Large-scale structure of the Perseid meteor swarm

Details Large-scale structure of the Perseid meteor swarm Large-scale structure of the Perseid meteor swarm

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985avest..18..249g&link_type=abstract

(Astronomicheskii Vestnik, vol. 18, July-Sept. 1984, p. 249-251) Solar System Research (ISSN 0038-0946), vol. 18, no. 3, Jan. 19

Astronomy and Astrophysics

Astronomy

Correlation Coefficients, Meteoroid Showers, Perseid Meteoroids, Temporal Distribution, Meteoritic Microstructures, Statistical Correlation

Scientific paper

The correlation coefficients between the observed numbers of meteors recorded concurrently by observing groups on a baseline of 2500-3000 km in 1980 and 1982 are calculated from a large base of statistical material including more than 1000 meteors. The results are compared with the same coefficients for 1951. It is concluded that large-scale formations in the swarm are encountered more frequently in recent years than in 1951.

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