Hostname: page-component-7bb8b95d7b-cx56b Total loading time: 0 Render date: 2024-09-17T23:20:43.433Z Has data issue: false hasContentIssue false
  • English
  • Français

77. Possible proofs of the lunar atmosphere

Published online by Cambridge University Press:  14 August 2015

F. Link
F. Link*
Affiliation:
Astronomical Institute of the Academy of Sciences, Prague, Czechoslovakia

Extract

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 the period 1955–57 a number of occultations of two radio sources 05·01 Taurus and 06·01 Gemini by the Moon takes place [1]. They will give an excellent opportunity to examine not only the exact position and the shape of these sources but possibly also some traces of the lunar atmosphere [2].

Type
Part VI: Meteors and Planets
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 400 - 402
Copyright
Copyright © Cambridge University Press 1957 

References

1. Link, F. and Neužil, L. B.A.C. 5, 112, 1954.Google Scholar
2. Link, F. B.A.C. 7, 1, 1956.Google Scholar
3. Dollfus, A. C.R. Paris , 234, 2046, 1952.Google Scholar
4. Berning, W. W. J. Meteorol. 8, 175, 1951.Google Scholar