中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Possible Noise Nature of Elsasser Variable z(-) in Highly Alfvenic Solar Wind Fluctuations

文献类型:期刊论文

作者Wang, X.; Tu, C. -Y.; He, J. -S.; Wang, L. -H.; Yao, S.; Zhang, L.; Tu, CY (reprint author), Peking Univ, Sch Earth & Space Sci, Beijing, Peoples R China.
刊名JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
出版日期2018
卷号123期号:1页码:57-67
ISSN号2169-9380
英文摘要It has been a long-standing debate on the nature of Elsasser variable z(-) observed in the solar wind fluctuations. It is widely believed that z(-) represents inward propagating Alfven waves and interacts nonlinearly with z(+) (outward propagating Alfven waves) to generate energy cascade. However, z(-) variations sometimes show a feature of convective structures. Here we present a new data analysis on autocorrelation functions of z(-) in order to get some definite information on its nature. We find that there is usually a large drop on the z(-) autocorrelation function when the solar wind fluctuations are highly Alfvenic. The large drop observed by Helios 2 spacecraft near 0.3AU appears at the first nonzero time lag r = 81s, where the value of the autocorrelation coefficient drops to 25%-65% of that at r = 0s. Beyond the first nonzero time lag, the autocorrelation coefficient decreases gradually to zero. The drop of z(-) correlation function also appears in the Wind observations near 1AU. These features of the z(-) correlation function may suggest that z(-) fluctuations consist of two components: high-frequency white noise and low-frequency pseudo structures, which correspond to flat and steep parts of z(-) power spectrum, respectively. This explanation is confirmed by doing a simple test on an artificial time series, which is obtained from the superposition of a random data series on its smoothed sequence. Our results suggest that in highly Alfvenic fluctuations, z(-) may not contribute importantly to the interactions with z(+) to produce energy cascade.
语种英语
资助机构National Natural Science Foundation of China [41504130, 41474147, 41674171, 41231069] ; Young Elite Scientists Sponsorship Program by China Association for Science and Technology [2016QNRC001]
源URL[http://ir.nssc.ac.cn/handle/122/6204]  
专题国家空间科学中心_空间科学部
通讯作者Tu, CY (reprint author), Peking Univ, Sch Earth & Space Sci, Beijing, Peoples R China.
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GB/T 7714
Wang, X.,Tu, C. -Y.,He, J. -S.,et al. Possible Noise Nature of Elsasser Variable z(-) in Highly Alfvenic Solar Wind Fluctuations[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2018,123(1):57-67.
APA Wang, X..,Tu, C. -Y..,He, J. -S..,Wang, L. -H..,Yao, S..,...&Tu, CY .(2018).Possible Noise Nature of Elsasser Variable z(-) in Highly Alfvenic Solar Wind Fluctuations.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,123(1),57-67.
MLA Wang, X.,et al."Possible Noise Nature of Elsasser Variable z(-) in Highly Alfvenic Solar Wind Fluctuations".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 123.1(2018):57-67.

入库方式: OAI收割

来源:国家空间科学中心

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