Astrophysical Hydromagnetic Turbulence

被引：0
|
作者：
A. Brandenburg
A. Lazarian
机构：
[1] Stockholm University,Nordita, KTH Royal Institute of Technology
[2] Stockholm University,Department of Astronomy
[3] University of Wisconsin-Madison,Department of Astronomy
来源：
Space Science Reviews | 2013年 / 178卷
关键词：
Magnetic fields; Turbulence; Sun: magnetic fields; ISM: magnetic fields;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Recent progress in astrophysical hydromagnetic turbulence is being reviewed. The physical ideas behind the now widely accepted Goldreich–Sridhar model and its extension to compressible magnetohydrodynamic turbulence are introduced. Implications for cosmic ray diffusion and acceleration is being discussed. Dynamo-generated magnetic fields with and without helicity are contrasted against each other. Certain turbulent transport processes are being modified and often suppressed by anisotropy and inhomogeneities of the turbulence, while others are being produced by such properties, which can lead to new large-scale instabilities of the turbulent medium. Applications of various such processes to astrophysical systems are being considered.
引用
收藏
页码：163 / 200
页数：37
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