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On the spatial structure of the Perseids meteor streamThe 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.
Document ID
19880005168
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Andreev, G. V. (Academy of Sciences of the Tajik SSR Doushanbe, Tajikistan)
Rubtsov, L. N. (Academy of Sciences of the Tajik SSR Doushanbe, Tajikistan)
Tarasova, I. I. (Academy of Sciences of the Tajik SSR Doushanbe, Tajikistan)
Date Acquired
September 5, 2013
Publication Date
August 1, 1987
Publication Information
Publication: International Council of Scientific Unions, Middle Atmosphere Program. Handbook for MAP, Volume 25
Subject Category
Astrophysics
Accession Number
88N14550
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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