Who Needs Turbulence? A Review of Turbulence Effects in the Heliosphere and on the Fundamental Process of Reconnection

被引:201
作者
Matthaeus, W. H. [1 ]
Velli, M. [2 ]
机构
[1] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
Magnetic reconnection; Turbulence; Solar wind; Corona; SOLAR-WIND; ALFVEN WAVES; MAGNETIC RECONNECTION; RADIAL EVOLUTION; OBSERVATIONAL CONSTRAINTS; STATISTICAL PROPERTIES; CYCLOTRON WAVES; DRIVEN; DISSIPATION; FIELD;
D O I
10.1007/s11214-011-9793-9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The significant influences of turbulence in neutral fluid hydrodynamics are well accepted but the potential for analogous effects in space and astrophysical plasmas is less widely recognized. This situation sometimes gives rise to the question posed in the title; "Who need turbulence?" After a brief overview of turbulence effects in hydrodynamics, some likely effects of turbulence in solar and heliospheric plasma physics are reviewed here, with the goal of providing at least a partial answer to the posed question.
引用
收藏
页码:145 / 168
页数:24
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