Volume 33 Issue 4
Jul.  2013
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L. YANG, J. K. CHAO. Alfvén Waves in the Solar Wind[J]. Chinese Journal of Space Science, 2013, 33(4): 353-373. doi: 10.11728/cjss2013.04.353
Citation: L. YANG, J. K. CHAO. Alfvén Waves in the Solar Wind[J]. Chinese Journal of Space Science, 2013, 33(4): 353-373. doi: 10.11728/cjss2013.04.353

Alfvén Waves in the Solar Wind

doi: 10.11728/cjss2013.04.353
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  • Author Bio:

    L. YANG, ylei@pmo.ac.cn

  • Received Date: 2013-05-02
  • Rev Recd Date: 2013-05-20
  • Publish Date: 2013-07-15
  • Alfvén waves are found to be ubiquitous in the solar wind. Recent progress in observational studies of the waves is reviewed to formulate a microscopic picture for the Alfvénic fluctuations. The main aspects of the observational properties of these waves, including the wave intervals, propagation, evolution, origin and generation, are presented. Then Alfvén wave heating and acceleration of the solar wind plasma are briefly introduced. The relation of the waves to rotational and tangential discontinuities, magnetic decreases, and other relatively large-scale structures such as flux tubes/ropes, magnetic clouds and interplanetary coronal mass ejections in the solar wind is particularly investigated. Finally, some remaining open questions are also indicated due to their fundamental importance of understanding of the physical nature of Alfvén waves and the role of the waves in heating and accelerating the solar wind.

     

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