Diffusion of long-period meteor streams

Details Diffusion of long-period meteor streams Diffusion of long-period meteor streams

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992avest..26...58e&link_type=abstract

Astronomicheskii Vestnik: Issledovaniia Solnechnoi Sistemy (ISSN 0320-930X), vol. 26, no. 5, p. 58-66.

Astronomy and Astrophysics

Astronomy

3

Diffusion, Halley'S Comet, Meteoroid Showers, Orbit Perturbation, Orbital Elements, Statistical Analysis, Stochastic Processes

Scientific paper

The diffusion of long-period meteor streams is considered on the basis of mappings for the description of planetary perturbations. Formulas for the dispersion of orbital elements under the conditions of limiting stochasticity are obtained. A statistical study of the evolution of meteor streams in the orbits of the Comets Thatcher, P/Swift-Tuttle, P/Halley, and P/Tempel-Tuttle is carried out. It is shown that the dispersion of orbital elements exhibits complex behavior due to the random distribution of meteor particles in the resonant zones.

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