Dynamics and dimensions of short-period meteoroid streams - Interrelations between meteor showers

Details Dynamics and dimensions of short-period meteoroid streams - Interrelations between meteor showers Dynamics and dimensions of short-period meteoroid streams - Interrelations between meteor showers

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68.1074b&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, Sept.-Oct. 1991, p. 1074-1085. In Russian.

Astronomy and Astrophysics

Astronomy

1

Meteoroid Showers, Orbit Perturbation, Orbital Elements, Eccentricity, Secular Variations, Solar Orbits

Scientific paper

The dynamics and dimensions of 22 short-period meteoroid streams are investigated. It is found that, at the early stage of evolution, meteoroid streams may be considered elliptical rings of relatively small thickness. The effect of planetary perturbations can essentially increase the stream width and thickness. As a result, one stream may produce several pairs of meteor showers that are active in different seasons. The meteoroid streams under review may theoretically produce 102 meteor showers. The existence of 72 showers is confirmed by photographic and radar observations.

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