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13. Atmospheric heights of telescopic meteors

Published online by Cambridge University Press:  14 August 2015

L. Kohoutek
L. Kohoutek*
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Prague

Extract

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The heights of sporadic telescopic meteors were observed from three stations, distant from each other 9·1, 6·0 and 3·2 km respectively, during the meteor expedition in the summer of 1960 (Kohoutek, 1967). Three teams of four observers gathered individually data on 1187 meteors, together with 1864 drawings, during the period of 7 nights, August 15–27. Altogether, 189 pairs observed by at least two stations were identified from the complete material. The heights of the respective beginning (b), centre (c) or end (e) points of 159 pairs were determined by means of graphic-numerical analysis.

Type
Session 2
Information
Symposium - International Astronomical Union , Volume 33: Physics and Dynamics of Meteors , 1968 , pp. 143 - 146
Copyright
Copyright © Reidel 1968 

References

Ceplecha, Z. (1966) Bull. astr. Inst. Csl., 17, 347.Google Scholar
Ceplecha, Z., Padevět, V. (1961) Bull. astr. Inst. Csl., 12, 191.Google Scholar
Hawkins, G.S., Southworth, R.B. (1958) Smithson. Contr. Astrophys., 2, 349.Google Scholar
Jacchia, L.G., Verniani, F., Briggs, R.E. (1965) Smithson. Contr. Astrophys., 10, 1.Google Scholar
Kohoutek, L. (1967) Bull. astr. Inst. Csl., 18, 171.Google Scholar
Kohoutek, L., Grygar, J. (1962) Bull. astr. Inst. Csl., 13, 9.Google Scholar
Öpik, E.J. (1958) Physics of Meteor Flight in the Atmosphere, Interscience Publishers, New York, Appendix 1–2.Google Scholar