Gauribidanur low-frequency solar spectrograph

Kishore, P; Kathiravan, C; Ramesh, R; Rajalingam, M; Barve, Indrajit V

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dc.contributor.author	Kishore, P
dc.contributor.author	Kathiravan, C
dc.contributor.author	Ramesh, R
dc.contributor.author	Rajalingam, M
dc.contributor.author	Barve, Indrajit V
dc.date.accessioned	2014-06-06T14:56:10Z
dc.date.available	2014-06-06T14:56:10Z
dc.date.issued	2014-10
dc.identifier.citation	Solar Physics, Vol. 289, No. 10, pp. 3995-4005	en
dc.identifier.issn	1573-093X
dc.identifier.uri	http://hdl.handle.net/2248/6619
dc.description	Open Access	en
dc.description	The original publication is available at springerlink.com
dc.description.abstract	A 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 results	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://dx.doi.org/10.1007/s11207-014-0539-1	en
dc.rights	© The Author(s) 2014. This article is published with open access at Springerlink.com	en
dc.subject	Instrumentation and Data Management	en
dc.subject	Radio Bursts, Dynamic Spectrum	en
dc.subject	Radio Bursts, Association with Flares	en
dc.subject	Magnetic Fields, Corona	en
dc.title	Gauribidanur low-frequency solar spectrograph	en
dc.type	Article	en