Please use this identifier to cite or link to this item:
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
ISSN: 1573-093X
???metadata.dc.rights???: © The Author(s) 2014. This article is published with open access at
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Gauribidanur low-frequency solar spectrograph.pdfOpen Access1.1 MBAdobe PDFView/Open

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.