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On Time-dependent Models of the Meteoric Background Complex

Published online by Cambridge University Press:  14 August 2015

Ján Štohl
Ján Štohl*
Affiliation:
Astronomical Institute, Slovak Academy of Sciences, Bratislava, Czechoslovakia

Abstract

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Continuous models of the meteoric background complex are discussed and analysed on the basis of observational data on radiants and hourly rates of sporadic meteors. A time-dependent, bi-elliptical model of the true radiant distribution fits the observational results.

Type
II: Meteors and Meteorites
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 141 - 144
Copyright
Copyright © Reidel 1980 

References

Lazarev, R.G.: 1965, Astron. Zhurnal 42, pp. 1075–1083.Google Scholar
Sekanina, Z.: 1973, Icarus 18, pp. 253–284.CrossRefGoogle Scholar
Stohl, J.: 1975, Acta F.R.N. Univ. Comen.-Astronomia et Geophysica 1, pp. 17–25.Google Scholar
Tkachuk, A.A.: 1978, Meteornye issledovaniya No. 5, pp. 67–73.Google Scholar