4.5 Review

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

期刊

SPACE SCIENCE REVIEWS
卷 160, 期 1-4, 页码 145-168

出版社

SPRINGER
DOI: 10.1007/s11214-011-9793-9

关键词

Magnetic reconnection; Turbulence; Solar wind; Corona

资金

  1. NASA [NNX08AI47G, NNX08AM48G]
  2. MMS project theory and modeling program [NNX08AI47G]
  3. Solar Probe Plus project
  4. NSF [NNX08AM48G]
  5. NASA [NNX08AM48G, 98521, NNX08AI47G, 100186] Funding Source: Federal RePORTER

向作者/读者索取更多资源

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.

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