On the spatial structure of the Perseids meteor stream

Details On the spatial structure of the Perseids meteor stream On the spatial structure of the Perseids meteor stream

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987maph...25..339a&link_type=abstract

In International Council of Scientific Unions, Middle Atmosphere Program. Handbook for MAP, Volume 25 p 339-343 (SEE N88-14502 0

Physics

Meteoroid Showers, Particle Emission, Particle Mass, Perseid Meteoroids, Spatial Distribution, Flux Density, Radar Tracking, Regression Analysis, Solar Longitude

Scientific paper

The analysis of radar observations of the Perseid meteor stream conducted in an ionospherical laboratory in the period from 1964 to 1981 is presented. The Perseids meteor rates were determined by the fluctuation method. Analysis of their hourly distributions showed that the stream maximum position is different for different years, i.e., the stream nodal position is constantly changing. The results of the analysis are presented and discussed.

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