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Titlebook: Kinetic Alfvén Waves in Laboratory, Space, and Astrophysical Plasmas; De-Jin Wu,Ling Chen Book 2020 Nanjing University Press 2020 Alfven w

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發(fā)表于 2025-3-21 17:50:23 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Kinetic Alfvén Waves in Laboratory, Space, and Astrophysical Plasmas
編輯De-Jin Wu,Ling Chen
視頻videohttp://file.papertrans.cn/544/543045/543045.mp4
概述Provides an extensive review of observations of kinetic Alfven waves (KAWs) in solar and heliospheric plasmas.Presents numerous applications of KAWs in the solar–terrestrial coupling system.Offers a d
叢書名稱Atmosphere, Earth, Ocean & Space
圖書封面Titlebook: Kinetic Alfvén Waves in Laboratory, Space, and Astrophysical Plasmas;  De-Jin Wu,Ling Chen Book 2020 Nanjing University Press 2020 Alfven w
描述.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 magneto
出版日期Book 2020
關(guān)鍵詞Alfven waves; Kinetic Alfven waves; Solar and heliospheric plasmas; Aurora and Auroral electron acceler
版次1
doihttps://doi.org/10.1007/978-981-13-7989-5
isbn_softcover978-981-13-7991-8
isbn_ebook978-981-13-7989-5Series ISSN 2524-440X Series E-ISSN 2524-4418
issn_series 2524-440X
copyrightNanjing University Press 2020
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 23:24:00 | 只看該作者
Laboratory Experiments of KAWs,ot been made until 1949. One of important reasons for this delay is that the long wavelength and low frequency characteristics of AWs make them very difficult to study experimentally in laboratory. The similar case happened on KAWs. When KAWs were discovered in 1970’s, their ability to heat plasma p
板凳
發(fā)表于 2025-3-22 03:57:22 | 只看該作者
KAWs in Magnetosphere-Ionosphere Coupling,e earth. The conception of intermittent plasma streams consisting of electrons and ions from the sun was introduced by Chapman and Ferraro (1930) to explain the cause of geomagnetic storms, and later the existence of the solar wind continuously blowing away from the sun was proposed successively by
地板
發(fā)表于 2025-3-22 05:26:04 | 只看該作者
5#
發(fā)表于 2025-3-22 09:17:52 | 只看該作者
KAW Turbulence in Solar Wind,f thermal fluctuations (or i.e., thermal noise) that is caused by the discrete randomness of microscopic particles (or i.e., the hypothesis of molecular chaos), however, the turbulent stochasticity of the plasma turbulence should be attributed to the chaotic nondeterminacy of plasma collective modes
6#
發(fā)表于 2025-3-22 13:56:12 | 只看該作者
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發(fā)表于 2025-3-22 17:17:41 | 只看該作者
KAWs in Extrasolar Astrophysical Plasmas,related particle kinetic phenomena, such as the auroral energetic electron acceleration in auroral magnetospheric plasmas, the anomalous particle transport in the magnetopause, the kinetic turbulence in the solar wind, and the solar coronal heating problem. The solar and solar-system plasma, especia
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發(fā)表于 2025-3-22 21:16:05 | 只看該作者
detection of a new substance class.Describes potential appliGalanin is a neuropeptide found both in the central and peripheral nervous system. The 29-amino acid peptide (named after its N-terminal glycine and C-terminal alanine) was identified in 1983 by its C-terminal amidation. This ‘reverse‘ appr
9#
發(fā)表于 2025-3-23 03:41:10 | 只看該作者
De-Jin Wu,Ling Chen-terminal alanine) was identified in 1983 by its C-terminal amidation. This ‘reverse‘ approach, that is to discover a substance through a distinct chemical feature, and only subsequently to characterize its biological activity, was novel and has been successful in the identification of several other
10#
發(fā)表于 2025-3-23 06:51:39 | 只看該作者
De-Jin Wu,Ling Chendetection of a new substance class.Describes potential appliGalanin is a neuropeptide found both in the central and peripheral nervous system. The 29-amino acid peptide (named after its N-terminal glycine and C-terminal alanine) was identified in 1983 by its C-terminal amidation. This ‘reverse‘ appr
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