Interplanetary Scintillation and its Relation to the Angular Structure of Radio Sources
Open Access
- 1 December 1966
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 134 (3) , 221-237
- https://doi.org/10.1093/mnras/134.3.221
Abstract
The recent discovery of interplanetary scintillation has provided a new technique for deriving inforrnation about the angular structure of radio sources in the range 0″.1−1″. A full account is given of the theory of the method and its practical application. The possibilities of the technique are illustrated by some typical observations at a frequency of 178 Mc/s.Keywords
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