Gauribidanur Low-Frequency Solar Spectrograph

被引：35
作者：
Kishore, P. [1 ]
Kathiravan, C. [1 ]
Ramesh, R. [1 ]
Rajalingam, M. [1 ]
Barve, Indrajit V. [1 ]
机构：
[1] Indian Inst Astrophys, Bangalore 560034, Karnataka, India
来源：
SOLAR PHYSICS | 2014年 / 289卷 / 10期
关键词：
Instrumentation and data management; Radio bursts; dynamic spectrum; association with flares; Magnetic fields; corona; PERIODIC RADIO-EMISSION; CORONAL MASS EJECTIONS; ENERGY RELEASES; II BURSTS; BAND; ASSOCIATION; ARRAY; MICROBURSTS; PARAMETERS; TRANSIENT;
D O I：
10.1007/s11207-014-0539-1
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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 approximate to 40-440 MHz. Radio emission in this frequency range originates close to the Sun, typically in the radial distance range r approximate to 1.1-2.0 R-circle dot. This article describes the characteristics of the GLOSS and the first results.
引用
收藏
页码：3995 / 4005
页数：11
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