On a fine structure of the Perseid meteoroid stream. Method of indices

Details On a fine structure of the Perseid meteoroid stream. Method of indices On a fine structure of the Perseid meteoroid stream. Method of indices

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.495..105s&link_type=abstract

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

Statistics

3

Meteoroid Streams, Fine Structures

Scientific paper

A fine structure of the Perseids is studied using a method of indices. The procedure, based only on mathematical statistics, is now used to study of a fine structure of the Perseid stream and its filaments which cannot be separated reliably by iteration methods. Besides the five orbital elements incorporated in the Southworth-Hawkins D-criterion, we have also included in the procedure the coordinates of the radiant which are one of the most accurately known parameter characteristic for physically related orbits. 351 (approx. 67%) of 522 Perseids taken into account were assigned to one of 11 chosen filaments of orbits.

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