A low-frequency radio spectropolarimeter for observations of the solar corona

dc.contributor.author	Kishore, P
dc.contributor.author	Ramesh, R
dc.contributor.author	Kathiravan, C
dc.contributor.author	Rajalingam, M
dc.date.accessioned	2020-11-17T13:55:28Z
dc.date.available	2020-11-17T13:55:28Z
dc.date.issued	2015-09
dc.identifier.citation	Solar Physics, Vol. 290, No. 9, pp. 2409-2422	en_US
dc.identifier.issn	0038-0938
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/7085
dc.description	Restricted Access © Springer The original publication is available at springerlink.com http://dx.doi.org/10.1007/s11207-015-0705-0	en_US
dc.description.abstract	A new spectropolarimeter for dedicated ground-based observations of radio emission from the solar corona at low frequencies (<100 MHz) has recently been commissioned at the Gauribidanur Radio Observatory near Bengaluru, India. We report the observational setup, the calibration scheme, and first results.	en_US
dc.language.iso	en	en_US
dc.publisher	Springer	en_US
dc.subject	Instrumentation and data management	en_US
dc.subject	Sun	en_US
dc.subject	Flares	en_US
dc.subject	Corona	en_US
dc.subject	Magnetic field	en_US
dc.subject	Polarized radio bursts	en_US
dc.title	A low-frequency radio spectropolarimeter for observations of the solar corona	en_US
dc.type	Article	en_US