Design and Performance of V.H.F. receiving equipment for reception of extremely weak signals of solar and Galactic origin in the metre wavelength region

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/969

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DC Field	Value	Language
dc.contributor.author	Bhargava, B. N	-
dc.contributor.author	Jayarajan, A. P	-
dc.date.accessioned	2006-04-19T04:07:29Z	-
dc.date.available	2006-04-19T04:07:29Z	-
dc.date.issued	1960	-
dc.identifier.citation	Journal of the Institution of Telecommunication Engineers, Vol. 6, No. 5, pp. 231-238	en
dc.identifier.uri	http://hdl.handle.net/2248/969	-
dc.description.abstract	Three V.H.F receivers of high gain stability and low internal noise designed and constructed at the Kodaikanal Observatory are described. The receivers which operate at 1 1/2, 3 and 5 meter wavelengths are being used for the measurement of extra-terrestrial emission of solar and galactic origin and also for observations of radio-star scintillation. A report on the performance of one of the receivers over long periods together with details of aerial systems used and calibrating equipment is also given	en
dc.format.extent	1959508 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	IETE	en
dc.subject	VHF receiving equipment	en
dc.title	Design and Performance of V.H.F. receiving equipment for reception of extremely weak signals of solar and Galactic origin in the metre wavelength region	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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