Hostname: page-component-6bf8c574d5-9nwgx Total loading time: 0 Render date: 2025-02-22T02:21:44.344Z Has data issue: false hasContentIssue false
  • English
  • Français

Observations of venus at 8.6-mm wavelength

Published online by Cambridge University Press:  14 August 2015

J. E. Gibson  and
R. J. McEwan
J. E. Gibson
Affiliation:
Radio Astronomy Branch, U.S. Naval Research Laboratory Washington, D.C., U.S.A.
R. J. McEwan
Affiliation:
Radio Astronomy Branch, U.S. Naval Research Laboratory Washington, D.C., U.S.A.

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.

Mayer, McCullough, and Sloanaker [1] and Drake and Ewen [2] have measured centimeter wavelength radiation from several of the planets; the former at 3.15 and 9.4 cm, the latter at a wide bandwidth centered near 3.75 cm. The first measurements were the observations of Venus by Mayer et al., made near inferior conjunction in late spring 1956. These were obtained with a sufficiently favorable signal-to-noise ratio to permit direct recognition of Venus in individual diurnal-rate scans, and a brightness temperature of 560 ± 73°K (mean error) was deduced for the planet at inferior conjunction, i.e. for the dark side of Venus.

Type
Part I: Moon and Planets
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 50 - 52
Copyright
Copyright © Stanford University Press 1959 

References

1. Mayer, C. H., McCullough, T. P., and Sloanaker, R. M. Ap. J. 127, 1, 11, 1958.Google Scholar
2. Drake, F. D., and Ewen, H. I. Proc. I.R.E. 46, 53, 1958.Google Scholar
3. Gibson, J. E. U.S. Nav. Res. Lab. Report 4864, December 1956.Google Scholar