Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-29T08:16:55.223Z Has data issue: false hasContentIssue false
  • English
  • Français

Protection of Omniwavelength Radio Astronomy and Preventing Radio Pollution of Space

Published online by Cambridge University Press:  12 April 2016

B. A. Doubinsky
B. A. Doubinsky*
Affiliation:
Institute of Radio Engineering and Electronics, Academy of Sciences, Moscow, USSR

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.

Radio pollution of space is connected with general ecological conditions resulting from world development. A practical aspect of the problem is related to the possibility of making radioastronomy observations of cosmic emissions and searching for signals from extraterrestrial civilizations over almost all of the entire radio spectrum. For this purpose, it was decided at WACR-79 to keep a quiet zone on the shielded side of the moon. Here we shall discuss the problem as it relates to an observatory in orbit. The vicinity of the L2 Lagrangian point of the earth-sun system is of particular interest as a location for such an observatory.

Type
Radio Frequency Interference
Information
International Astronomical Union Colloquium , Volume 112: Light Pollution, Radio Interference, and Space Debris , 1991 , pp. 305 - 309
Copyright
Copyright © Astronomical Society of the Pacific 1991

References

[1] Boyarchuck, L. A., Kardashev, N. S., and Yatskiv, Y. S., “An Orbiting Super-Observatory Before the Year 2000?,” Report to 20th General Assembly of the IAU, reported in “IAU Today,” Baltimore, MD, August 10,1988.Google Scholar
[2] ITU. Radio Regulations, 1982. Article 28, Sec. 4.Google Scholar
[3] Recommendations and Reports of the CCIR, 1986, v. 4, part. 1.Google Scholar