Observation of spontaneous decay of Alfvenic fluctuations into co- and counter-propagating magnetosonic waves in a laboratory plasma

被引:4
作者
Shi, Peiyun [1 ]
Yang, Zhida [1 ]
Luo, Ming [1 ]
Wang, Rongsheng [2 ]
Lu, Quanming [2 ]
Sun, Xuan [1 ]
机构
[1] Univ Sci & Technol China, Dept Engn & Appl Phys, Hefei 230026, Anhui, Peoples R China
[2] Univ Sci & Technol China, Dept Geophys & Planetary Sci, Hefei 230026, Anhui, Peoples R China
基金
国家重点研发计划; 中国国家自然科学基金;
关键词
INTERSTELLAR TURBULENCE; PARAMETRIC DECAY; INSTABILITIES;
D O I
10.1063/1.5082802
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
We show experimentally that Alfvenic fluctuations can spontaneously decay into a fast and a slow magnetosonic wave in an inhomogeneous plasma. The fast wave of higher frequency propagates in the same direction, while the slow wave of lower frequency propagates in the opposite direction with the pump wave. Both of the daughter waves are characterized by strong parallel but modest perpendicular fluctuations. The measured frequencies and wavenumbers are found to satisfy the energy and momentum conservation conditions for a nonlinear three wave interaction. The evidence of energy flowing from pump fluctuations into daughter waves is also presented in this paper. The results may shed light on the origin of inward Alfven waves observed in the solar corona and chromosphere and how shear Alfven waves deposit its energy by driving compressional perturbations. Published under license by AIP Publishing.
引用
收藏
页数:5
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