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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6619
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dc.contributor.authorKishore, P-
dc.contributor.authorKathiravan, C-
dc.contributor.authorRamesh, R-
dc.contributor.authorRajalingam, M-
dc.contributor.authorBarve, Indrajit V-
dc.date.accessioned2014-06-06T14:56:10Z-
dc.date.available2014-06-06T14:56:10Z-
dc.date.issued2014-10-
dc.identifier.citationSolar Physics, Vol. 289, No. 10, pp. 3995-4005en
dc.identifier.issn1573-093X-
dc.identifier.urihttp://hdl.handle.net/2248/6619-
dc.descriptionOpen Accessen
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractA new radio spectrograph, dedicated to observe the Sun, has been recently commissioned by the Indian Institute of Astrophysics (IIA) at the Gauribidanur Radio Observatory, about 100 km North of Bangalore. The instrument, called the Gauribidanur Low-frequency Solar Spectrograph (GLOSS), operates in the frequency range≈40 – 440 MHz. Radio emission in this frequency range originates close to the Sun, typically in the radial distance range r≈1.1 – 2.0 R⊙. This article describes the characteristics of the GLOSS and the first resultsen
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://dx.doi.org/10.1007/s11207-014-0539-1en
dc.rights© The Author(s) 2014. This article is published with open access at Springerlink.comen
dc.subjectInstrumentation and Data Managementen
dc.subjectRadio Bursts, Dynamic Spectrumen
dc.subjectRadio Bursts, Association with Flaresen
dc.subjectMagnetic Fields, Coronaen
dc.titleGauribidanur low-frequency solar spectrographen
dc.typeArticleen
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