Interplanetary Scintillation and its Relation to the Angular Structure of Radio Sources

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 ill...

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Published in:Monthly notices of the Royal Astronomical Society 1966-12, Vol.134 (3), p.221-237
Main Authors: Little, L. T., Hezmsh, A.
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Language:English
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container_title Monthly notices of the Royal Astronomical Society
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Hezmsh, A.
description 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.
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title Interplanetary Scintillation and its Relation to the Angular Structure of Radio Sources
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