Published December 1, 1971
| Published
Journal Article
Open
Interplanetary Scintillation of Radio Sources at Metre Wavelengths--II: Theory
- Creators
-
Readhead, A. C. S.
Abstract
Interplanetary scintillation is being used, in a survey of radio sources, to study angular structure in the range 0"·1-1" at a frequency of 81·5 MHz. The application of diffraction theory to scintillation at this frequency is discussed, and the diffracting parameters of the interplanetary medium are derived. The dependence of scintillation index on angular structure and receiver bandwidth is determined.
Additional Information
© 1971 Royal Astronomical Society. Provided by the NASA Astrophysics Data System. (Received 1971 July 23) I thank Dr A. Hewish for his help and encouragement, and for many useful discussions. I also thank my father, C. T. Readhead, for financial support during the early part of this work, and I gratefully acknowledge the support of an Isaac Newton Studentship received during the course of this work.Attached Files
Published - mnras155-0185.pdf
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Additional details
- Eprint ID
- 103596
- Resolver ID
- CaltechAUTHORS:20200601-103015409
- Cambridge University
- Created
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2020-06-01Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field