitational Attraction

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001jimo...29..134g&link_type=abstract

WGN, Journal of the International Meteor Organization, vol. 29, no. 4, p. 134-138

Computer Science

Scientific paper

The zenith attraction formulae of Schiaparelli and Andreev do not fully account for the Earth's gravitational effects on meteor radiant estimation from the perspective of a single observer. This paper provides the necessary correction formulae to eliminate the gravitational component of radiant diffuseness seen in low-elevation, slow-encounter meteors.

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