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Two Station Television Meteor Studies

Published online by Cambridge University Press:  14 August 2015

R. L. Hawkes  and
J. Jones
R. L. Hawkes
Affiliation:
Department of Physics, The University of Western Ontario, London, Canada N6A 3K7
J. Jones
Affiliation:
Department of Physics, The University of Western Ontario, London, Canada N6A 3K7

Extract

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Single station studies cannot provide detailed information such as zenith angle, velocity, heights and magnitude for individual meteors and Ceplecha (1976) has stressed the need for two station television observations which could provide such information through triangulation analyses. This paper deals with some of the results of the first two station television intensifier study of faint meteors, and the implications of these results concerning the validity of the current theories of the structure and ablation of dustball meteors.

Type
II: Meteors and Meteorites
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 117 - 120
Copyright
Copyright © Reidel 1980 

References

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