A low-frequency (30-110 MHz) Antenna system for observations of polarized radio emission from the solar corona

dc.contributor.author	Ramesh, R
dc.contributor.author	Kathiravan, C
dc.contributor.author	Sundararajan, M. S
dc.contributor.author	Barve, Indrajit V
dc.contributor.author	Sastry, Ch. V
dc.date.accessioned	2008-12-15T14:21:03Z
dc.date.available	2008-12-15T14:21:03Z
dc.date.issued	2008-12
dc.identifier.citation	Solar Physics, Vol. 253, No. 1 - 2, pp. 319 - 327	en
dc.identifier.issn	0038-0938 (Print) 1573-093X (Online)
dc.identifier.uri	http://hdl.handle.net/2248/4061
dc.description	Restricted Access.	en
dc.description	The original publication is available at springerlink.com
dc.description.abstract	An interferometer antenna system to observe polarized radio emission from the solar corona at different frequencies in the range 30-110 MHz has been commissioned recently by the Indian Institute of Astrophysics at the Gauribidanur Radio Observatory (latitude 13°36'12''N and longitude 77°27'07''E), about 100 km north of Bangalore( http://www.iiap.res.in/centres_radio.htm ). This paper describes the antenna system, associated analog/digital receiver setup, calibration scheme, and preliminary results.	en
dc.language.iso	en	en
dc.publisher	Springer Netherlands	en
dc.relation.uri	http://www.springerlink.com/content/p33772pj73h60332/	en
dc.rights	© Springer	en
dc.subject	Magnetic Fields	en
dc.subject	Solar Corona	en
dc.subject	Radio Observations	en
dc.subject	Polarization	en
dc.title	A low-frequency (30-110 MHz) Antenna system for observations of polarized radio emission from the solar corona	en
dc.type	Article	en