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实验室、空间和天体等离子体中的动力学阿尔文波

实验室、空间和天体等离子体中的动力学阿尔文波

1星价 ¥121.0 (7.2折)
2星价¥121.0 定价¥168.0
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  • ISBN:9787305239250
  • 装帧:一般胶版纸
  • 册数:暂无
  • 重量:暂无
  • 开本:16开
  • 页数:378
  • 出版时间:2021-10-01
  • 条形码:9787305239250 ; 978-7-305-23925-0

本书特色

吴德金研究员从事动力学阿尔文波的研究二十多年,是这一领域的专家。本书由南京大学出版社和施普林格出版社(Springer)联合出版,系统介绍了吴德金研究员团队和该领域其他同行在这一国际前沿领域的研究成果,同时也是国家自然科学基金重点项目“太阳大气中的精细结构及其波动过程与加热机制”成果的反映,具有极高的学术价值。 本书入选江苏省金陵科技著作出版基金项目。

内容简介

本书以阿尔文波的理论与实验研究为主线,以作者团队的研究工作为主要内容,介绍了动力学阿尔文波的基础理论与实验研究,以及对一些观测验证和有关的应用。本书系统地介绍动力学阿尔文波在空间和天体等离子体中的应用,重点关注在日地耦合系统中的一些关键动力学区域,同时也对动力学阿尔文波在太阳系外其他高温等离子体加热和银河系外延伸射电源的高能电子加速与喷流准直性问题中可能的应用进行了介绍和讨论。为保证内容的完整性并方便读者查阅,也对动力学阿尔文波的基本物理特性及其主要的实验验证分别进行了简要介绍。本书主要读者对象为等离子体物理、空间物理、太阳物理和天体等离子体领域的研究人员和高年级研究生,可为相关领域的研究者提供合适的参考。

目录

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
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作者简介

吴德金,紫金山天文台研究员、博士研究生导师、中国科学院特聘研究员,主要从事太阳物理、等离子天体物理和空间等离子体等领域的研究工作。研究项目《太阳和空间等离子体中的动力学阿尔文波与电子能化机制》获得“江苏省2006年度科技进步一等奖(排名**)”,科研成果三次入选“国家天文台年度十大天文科技进展”,先后得到国家杰出青年科学基金项目、中国科学院百人计划资助项目等20多项资助,取得了一系列重要的创新性研究成果。在SCI收录期刊上发表有关学术研究论文130余篇,引用达1400多次,得到了国内外同行专家的充分肯定,在相关研究领域产生了一定的学术影响,特别是在动力学阿尔文波的研究领域居于国际先进水平。在由国际天文联合会主席等国际著名专家组成的权威评估小组给中国科学院的专家评估报告中,对吴德金及其团队的工作给予了极高评价,认为“吴德金及其领导的研究组在动力学阿尔文波及其应用的研究领域里具有国际竞争力、达到国际先进水平”。

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