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First radio burst imaging observation from Mingantu Ultrawide Spectral Radioheliograph

Published online by Cambridge University Press:  09 September 2016

Yihua Yan ,
Linjie Chen ,
Sijie Yu  and
CSRH Team
Yihua Yan
Affiliation:
Key Laboratory of Solar Activity, Chinese Academy of Sciences, Beijing, 100012, China email: yyh@nao.cas.cn
Linjie Chen
Affiliation:
Key Laboratory of Solar Activity, Chinese Academy of Sciences, Beijing, 100012, China email: yyh@nao.cas.cn
Sijie Yu
Affiliation:
Key Laboratory of Solar Activity, Chinese Academy of Sciences, Beijing, 100012, China email: yyh@nao.cas.cn
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Abstract

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The Chinese Spectral Radioheliograph (CSRH) with two arrays in 400MHz-2GHz/2-15GHz ranges with 64/520 frequency channels have been established in Mingantu Observing Station, Inner Mongolia of China, since 2013 and is in test observations now. CSRH is renamed as Mingantu Ultrawide SpEctral Radioheliograph (MUSER) after its accomplishment. We introduce the progress and current status of MUSER. The first burst imaging results of MUSER is presented.

Keywords

Radioheliographsolar radio burstsflaresCMEscoronal magnetic field
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S320: Solar and Stellar Flares and their Effects on Planets , August 2015 , pp. 427 - 435
Copyright
Copyright © International Astronomical Union 2016 

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