Readhead, A. C. S. (1971) Interplanetary Scintillation of Radio Sources at Metre Wavelengths--II: Theory. Monthly Notices of the Royal Astronomical Society, 155 (2). pp. 185-197. ISSN 0035-8711. doi:10.1093/mnras/155.2.185. https://resolver.caltech.edu/CaltechAUTHORS:20200601-103015409
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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.
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| 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. | |||||||||
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| Issue or Number: | 2 | |||||||||
| DOI: | 10.1093/mnras/155.2.185 | |||||||||
| Record Number: | CaltechAUTHORS:20200601-103015409 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20200601-103015409 | |||||||||
| Official Citation: | A. C. S. Readhead, Interplanetary Scintillation of Radio Sources at Metre Wavelengths—II: Theory, Monthly Notices of the Royal Astronomical Society, Volume 155, Issue 2, December 1971, Pages 185–197, https://doi.org/10.1093/mnras/155.2.185 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 103596 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | George Porter | |||||||||
| Deposited On: | 01 Jun 2020 17:50 | |||||||||
| Last Modified: | 16 Nov 2021 18:23 |
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