Resonance structure of meteoroid streams

Details Resonance structure of meteoroid streams Resonance structure of meteoroid streams

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.495...43e&link_type=abstract

In: Proceedings of the Meteoroids 2001 Conference, 6 - 10 August 2001, Kiruna, Sweden. Ed.: Barbara Warmbein. ESA SP-495, Noordw

Physics

6

Meteoroids

Scientific paper

The dynamical behaviour of meteoroid streams is studied on the basis of the resonance theory of perturbations. Parameters of principal resonance zones near orbits of the main meteoroid streams are given. It is shown that resonant particles may produce very concentrated meteoroid streams. The Leonid, Lyrid, Ursid and Bootid outbursts as indicators of the resonant motion are discussed. Recommendations are proposed for observations of resonanct structures.

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