Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-25T15:48:41.703Z Has data issue: false hasContentIssue false
  • English
  • Français

18. Current progress in development and results obtained with the ‘Mills Cross’ at the Radiophysics Laboratory

Published online by Cambridge University Press:  14 August 2015

J. L. Pawsey
J. L. Pawsey*
Affiliation:
Division of Radiophysics, Commonwealth Scientific and Industrial Research Organization, Sydney, Australia

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.

The study of continuous spectrum cosmic radio waves in the Radiophysics Laboratory is based mainly on two large ‘Mills Crosses’: one on 85 Mc./s. which has been in use for a year, and another on 20 Mc./s. which is under construction. The principle of this instrument has been described by Mills and Little (1953) [1]. It utilizes two long thin arrays arranged in the form of a cross and gives an effective ‘pencil-beam’ response which records both the background and discrete sources simultaneously. Essential data relating to these Crosses are given in Table 1.

Type
Part II: Point Sources: Individual Study and Physical Theory
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 123 - 131
Copyright
Copyright © Cambridge University Press 1957 

References

1. Mills, B. Y. and Little, A. G. Aust. J. Phys. 6, 272, 1953.Google Scholar
2. Mills, B. Y. Aust. J. Phys. 8, 368, 1955.CrossRefGoogle Scholar
3. Shklovsky, I. S. U.S.S.R. Acad. Sc. Ast. J. 29, 418, 1952.Google Scholar
Shklovsky, I. S. U.S.S.R. Acad. Sc. Ast. J. 30, 15, 1953.Google Scholar
4. Hanbury Brown, R. and Hazard, C. Phil. Mag. 43, 137, 1952.Google Scholar
5. Hanbury Brown, R. and Hazard, C. M.N.R.A.S. 113, 123, 1953.Google Scholar