Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-29T11:26:52.959Z Has data issue: false hasContentIssue false
  • English
  • Français

8. Quadrantid Meteor Shower: Eleven Years of Radar Observations

Published online by Cambridge University Press:  12 April 2016

B. A. McIntosh

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In studying the evolution of meteor streams from cometary debris it is desirable to know the distribution of particles both around the orbit and in the cross section perpendicular to the orbit. Earth-based observations are limited to a once-per-year sample and also limited by the position of the observer on earth as it crosses the meteor stream. A continuous series, 11 years, of records of the Quadrantid meteor shower illustrates the problems and the results that can be achieved. International cooperation would greatly assist such studies.

Type
Part III. Meteors and Meteoroids
Information
International Astronomical Union Colloquium , Volume 39: Comets, Asteroids, Meteorites: Interrelations, Evolution and Origins , December 1977 , pp. 171 - 174
Copyright
Copyright © A.H. Delsemme 1977

References

Belkovich, D. I., and Tohktasev, V. S. 1974, Bull. Astron. Inst. Czech., 25, 370.Google Scholar
Hajduk, A., McIntosh, B. A., and Simek, M. 1974, Bull. Astron. Inst. Czech., 25, 305.Google Scholar
Hindley, K. B. 1972, Sky and Telescope, 44, 162.Google Scholar
McIntosh, B. A. 1966, Can. J. Phys., 44, 2729.Google Scholar
McIntosh, B. A. 1971, Bull. Astron. Inst. Czech., 25, 362.Google Scholar
Poole, L.M.G., Hughes, D. W., and Kaiser, T. R. 1972, Mon. Not. R. Astr. Soc., 156, 223.Google Scholar