中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Determining the mechanism of cusp proton aurora

文献类型:期刊论文

作者Xiao, Fuliang; Zong, Qiugang; Su, Zhenpeng; Yang, Chang; He, Zhaoguo; Wang, Yongfu; Gao, Zhonglei
刊名SCIENTIFIC REPORTS
出版日期2013
卷号3页码:1654
ISSN号2045-2322
通讯作者Xiao, FL (reprint author), Changsha Univ Sci & Technol, Sch Phys & Elect Sci, Changsha 410004, Hunan, Peoples R China.
英文摘要Earth's cusp proton aurora occurs near the prenoon and is primarily produced by the precipitation of solar energetic (2-10 keV) protons. Cusp auroral precipitation provides a direct source of energy for the high-latitude dayside upper atmosphere, contributing to chemical composition change and global climate variability. Previous studies have indicated that magnetic reconnection allows solar energetic protons to cross the magnetopause and enter the cusp region, producing cusp auroral precipitation. However, energetic protons are easily trapped in the cusp region due to a minimum magnetic field existing there. Hence, the mechanism of cusp proton aurora has remained a significant challenge for tens of years. Based on the satellite data and calculations of diffusion equation, we demonstrate that EMIC waves can yield the trapped proton scattering that causes cusp proton aurora. This moves forward a step toward identifying the generation mechanism of cusp proton aurora.
收录类别SCI
语种英语
源URL[http://ir.nssc.ac.cn/handle/122/4976]  
专题国家空间科学中心_空间环境部
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GB/T 7714
Xiao, Fuliang,Zong, Qiugang,Su, Zhenpeng,et al. Determining the mechanism of cusp proton aurora[J]. SCIENTIFIC REPORTS,2013,3:1654.
APA Xiao, Fuliang.,Zong, Qiugang.,Su, Zhenpeng.,Yang, Chang.,He, Zhaoguo.,...&Gao, Zhonglei.(2013).Determining the mechanism of cusp proton aurora.SCIENTIFIC REPORTS,3,1654.
MLA Xiao, Fuliang,et al."Determining the mechanism of cusp proton aurora".SCIENTIFIC REPORTS 3(2013):1654.

入库方式: OAI收割

来源:国家空间科学中心

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