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1.2.4 Scattering Layer of Cosmic Dust in the Upper Atmosphere

Published online by Cambridge University Press:  12 April 2016

François Link
François Link*
Affiliation:
Institut d’Astrophysique, 75014 Paris, France

Extract

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The upper atmosphere acts as a giant collector of cosmic dust swept by the Earth on its travel through space. The transient presence of cosmic dust in the upper atmosphere was detected by the rise of the luminance of the twilight sky during the activity of several meteoric showers either by balloon photometers launched by C.N.E.S. at Aire sur l’Adour (Fehrenbach et al., 1972 a) or by the similar photometer at the Pic du Midi Observatory (Link, 1973).

Type
1 Zodiacal Light
Information
International Astronomical Union Colloquium , Volume 31: Interplanetary Dust and Zodiacal Light , 1976 , pp. 107 - 111
Copyright
Copyright © Springer-Verlag 1976

References

Fehrenbach, M., Frimout, D., Link, F. and Lippens, C. 1972a, Ann. Géophys. 28, 363 Google Scholar
Fehrenbach, M., Frimout, D., Link, F., Lippens, C. and Weill, G. 1972b, Compt. Rendus. Acad. Sci. Paris B-275, 223.Google Scholar
Fehrenbach, M. and Link, F. 1974, Compt. Rend. Acad. Sci. Paris B-279, 687 Google Scholar
Giese, R.H. 1970, Max Planck Inst. PAE/Extraterr. 70, München Google Scholar
Link, F. 1950, Bull. Astron. Inst. Czechoslov. 2, 1 Google Scholar
Link, F. 1973, Space Research XIV, 703 Google Scholar
Link, F. and Weill, G. submitted for publication to Geophys. Ann. Google Scholar