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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7085
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dc.contributor.authorKishore, P-
dc.contributor.authorRamesh, R-
dc.contributor.authorKathiravan, C-
dc.contributor.authorRajalingam, M-
dc.date.accessioned2020-11-17T13:55:28Z-
dc.date.available2020-11-17T13:55:28Z-
dc.date.issued2015-09-
dc.identifier.citationSolar Physics, Vol. 290, No. 9, pp. 2409-2422en_US
dc.identifier.issn0038-0938-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7085-
dc.descriptionRestricted Access © Springer The original publication is available at springerlink.com http://dx.doi.org/10.1007/s11207-015-0705-0en_US
dc.description.abstractA 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.isoenen_US
dc.publisherSpringeren_US
dc.subjectInstrumentation and data managementen_US
dc.subjectSunen_US
dc.subjectFlaresen_US
dc.subjectCoronaen_US
dc.subjectMagnetic fielden_US
dc.subjectPolarized radio burstsen_US
dc.titleA low-frequency radio spectropolarimeter for observations of the solar coronaen_US
dc.typeArticleen_US
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