Gauribidanur low-frequency solar spectrograph

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6619

Title:	Gauribidanur low-frequency solar spectrograph
Authors:	Kishore, P Kathiravan, C Ramesh, R Rajalingam, M Barve, Indrajit V
Keywords:	Instrumentation and Data Management Radio Bursts, Dynamic Spectrum Radio Bursts, Association with Flares Magnetic Fields, Corona
Issue Date:	Oct-2014
Publisher:	Springer
Citation:	Solar Physics, Vol. 289, No. 10, pp. 3995-4005
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
Description:	Open Access The original publication is available at springerlink.com
URI:	http://hdl.handle.net/2248/6619
ISSN:	1573-093X
Appears in Collections:	IIAP Publications

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