Kinetic Alfvén Waves in Laboratory, Space, and Astrophysical Plasmas
Kinetic Alfvén Waves in Laboratory, Space, and Astrophysical Plasmas
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DOI：
10.1007/978-981-13-7989-5
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发表时间：
2020
期刊：
影响因子：
--
通讯作者：
Dejin Wu;Ling Chen
中科院分区：
文献类型：
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作者：
Dejin Wu;Ling Chen
在姊妹篇《动力学阿尔文波：理论、实验和应用》中，我们介绍了基于磁性等离子体动力学和流体描述的动力学阿尔文波（KAWs）的系统理论和基本原理。本卷建立在此基础上，并进行深入的分析和讨论的观测，产生，和应用的KAWs在各种等离子体环境中的太阳-地球耦合系统，这是一个独特的天然实验室的全面和彻底的研究KAWs。然而，首先，在这一章的介绍中，我们简要地回顾了KAWs的主要物理性质，而没有证明，这是从同伴卷，并建立了基础，为以下章节。
In the companion volume,Kinetic Alfvén Wave: Theory, Experiment, and Application, we have presented the systematic theories and basic principles of kinetic Alfvén waves (KAWs) based on both kinetic and fluid descriptions of magnetic plasmas. The present volume builds upon that and proceeds into the in-depth analyses and discussions of observation, generation, and application of KAWs in various plasma environments in the solar-terrestrial coupling system, which is a unique natural laboratory for the comprehensive and thorough study of KAWs. However, first of all, in this introductory chapter we concisely review main physical properties of KAWs without proving, which are from the companion volume and set up the basis for the following chapters.