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Kinetic alfven waves in laboratory, ...

Chen, Ling.

Kinetic alfven waves in laboratory, space, and astrophysical plasmas

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Kinetic alfven waves in laboratory, space, and astrophysical plasmasby De-Jin Wu, Ling Chen.
作者:	Wu, De-Jin.
其他作者:	Chen, Ling.
出版者:	Singapore :Springer Singapore :2020.
面頁冊數:	xiii, 346 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
標題:	Magnetohydrodynamic waves.
電子資源:	https://doi.org/10.1007/978-981-13-7989-5
ISBN:	9789811379895$q(electronic bk.)

Kinetic alfven waves in laboratory, space, and astrophysical plasmas
Wu, De-Jin.

Kinetic alfven waves in laboratory, space, and astrophysical plasmas[electronic resource] /by De-Jin Wu, Ling Chen. - Singapore :Springer Singapore :2020. - xiii, 346 p. :ill., digital ;24 cm. - Atmosphere, earth, ocean & space,2524-440X. - Atmosphere, earth, ocean & space..

Basic Theories and Properties of KAWs -- KAWs in Laboratory Plasmas -- KAWs in Magnetosphere-Ionosphere Coupling -- KAWs in Solar Wind-Magnetosphere Interaction -- KAWs in Solar Wind Turbulence -- KAWs in Solar Atmosphere Heating -- KAWs in Other Astrophysical Plasmas.

This book provides a systematic introduction to the observation and application of kinetic Alfven waves (KAWs) in various plasma environments, with a special focus on the solar-terrestrial coupling system. Alfven waves are low-frequency and long-wavelength fluctuations that pervade laboratory, space and cosmic plasmas. KAWs are dispersive Alfven waves with a short wavelength comparable to particle kinematic scales and hence can play important roles in the energization and transport of plasma particles, the formation of fine magneto-plasma structures, and the dissipation of turbulent Alfven waves. Since the 1990s, experimental studies on KAWs in laboratory and space plasmas have significantly advanced our understanding of KAWs, making them an increasingly interesting subject. Without a doubt, the solar-terrestrial coupling system provides us with a unique natural laboratory for the comprehensive study of KAWs. This book presents extensive observations of KAWs in solar and heliospheric plasmas, as well as numerous applications of KAWs in the solar-terrestrial coupling system, including solar atmosphere heating, solarwind turbulence, solar wind-magnetosphere interactions, and magnetosphere-ionosphere coupling. In addition, for the sake of consistency, the book includes the basic theories and physical properties of KAWs, as well as their experimental demonstrations in laboratory plasmas. In closing, it discusses possible applications of KAWs to other astrophysical plasmas. Accordingly, the book covers all the major aspects of KAWs in a coherent manner that will appeal to advanced graduate students and researchers whose work involves laboratory, space and astrophysical plasmas.

ISBN: 9789811379895$q(electronic bk.)

Standard No.: 10.1007/978-981-13-7989-5doiSubjects--Topical Terms:

225451
Magnetohydrodynamic waves.

LC Class. No.: QC718.5.M36 / W834 2020

Dewey Class. No.: 530.44

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520 $a This book provides a systematic introduction to the observation and application of kinetic Alfven waves (KAWs) in various plasma environments, with a special focus on the solar-terrestrial coupling system. Alfven waves are low-frequency and long-wavelength fluctuations that pervade laboratory, space and cosmic plasmas. KAWs are dispersive Alfven waves with a short wavelength comparable to particle kinematic scales and hence can play important roles in the energization and transport of plasma particles, the formation of fine magneto-plasma structures, and the dissipation of turbulent Alfven waves. Since the 1990s, experimental studies on KAWs in laboratory and space plasmas have significantly advanced our understanding of KAWs, making them an increasingly interesting subject. Without a doubt, the solar-terrestrial coupling system provides us with a unique natural laboratory for the comprehensive study of KAWs. This book presents extensive observations of KAWs in solar and heliospheric plasmas, as well as numerous applications of KAWs in the solar-terrestrial coupling system, including solar atmosphere heating, solarwind turbulence, solar wind-magnetosphere interactions, and magnetosphere-ionosphere coupling. In addition, for the sake of consistency, the book includes the basic theories and physical properties of KAWs, as well as their experimental demonstrations in laboratory plasmas. In closing, it discusses possible applications of KAWs to other astrophysical plasmas. Accordingly, the book covers all the major aspects of KAWs in a coherent manner that will appeal to advanced graduate students and researchers whose work involves laboratory, space and astrophysical plasmas.
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