The frequency agile solar radiotelescope

被引：19

作者：

Bastian, TS ^{[1
]}

机构：

[1] Natl Radio Astron Observ, Charlottesville, VA 22903 USA

来源：

ENERGY RELEASE AND PARTICLE ACCELERATION IN THE SOLAR ATMOSPHERE - FLARES AND RELATED PHENOMENA | 2003年 / 32卷 / 12期

关键词：

D O I：

10.1016/S0273-1177(03)00903-7

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The Frequency Agile Solar Radiotelescope (FASR), a telescope concept currently under study, will be a ground based solar-dedicated radio telescope designed and optimized to produce high resolution, high-fidelity, and high-dynamic-range images over a broad frequency range (similar to0.1-24 GHz). As such, FASR will address an extremely broad science program, including the nature and evolution of coronal magnetic fields, the physics of flares, drivers of space weather, and the quiet Sun. An important goal is to mainstream solar radio observations by providing a number of standard data products for use by the wider solar physics community. The instrument specifications and the key science elements that FASR will address are briefly discussed, as well as several operational issues. (C) 2003 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：2705 / 2714

页数：10

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