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實驗室、空間和天體等離子體中的動力學阿爾文波 版權信息
- ISBN：9787305239250
- 條形碼：9787305239250 ; 978-7-305-23925-0
- 裝幀：一般膠版紙
- 冊數：暫無
- 重量：暫無
- 所屬分類：>
實驗室、空間和天體等離子體中的動力學阿爾文波 本書特色
吳德金研究員從事動力學阿爾文波的研究二十多年，是這一領域的專家。本書由南京大學出版社和施普林格出版社（Springer）聯合出版，系統介紹了吳德金研究員團隊和該領域其他同行在這一國際前沿領域的研究成果，同時也是國家自然科學基金重點項目“太陽大氣中的精細結構及其波動過程與加熱機制”成果的反映，具有極高的學術價值。 本書入選江蘇省金陵科技著作出版基金項目。
實驗室、空間和天體等離子體中的動力學阿爾文波 內容簡介
本書以阿爾文波的理論與實驗研究為主線，以作者團隊的研究工作為主要內容，介紹了動力學阿爾文波的基礎理論與實驗研究，以及對一些觀測驗證和有關的應用。本書系統地介紹動力學阿爾文波在空間和天體等離子體中的應用，重點關注在日地耦合系統中的一些關鍵動力學區域，同時也對動力學阿爾文波在太陽系外其他高溫等離子體加熱和銀河系外延伸射電源的高能電子加速與噴流準直性問題中可能的應用進行了介紹和討論。為保證內容的完整性并方便讀者查閱，也對動力學阿爾文波的基本物理特性及其主要的實驗驗證分別進行了簡要介紹。本書主要讀者對象為等離子體物理、空間物理、太陽物理和天體等離子體領域的研究人員和高年級研究生，可為相關領域的研究者提供合適的參考。
實驗室、空間和天體等離子體中的動力學阿爾文波 目錄
Chapter 1 Basic Physical Properties of KAWs
1．1 From AWs to KAWs
1．2 Dispersion and Propagation of KAWs
1．3 Polarization and Wave-Particle Interaction of KAWs
1．4 Excitation of KAWs in Homogeneous Plasmas
1．5 Excitation of KAWs in Inhomogeneous Plasmas
1．6 Generation of KAWs by Nonlinear Processes
References
Chapter 2 Laboratory Experiments of KAWs
2．1 Early Experiments of Plasma Heating by KAWs
2．2 Measurements of KAW Dispersion Relations
2．3 Propagation and Dissipation of KAWs
2．4 Excitation and Evolution of KAWs by Plasma Striations
2．5 Generation of KAWs by Other Plasma Phenomena
2．6 Laboratory Experiments Versus Space Observations
References
Chapter 3 KAWs in Magnetosphere-Ionosphere Coupling
3．1 Solar Wind-Magnetosphere-Ionosphere Interaction
3．2 Aurora and Magnetosphere-Ionosphere Coupling
3．3 Observation and Identification of SKAWs
3．4 Theoretical Models of SKAWs in Auroral Plasmas
3．5 Auroral Electron Acceleration by SKAWs
References
Chapter 4 KAWs in Solar Wind-Magnetosphere Coupling
4．1 Solar Wind-Magnetosphere Interacting Boundary Layers
4．2 Observations of KAW Turbulence in Magnetosphere
4．3 Diffusion Equation of Particles Due to KAW Turbulence
4．4 Particle Transport by KAWs at Magnetopause
4．5 Formation of Ion Beams by KAWs in Magnetotail
References
Chapter fi KAW Turbulenee in Solar Wind
5．1 Solar Wind． Natural Laboratory for Plasma Turbulence
5．2 Anisotropic Cascade of AW Turbulence Towards Small Scales
5．2．1 Iroshnikov-Kraichnan Theory of AW Turbulence
5．2．2 Goldreich-Sridhar Theory of AW Turbulence
5．2．3 Boldyrev Theory of AW Turbulence
5．2．4 Observations of Spectral Anisotropy of AW Turbulence
5．3 Gyrokinetic Description of KAWs
5．3．1 Gyrokinetic Approximations
5．3．2 Gyrokinetic Equations
5．3．3 Gyrokinetic Dispersion Relation of KAWs
5．4 Theory and Simulation of KAWs Turbulence
5．4．1 Basic Properties of KAW Turbulence
5．4．2 Power Spectra of KAW Turbulence
5．4．3 AstroGK Simulations of Ion-Scale KAW Turbulence
5．4．4 AstroGK Simulations of Electron-Scale KAW Turbulence
5．4．5 Kinetic PIC Simulations of KAW Turbulence
5．4．6 Fluid-Like Simulations of KAW Turbulence
5．4．7 Effects of Dispersion on KAW Turbulent Spectra
5．5 Observational Identifications of KAW Turbulence
5．5．1 Initial Identifications of KAW Dispersion and Polarization
5．5．2 Refined Identifications of KAW Dispersion and Spectra
5．5．3 Identifications of KAW Magnetic Compressibility
5．5．4 Identifications of KAW Magnetic Helicity
References
Chapter 6 KAWs in Solar Atmosphere Heating
6．1 Modern View of Solar Coronal Heating Problem
6．2 Generation and Observation of KAWs in Solar Atmosphere
6．2．1 Generation of KAWs by Solar AW Turbulence
6．2．2 Generation of KAWs by Solar Field-Aligned Currents
6．2．3 Generation of KAWs by Solar Field-Aligned Striations
6．2．4 Possible Solar Observation Evidence of KAWs
6．3 Upper Chromospheric Heating by Joule Dissipation of KAWs
6．3．1 Sunspot Upper-Chromospheric Heating Problem
6．3．2 Joule Dissipation of KAWs by Collision Resistance
6．3．3 Upper-Chromospheric Heating by KAW Joule Dissipation
6．4 Inner Coronal Heating by Landau Damping of KAWs
6．4．1 Heating Problems of Coronal Loops and Plumes
6．4．2 Landau Damping of KAWs
6．4．3 Coronal Loop Heating by KAW Landau Damping
6．4．4 Empirical Model of Coronal Hole and Plumes
6．4．5 Coronal Plume Heating by KAW Landau Damping
6．5 Extended Solar Coronal Heating by Nonlinear KAWs
6．5．1 Anomalous Energization Phenomena of Coronal Ions
6．5．2 Interaction of Minor Heavy Ions with SKAWs
6．5．3 Energization of Minor Heavy Ions by SKAWs
6．6 Interplanetary Solar Wind Heating by Turbulent KAWs
References
Chapter 7 KAWs in Extrasolar Astrophysical Plasmas
7．1 Plasma Turbulence from Cosmological to Kinetic Scales
7．2 KAW Heating of Stellar and Accretion Disk Coronae
7．3 KAW Heating of Galactic Halos and Intracluster Medium
7．4 KAWs and Their Roles in Extended Radio Sources
References
1．1 From AWs to KAWs
1．2 Dispersion and Propagation of KAWs
1．3 Polarization and Wave-Particle Interaction of KAWs
1．4 Excitation of KAWs in Homogeneous Plasmas
1．5 Excitation of KAWs in Inhomogeneous Plasmas
1．6 Generation of KAWs by Nonlinear Processes
References
Chapter 2 Laboratory Experiments of KAWs
2．1 Early Experiments of Plasma Heating by KAWs
2．2 Measurements of KAW Dispersion Relations
2．3 Propagation and Dissipation of KAWs
2．4 Excitation and Evolution of KAWs by Plasma Striations
2．5 Generation of KAWs by Other Plasma Phenomena
2．6 Laboratory Experiments Versus Space Observations
References
Chapter 3 KAWs in Magnetosphere-Ionosphere Coupling
3．1 Solar Wind-Magnetosphere-Ionosphere Interaction
3．2 Aurora and Magnetosphere-Ionosphere Coupling
3．3 Observation and Identification of SKAWs
3．4 Theoretical Models of SKAWs in Auroral Plasmas
3．5 Auroral Electron Acceleration by SKAWs
References
Chapter 4 KAWs in Solar Wind-Magnetosphere Coupling
4．1 Solar Wind-Magnetosphere Interacting Boundary Layers
4．2 Observations of KAW Turbulence in Magnetosphere
4．3 Diffusion Equation of Particles Due to KAW Turbulence
4．4 Particle Transport by KAWs at Magnetopause
4．5 Formation of Ion Beams by KAWs in Magnetotail
References
Chapter fi KAW Turbulenee in Solar Wind
5．1 Solar Wind． Natural Laboratory for Plasma Turbulence
5．2 Anisotropic Cascade of AW Turbulence Towards Small Scales
5．2．1 Iroshnikov-Kraichnan Theory of AW Turbulence
5．2．2 Goldreich-Sridhar Theory of AW Turbulence
5．2．3 Boldyrev Theory of AW Turbulence
5．2．4 Observations of Spectral Anisotropy of AW Turbulence
5．3 Gyrokinetic Description of KAWs
5．3．1 Gyrokinetic Approximations
5．3．2 Gyrokinetic Equations
5．3．3 Gyrokinetic Dispersion Relation of KAWs
5．4 Theory and Simulation of KAWs Turbulence
5．4．1 Basic Properties of KAW Turbulence
5．4．2 Power Spectra of KAW Turbulence
5．4．3 AstroGK Simulations of Ion-Scale KAW Turbulence
5．4．4 AstroGK Simulations of Electron-Scale KAW Turbulence
5．4．5 Kinetic PIC Simulations of KAW Turbulence
5．4．6 Fluid-Like Simulations of KAW Turbulence
5．4．7 Effects of Dispersion on KAW Turbulent Spectra
5．5 Observational Identifications of KAW Turbulence
5．5．1 Initial Identifications of KAW Dispersion and Polarization
5．5．2 Refined Identifications of KAW Dispersion and Spectra
5．5．3 Identifications of KAW Magnetic Compressibility
5．5．4 Identifications of KAW Magnetic Helicity
References
Chapter 6 KAWs in Solar Atmosphere Heating
6．1 Modern View of Solar Coronal Heating Problem
6．2 Generation and Observation of KAWs in Solar Atmosphere
6．2．1 Generation of KAWs by Solar AW Turbulence
6．2．2 Generation of KAWs by Solar Field-Aligned Currents
6．2．3 Generation of KAWs by Solar Field-Aligned Striations
6．2．4 Possible Solar Observation Evidence of KAWs
6．3 Upper Chromospheric Heating by Joule Dissipation of KAWs
6．3．1 Sunspot Upper-Chromospheric Heating Problem
6．3．2 Joule Dissipation of KAWs by Collision Resistance
6．3．3 Upper-Chromospheric Heating by KAW Joule Dissipation
6．4 Inner Coronal Heating by Landau Damping of KAWs
6．4．1 Heating Problems of Coronal Loops and Plumes
6．4．2 Landau Damping of KAWs
6．4．3 Coronal Loop Heating by KAW Landau Damping
6．4．4 Empirical Model of Coronal Hole and Plumes
6．4．5 Coronal Plume Heating by KAW Landau Damping
6．5 Extended Solar Coronal Heating by Nonlinear KAWs
6．5．1 Anomalous Energization Phenomena of Coronal Ions
6．5．2 Interaction of Minor Heavy Ions with SKAWs
6．5．3 Energization of Minor Heavy Ions by SKAWs
6．6 Interplanetary Solar Wind Heating by Turbulent KAWs
References
Chapter 7 KAWs in Extrasolar Astrophysical Plasmas
7．1 Plasma Turbulence from Cosmological to Kinetic Scales
7．2 KAW Heating of Stellar and Accretion Disk Coronae
7．3 KAW Heating of Galactic Halos and Intracluster Medium
7．4 KAWs and Their Roles in Extended Radio Sources
References
展開全部
實驗室、空間和天體等離子體中的動力學阿爾文波 作者簡介
吳德金，紫金山天文臺研究員、博士研究生導師、中國科學院特聘研究員，主要從事太陽物理、等離子天體物理和空間等離子體等領域的研究工作。研究項目《太陽和空間等離子體中的動力學阿爾文波與電子能化機制》獲得“江蘇省2006年度科技進步一等獎（排名第一）”，科研成果三次入選“國家天文臺年度十大天文科技進展”，先后得到國家杰出青年科學基金項目、中國科學院百人計劃資助項目等20多項資助，取得了一系列重要的創新性研究成果。在SCI收錄期刊上發表有關學術研究論文130余篇，引用達1400多次，得到了國內外同行專家的充分肯定，在相關研究領域產生了一定的學術影響，特別是在動力學阿爾文波的研究領域居于國際先進水平。在由國際天文聯合會主席等國際著名專家組成的權威評估小組給中國科學院的專家評估報告中，對吳德金及其團隊的工作給予了極高評價，認為“吳德金及其領導的研究組在動力學阿爾文波及其應用的研究領域里具有國際競爭力、達到國際先進水平”。
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