期刊
NONLINEAR PROCESSES IN GEOPHYSICS
卷 16, 期 1, 页码 83-98出版社
COPERNICUS GESELLSCHAFT MBH
DOI: 10.5194/npg-16-83-2009
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- ANR [06-BLAN-0363-01]
- INSU/PNST Program
The paper reviews the recent progress on wave turbulence for magnetized plasmas (MHD, Hall MHD and electron MHD) in the incompressible and compressible cases. The emphasis is made on homogeneous and anisotropic turbulence which usually provides the best theoretical framework to investigate space and laboratory plasmas. The solar wind and the coronal heating problems are presented as two examples of application of anisotropic wave turbulence. The most important results of wave turbulence are reported and discussed in the context of natural and simulated magnetized plasmas. Important issues and possible spurious interpretations are also discussed.
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