Radio Observations of Coronal Mass Ejections: Space Weather Aspects

被引:24
作者
Vourlidas, Angelos [1 ]
Carley, Eoin P. [2 ]
Vilmer, Nicole [3 ,4 ]
机构
[1] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[2] Dublin Inst Adv Studies, Sch Cosm Phys, Dublin, Ireland
[3] Univ Paris, Sorbonne Univ, CNRS, LESIA,Observ Paris,Univ PSL, Meudon, France
[4] Univ Orleans, PSL Res Univ, Stn Radioastron Nancay, Observ Paris,CNRS, Nancay, France
来源
FRONTIERS IN ASTRONOMY AND SPACE SCIENCES | 2020年 / 7卷
关键词
sun; radio astronomy; coronal mass ejections; space weather; spectropolarimetry; SOLAR CORONA; X-RAY; SIGNATURES; PARTICLES; EMISSION; CURRENTS; REGIONS; BURSTS; ARRAY; SOHO;
D O I
10.3389/fspas.2020.00043
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We review the current state-of-affairs in radio observations of Coronal Mass Ejections (CMEs) from a Space Weather perspective. In particular, we examine the role of radio observations in predicting or presaging an eruption, in capturing the formation stages of the CME, and in following the CME evolution in the corona and heliosphere. We then look to the future and identify capabilities and research areas where radio observations-particularly, spectropolarimetric imaging-offer unique advantages for Space Weather research on CMEs. We close with a discussion of open issues and possible strategies for enhancing the relevance and importance of radio astronomy for Space Weather science.
引用
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页数:12
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