Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-27T14:05:05.286Z Has data issue: false hasContentIssue false
  • English
  • Français

Interplanetary Scintillation Studies at the Molonglo Radio Observatory

Published online by Cambridge University Press:  25 April 2016

R. G. Milne
R. G. Milne*
Affiliation:
Cornell-Sydney University Astronomy Centre, School of Physics, University of Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

The structure of small diameter radio sources can be investigated by studying the scintillation of the source due to the interplanetary medium when the line of sight approaches the Sun. Observations of radio source scintillation are currently being undertaken with the separate arms of the 1 mile radio telescope at the Molonglo Observatory. The EW arm allows successive transit observations with three fan beams, 1′.4 EW by 4°.2 NS at 408 MHz, bandwidth 2.5 MHz. Sources transit the half-power points of each beam in 6 sec δ seconds of time (δ is the source declination). The NS arm gives eleven fan beams at neighbouring declination, 1′.5 sec Z NS by 4° EW (Z is the zenith angle). Complete transit of a NS beam takes 15 sec δ minutes.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 2 , March 1972 , pp. 88 - 89
Copyright
Copyright © Astronomical Society of Australia 1972

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Mills, B. Y., Aitchison, R. E., Little, A. G. and McAdam, W. B., Proc. IRE (Aust.), 51, 156 (1963).Google Scholar
2 Young, A. T., Astrophys. J., 168, 543 (1971).CrossRefGoogle Scholar
3 Cohen, M. H., Gundermann, E. J., Hardebeck, H. E. and Sharp, L. E. Astrophys. J., 147, 449 (1967).CrossRefGoogle Scholar
4 Harris, D. E. and Hardebeck, E. G., Astrophys. Suppl. No. 170, 19, 115 (1969).CrossRefGoogle Scholar
5 Little, L. T. and Hewish, A., Mon. Not. R. astr. Soc, 138, 393 (1968).CrossRefGoogle Scholar
6 Anderson, B. and Donaldson, W., Mon. Not. R. astr. Soc, 137, 81 (1967).CrossRefGoogle Scholar