The Gauribidanur Radioheliograph

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3266

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DC Field	Value	Language
dc.contributor.author	Ramesh, R	-
dc.contributor.author	Subramanian, K. R	-
dc.contributor.author	Sundararajan, M. S	-
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2008-08-25T04:26:47Z	-
dc.date.available	2008-08-25T04:26:47Z	-
dc.date.issued	1998-08	-
dc.identifier.citation	Solar Physics, Vol. 181, No. 2, pp. 439 - 453	en
dc.identifier.issn	0038 - 0938	-
dc.identifier.uri	http://hdl.handle.net/2248/3266	-
dc.description	Restricted Access	en
dc.description.abstract	A new radio heliograph for obtaining two-dimensional images of the solar corona sequentially at many frequencies in the range 40-150 MHz has been built by the Indian Institute of Astrophysics at the Gauribidanur Radio Observatory (lat. 13 deg36'12'' N and long. 77 deg27'07'' E) about 100 km north of Bangalore, India. This paper describes various aspects of the antenna system, receiver front end, digital hardware, the data acquisition and the calibration procedure. The performance of the instrument is illustrated with maps of the continuum emission from the undisturbed corona at different frequencies.	en
dc.format.extent	368609 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://dx.doi.org/10.1023/A:1005075003370	en
dc.subject	Radio Heliograph	en
dc.subject	Solar Corona	en
dc.title	The Gauribidanur Radioheliograph	en
dc.type	Article	en
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