自然科學類

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相關購書資訊(請參考以下連結):

  •   隨著太空電漿物理現象的不同,其所涵蓋的特徵尺度範圍可小至電子的慣性尺度,也可大至磁流體力學(MHD)的尺度。雖然利用磁流體電漿模型,已經可用來描述許多的太空物理現象,但是就像大氣物理中的地轉風模式一樣,我們應該要謹慎考慮它們的適用範圍。本書的重點之一,就是要教導學生,科學家是如何得到那些特定電漿模型的控制方程式,並讓讀者了解,要獲得這套控制方程式,需要做哪些基本的假設。我們相信,除非學生能徹底了解各種電漿模式的控制方程式以及它們的線性色散關係是如何推導出來的,否則是很難真正了解不同電漿模型的適用條件,也自然很難對症下藥,選用正確的電漿模式,來解釋分析觀測到的物理現象。
      本書一開始先介紹電漿微觀動力模式、電子-正離子雙流體模式、與單流體電漿模式的基本方程式。接著介紹電子-正離子雙流體電漿與磁流體電漿中的線性波色散關係式。並於本書後段介紹電漿微觀動力模式中的線性波色散關係式。因為認識帶電粒子在相空間中的運動軌跡,將有助於了解電漿微觀動力模式中,波與粒子的交互作用,因此在介紹電漿微觀動力模式的線性波色散關係前,本書將先介紹如何分析帶電粒子在不同電磁場環境中,所可能出現的多重時間尺度的運動情形。
      本書是針對兩學期研究所課程所設計的教科書。內容只涵蓋電漿物理的基本課題,因此授課老師可在一學年的時間裡,輕鬆的教完本書全部的課程。本書中第二、三章所推導的各種基本方程式,可為太空觀測資料的分析工作以及不同尺度電漿模擬碼的設計工作,提供非常實用的理論基礎。包括了太空物理、天文物理、與實驗室電漿物理等領域的學生與研究人員將發現本書的內容實用,且對相關研究工作有所幫助。
      本書封面圖片為沿著日地連線方向所作的磁鞘觀測結果。這項觀測結果顯示,或式(3.62),是一個比著名的CGL雙絕熱狀態方程式,還更具普遍性的絕熱方程式。(感謝趙寄昆教授提供這份珍貴的太空觀測資料分析結果。)
  • 呂凌霄
    國立中央大學太空科學研究所&大氣科學系副教授
    美國阿拉斯加大學費班克分校太空物理博士
    研究專長:太空物理、電漿物理、數值模擬
  • Preface

    Chapter 1 Introduction
    1.1. Definition of Plasma
    1.2. The SI Units and The Gaussian Units
    1.3. Temperature in Units of oK and eV
    1.4. Boltzmann Relation
    1.5. Debye Shielding and Debye Length
    1.6. Plasma Parameter
    1.7. Plasma Frequency
    1.8. Gyro Frequency and Gyro Radius (or Larmor Radius)
    1.9. Collisions

    Chapter 2 Deriving the Vlasov Equation From the Klimontovich Equation
    2.1. Klimontovich Equation
    2.2. Vlasov Equation

    Chapter 3 Deriving the Fluid Equations From the Vlasov Equation
    3.1. The Vlasov-Maxwell System
    3.2. The Fluid Variables
    3.3. The Fluid Equations

    Chapter 4 Deriving the Vlasov Equation From the Liouville Equation
    4.1. Liouville Equation
    4.2. BBGKY Hierarchy

    Chapter 5 Linear Waves in the Electron-Ion Two-Fluid Plasma
    5.1. How to Linearize the Nonlinear Plasma Equations
    5.2. Linear Plane Waves in Uniform Two-Fluid Plasma
    5.3. Dispersion Relations of High-Frequency Waves in a Uniform Two-Fluid Plasma
    5.4. Dispersion Relations of Cross-Ion-Electron-Time-Scale Linear Wave Modes in Uniform Two-Fluid Plasma

    Chapter 6 Linear Waves in the MHD Plasma
    6.1. Linearized Wave Equations in a Uniform Isotropic MHD Plasma
    6.2. Linear Wave Modes in the MHD Plasma

    Chapter 7 Particle Motions With Multiple Time Scales
    7.1. Periodic Motions and Drift Motions of a Charged Particle
    7.2. Fluid Drift 103
    7.3. Drift Motion in Time-Dependent Fields 106

    Chapter 8 Equilibrium Solutions of the Vlasov Equation
    8.1. Characteristic Curves of a Partial Differential Equation
    8.2. Equilibrium Solutions of Time-Independent Vlasov-Maxwell Equations

    Chapter 9 Electrostatic Linear Waves in the Vlasov Plasma
    9.1. Landau Contour
    9.2. Linear Dispersion Relations of Electrostatic Waves
    9.3. Landau Damping
    9.4. Nyquist Method

    Chapter 10 Two-Stream Instability

    Chapter 11 Linear Waves in the Vlasov Plasma
    11.1. Linear Waves in Field-Free Plasma (E00, B00)
    11.2. Linear Waves in Magnetized Plasma With Uniform Background B0

    Appendix A Static Electric Field and Magnetic Field
    A.1. General Solutions
    A.2. Solutions of Special Cases

    Appendix B Ohm’s Law in One-Fluid Plasma

    Appendix C Frozen-in Flux
    C.1. Proof of Frozen-in Flux (Method 1)
    C.2. Proof of Frozen-in Flux (Method 2)
    C.3. Conservation of Circulation vs. Frozen-in Flux in MHD Plasma
    C.4 Equipotential Surface in MHD Plasma

    Appendix D Curvature Drift

    Appendix E Gradient B Drift

    Appendix F Deriving the Relativistic Vlasov Equation From the Relativistic Klimontovich Equation
    F.1. Relativistic Klimontovich Equation
    F.2. Relativistic Vlasov Equation

    Appendix G Functions of Complex Variable
    G.1. Analytic Function & Residue Theorem
    G.2. Branch Point and Riemann Surface

    Appendix H Special Functions for Studying Linear Waves in Kinetic Plasmas
    H.1. Bessel Function
    H.2. Error Function
    H.3. Plasma Dispersion Function
    Index
  •   The characteristic scale lengths of various space plasma phenomena range from the electron inertial length to the magnetohydrodynamic (MHD) scale length. Just like the geostrophic-wind approximation in the atmospheric physics, the MHD approximation in the space plasma physics has limitation in its applications. One of the important goals of this book is to show the students how scientists obtain the governing equations of a given plasma model and what assumptions have been made to obtain the set of governing equations shown in the literatures. We believe that, unless the students know how to derive the governing equations and how to obtain the wave mode from a simplified linear dispersion relation, it will be difficult for the students to fully understand the limitations of a given plasma model and how to choose the correct model to explain the observed phenomena.
      This book is written based on three textbooks: Krall & Trivelpiece (1973), Nicholson (1983), Chen (1984), which are the most popular textbooks when I was a student, as well as the lectures I learned from Professor J. K. Chao when I was an undergraduate student in National Central University, and the lectures I learned from Professor J. R. Kan when I was a graduate student in University of Alaska Fairbanks. I later found out that the extra information I learned from Professor Chao can be found in the following books or articles: Chao (1970), Rossi & Olbert (1970), and Kantrowitz & Petschek (1966). The extra information I learned from Professor Kan are based on the classical book by Stix (1962). Of course, I have also add additional information based on my own research experiences in various subjects.
      Many textbooks and theoretical papers written before 1980s or even 1990s are based on the Gaussian units. Since magnetic field and electric field have the same dimension in the Gaussian units, it is easy for theorists to check the correctness of their theoretical derivations. But all instruments are designed based on the SI units, thus, it is hard to apply the theoretical results (in the Gaussian units) to the space observations (in the SI units).   Scientists in our space community have tried very hard to change Gaussian units to SI units in all the new textbooks and scientific papers. Change of the units makes the old textbooks and the classical papers hard to follow by the readers of the new generations. We use the SI units in most of the derivations presented in this book. To help the students to read the classical papers in the literatures, we also present the basic equations in both units in Chapters 1 and 3. A brief summary of each chapter is given below:
      Chapter 1 gives a brief introduction to the plasma physics. In addition to introduce the characteristic frequencies, characteristic scale lengths, and collision frequencies, I also review the SI units and the Gaussian units in Chapter 1.
      Chapter 2 derives the Vlasov equation based on the Klimontovich equation, which I learned from Nicholson (1983). They are many different ways to obtain the Vlasov equation (e.g., Nicholson, 1983). I preferred to derive the Vlasov equation from the Klimontovich equation, for the reason that the approaches used in the Klimontovich equations are very similar to the approaches used in the particle-code simulation.
      Chapter 3 derives the two-fluid equations and the one-fluid equations from the Vlasov equation. This chapter is written based on what I learned from Professor J. K. Chao (Chao, 1970; Rossi & Olbert, 1970) and with some extensions based on my own experiences in these subjects. The fluid equations in the flux conservation forms shown in this chapter are particularly useful in analyzing the space plasma data and in designing the fluid simulation models.
      Chapter 4 shows the classical way to obtain the Boltzmann equation from the Liouville equation. Since the way to reduce a 6N-dimensional system to a 6-dimensional system is very similar to the way to reduce a 6-dimensional system to a 3-dimensional system, I decided to put the Chapter 4 after the derivation of fluid equations from Vlasov equations in Chapter 3.
      Chapter 5 derives the dispersion relation of the linear waves in the ion-electron two-fluid plasmas. The mobility-tensor approach makes the complete linear wave analysis in the ion-electron two-fluid plasma an easy task. I learned the mobility-tensor approach from Professor J. R. Kan. According to Professor Kan, his lecture was based on the classical book by Stix (1962). For advanced study, I recommend the students to find the numerical solutions ω(k) and plot the Friedrich's diagrams of all the wave modes based on the linear dispersion relation obtained in this chapter.
      Chapter 6 derives the dispersion relation of the linear waves in the MHD plasmas. This chapter is written based on the classical paper by Kantrowitz & Petschek (1966). I leave the Friedrich's diagrams of the MHD waves as an exercise to the students. What they leaned from the Friedrich's diagrams of the MHD waves can also help them to study the linear waves in Chapter 5.
      Chapter 7 and Appendices D & E introduce the single particle drift motions, the diamagnetic current, and the ponderomotive force. This chapter is written based on what I learned from Nicholson (1983) and with some extensions based on my own experiences in these subjects. The multiple-time-scale analysis shown in this chapter can be generalized to study wave-wave interactions at different time scales. It can also help the students to develop or to understand the gyro-kinetic simulation model. Since the gyro-kinetic model is a model in between the fluid model and the kinetic model, I put this chapter between the discussion of fluid models in Chapters 5 & 6 and the discussion of kinetic models in Chapters 8-11. Indeed, I think most of the single particle drift motions are strongly related to the kinetic plasma physics, except the diamagnetic current and the polarization drift. Therefore, I decide to put this chapter before the section of kinetic plasma physics, rather than at the beginning of this book. Examples discussed in this chapter are exclusively from space plasma physics. Instructors from different field can ignore these examples and use their own examples to demonstrate the drift motions and their consequences.
      Chapter 8 shows the possible nonlinear equilibrium solutions of the plasma distribution function with given background electric field and magnetic field. This chapter is written based on what I learned from the books by Krall & Trivelpiece (1973) and with some extensions based on my own experiences in this topic. The nonlinear equilibrium solutions discussed in this chapter are essential for studying linear waves in the kinetic plasma as discussed later in Chapters 9 and 11.
      Chapter 9 shows the importance of Landau contour in studying linear waves in the kinetic plasma and discusses the possible unstable distribution function in a spatially uniform plasma. This chapter is written based on what I learned from the books by Krall & Trivelpiece (1973) and Nicholson (1983) and with some extensions and detailed derivations based on my own experiences in this subject.
      Chapter 10 briefly describes the two-stream instability based on the classical approaches discussed in the textbooks Krall & Trivelpiece (1973) and Chen (1984). The two-stream instability is a good example of the unstable waves that could occur in a uniform medium as discussed in Chapter 9. I do not discuss the nonlinear evolution of the two-stream instability in this chapter. I recommend the students to learn the nonlinear evolution of the two-stream instability from a kinetic simulation of the two-stream instability.
      Chapter 11 derives the dispersion relation of the linear waves in unmagnetized and magnetized kinetic plasma. This chapter is written based on what I learned from the books by Krall & Trivelpiece (1973) and with some extensions and detailed derivations based on my own experiences in this subject.
    Note that, for simplicity, all the linear waves discussed in this book are assumed to propagate in a uniform equilibrium medium. A brief discussion has been made at the beginning of Chapter 5 to show the students how to linearize the governing equations when the background medium is non-uniform. Since studying the linear waves in a non-uniform medium requires the knowledge of non-uniform equilibrium solutions, which are highly nonlinear solutions, the study of linear waves in a non-uniform medium is beyond the scope of this book. It will be discussed in the advanced course of nonlinear plasma physics in the future.
      This book is a collection of the lecture notes I put on my web site during the past 10 years. The lecture notes are written for a two-semester graduate course, which I taught for nearly 20 years in National Central University. Initially, I put the lecture notes on the web so that I do not need to carry the lecture notes or the textbooks with me everywhere I go, particularly when I visit another institute or attend a conference abroad. Since these notes are initially written for myself, there are limited discussions on the physical meanings of the governing equations and the wave modes in these notes. When I finally converted them into lecture notes, I found that it is a good idea to give the students a chance to think and to find out the physical meaning of different plasma processes all by themselves. As a result, this book will provide both the students and the instructors enough freedom to use their own examples to interpret the wave modes or the governing equations without the interference from the author. Another type of information that is missing from this book is the historical review of the discovery of different wave modes. This type of information can help students to learn the importance of each wave mode.       Fortunately, nowadays, the students can easily learn the historical information by the keyword searching on the internet-based encyclopedia.
      This book is written for a two-semester graduate course. It contains only the fundamental subjects in the plasma physics. Thus, an instructor can easily cover the entire book in two semesters. I usually taught the Chapters 1-4, 6, and the first half of the Chapters 5 and 7 during the first semester. It took me about two third of the second semester to finish the Chapters 8-11. For the rest of the second semester, depending on the research background of the students in the class, I will either go back to Chapters 5 and 7 or teach some nonlinear plasma physics, which are not included in this book but can be found in textbooks elsewhere.
      In acknowledgment, I would like to thank Professor J. K. Chao of National Central University, Professor K. R. Chu of National Taiwan University (previously a professor of National Tsing Hua University for nearly 30 years), and Professor J. R. Kan of University of Alaska Fairbanks, who have shown me the beauty of the plasma physics in my early studies. I am also grateful to the students for their corrections and comments over the years. Without their help, it will be very difficult for me to find out all the typos hiding in my lecture notes.

    Ling-Hsiao Lyu
    National Central University
    December 10, 2010