Physics Of Space Plasmas: An Introduction, 2nd Ed, by George Parks

In summary, "Physics Of Space Plasmas: An Introduction" by George Parks is a comprehensive textbook that covers the physics of space plasmas, incorporating new information from recent space missions. It includes topics such as electrodynamics in space, equations and definitions, magnetic and electric fields, particles in space, magnetohydrodynamic equations and concepts, planetary and stellar winds, interplanetary magnetic field, and more. The second edition also includes new material on kinetic physics and how electromagnetic fields behave in rotating frames. This book is a valuable resource for students and researchers in the field of space plasma physics.

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  • Author: George Parks
  • Title: Physics Of Space Plasmas: An Introduction
  • Amazon Link: https://www.amazon.com/dp/0813341299/?tag=pfamazon01-20
  • Prerequisities: Introductory physics, modern physics, calculus through PDEs, E&M, introductory astrophysics/astronomy (basically three years of a Physics BS program)
  • Contents: Undergraduate, upper level; Graduate, introductory

Table of Contents

Code:
1 Electrodynamics in Space
 1.1  Introduction
 1.2  Solar and Stellar Winds
 1.3  Interplanetary Magnetic Field
 1.4  Interplanetary Electric Field
 1.5  Solar and Stellar Activities
 1.6  Collisionless Shock Waves
 1.7  Magnetospheres of Cosmic Bodies
 1.8  Magnetospheres of Planets
 1.9  Heliosphere and Heliopause
 1.10 Comparative Magnetospheres
 
2 Equations and Definitions
 2.1  Introduction
 2.2  Maxwell Equations
 2.3  Lorentz Equation of Motion
 2.4  Statistical Concepts
 2.5  Statistical Equations
 2.6  Electrodyanmics in Special Theory of Relativity
 2.7  Electrodynamics in General Relativity
 2.8  Charged Particles in Space
 2.9  How to Study Plasma Phenomena in Space
 
3 Magnetic and Electric Fields in Space

 3.1  Introduction
 3.2  Representations of Magnetic Fields
 3.3  Magnetic Fields in Space
 3.4  Inhomogeneous Magnetic Fields
 3.5  Rotational Magnetic Fields
 3.6  Spinning Magnetic Dipoles
 3.7  Representations of Electric Fields
 3.8  Electric Field of Rotating Dipoles
 3.9  Plasmasphere and Plasmapause
 3.10 Concluding Remarks
 
4 Particles in Space
 4.1  Introduction
 4.2  Discovery of Earth's Radiation Belt
 4.3  Lorentz Equation of Motion
 4.4  Guiding Center Drift Equations
 4.5  Motion in an Inhomogeneous Magnetic Field
 4.6  Motion in Inhomogeneous Electric Field
 4.7  Motion in Time-Dependent Magnetic Field
 4.8  Motion in Time-Dependent Electric Field
 4.9  Ponderomotive Force
 4.10 Summary of Guiding Center Drifts and Currents
 4.11 Adiabatic Invariants
 4.12 Trapped Particles in the Magnetosphere
 4.13 Earth's Radiation Belt Particles
 4.14 Motion of Trapped Particles in Non-Dipole Field
 4.15 Particles in Magnetic Neutral Regions
 4.16 Concluding Remarks
 
5 Magnetohydrodynamic Equations and Concepts
 5.1  Introduction
 5.2  General Concepts of Fluid Dynamics
 5.3  One-Fluid Magnetohydrodynamic Equations
 5.4  Magnetic Field and MHD Fluids
 5.5  Ideal MHD Fluid (σ = ∞)
 5.6  Limitations of Ideal MHD Theory
 5.7  Flow of MHD Fluid
 5.8  Derivation of Momentum Equation
 5.9  Maxwellian Plasma
 5.10 Restrictions of MHD Fluids
 5.11 Concluding Remarks

6 Planetary and Stellar Winds and Interplanetary Magnetic Field
 6.1  Introduction
 6.2  Static Neutral Atmosphere
 6.3  Ionospheres
 6.4  The Sun and Solar Wind
 6.5  Chapman's Static Solar Wind Model
 6.6  Parker's Fluid Solar Wind Model
 6.7  Kinetic Models of Solar Wind
 6.8  Interplanetary Magnetic Field
 6.9  Interplanetary Current Sheet
 6.10 Concluding Remarks
 
7 Currents in Space
 7.1  Introduction
 7.2  Currents in Plasmas
 7.3  Diamagnetic Current
 7.4  Ring Current in Magnetospheres
 7.5  Currents in Plasmas Including Collisions
 7.6  Currents in Ionospheres
 7.7  Field-Aligned Currents
 7.8  Magnetic Tail Currents
 7.9  Concluding Remarks

8 Boundaries in Space
 8.1  Introduction
 8.2  Basic Equations and Assumptions
 8.3  Closed and Open Boundary Models
 8.4  Continuity of Momentum and Energy
 8.5  Equations of MHD Discontinuities
 8.6  Test of Theory
 8.7  Theory of Boundary Layer
 8.8  Kinetic Formulation of Boundaries
 8.9  Concluding Remarks

9 Waves in Space
 9.1  Introduction
 9.2  Electromagnetic Waves in Space
 9.3  Basic Equations and Concepts
 9.4  Electrostatic Waves
 9.5  Kinetic Theory of Electrostatic Waves
 9.6  Electrostatic Solitary Waves in Space
 9.7  Electromagnetic Waves
 9.8  Whistlers in Earth's Magnetosphere
 9.9  Kinetic Theory of Electromagnetic Waves
 9.10 Cyclotron Resonance Theory
 9.11 Theory of Auroral Kilometric Radiation
 9.12 Magnetohydrodynamic Waves
 9.13 Concluding Remarks

10 Shocks in Space
 10.1  Introduction
 10.2  Basic Concepts and Definitions
 10.3  Steeping of MHD Waves
 10.4  Shock Waves in Ordinary Fluids
 10.5  MHD Shocks
 10.6  Acceleration of Particles at Shocks
 10.7  Foreshock Particles Structure and Waves
 10.8  Structure of Weak MHD Shocks
 10.9  Kinetic Formulation of Schocks
 10.10 Concluding Remarks

11 Instabilities in Space
 11.1  Introduction
 11.2  Classification of Instabilities
 11.3  Methods of Instability Analysis
 11.4  MHD Instabilities
 11.5  Tearing Mode Instability
 11.6  Magnetospheric Substorm Instability
 11.7  Unanswered Questions
 11.8  New Spacecraft Observations
 11.9  Concluding Remarks

Appendices

A  Useful Constants and Units

B  Average Plasma Properties of Earth's Environment

C  Useful Vector and Tensor Formulas
 C.1  Vector Operations
 C.2  Change of Variables
 
D  Magnetic Indices
 D.1 A[SUB]E[/SUB] Index
 D.2 K[SUB]P[/SUB] Index
 D.3 D[SUB]st[/SUB] Index
 
Bibliograpy

Index

From Publisher
In its inaugural edition, Physics of Space Plasmas was the most widely used textbook for courses in space plasma physics, and included up-to-date observations from space available at the time. Throughout universities in the United States and abroad-it has proven itself indispensable. In the more than ten years since, an amazing number of new space plasma observations have been made. These more recent observations have revealed new and exciting information about space plasma. Now, incorporating new information from several NASA and ESA space missions, the completely revised second edition is expanded to include kinetic physics so that kinetic features in the plasma data can be explained more clearly. In addition, Parks now includes a clear and simple discussion of how electromagnetic fields behave in rotating frames. This thoroughly revised second edition retains the thoughtful examples and problems of the first edition and expands to include new examples, problem sets, schematic diagrams, and images that complement the new material.
 
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  • #2
I am only familiar with the first edition. I found it in the university library while I was taking intro plasma physics and found that it was a great resource - plus I was mostly interested in space plasmas so it was a nice supplement to the required books (intro plasma physics by Chen, and Intro plasma theory by Nicholson). In particular, I recall gaining some insight on the guiding center approach to single particle motion, as well as a nice development of the double adiabatic theory equations of state - with more insight than my professor. I also like Parks' easy discussions of basic MHD, and how he gives you some understanding of where the MHD model comes from.

I like how the book is mostly organized according to specific physical ideas: fields in space, particles in space, currents in space, etc. It help provide a unified view of the physics. In the first edition the chapters on waves and instabilities left something to be desired - the instabilities chapter was particularly weak. Hopefully the second edition has improved them. On the other hand, I liked his presentation about shocks. In addition to the basic theory the book presents a fair amount of data - mostly from spacecraft in the Earth's magnetosphere. I recall reading a good section on substorms as well.

This book works well along side the book by Kivelson and Russel. Parks is more rigorous in most sections and presents a more unified view of plasma physics, while K&R presents a lot of phenomenology and presents more unified views of things like regions of the magnetosphere. In some sense, Parks is mostly a plasma physics book that strongly emphasizes space physics, while K&R is a space physics book that presents basic plasma physics as needed along the way. I personally like Parks much more, but they both serve a purpose.

jason
 

FAQ: Physics Of Space Plasmas: An Introduction, 2nd Ed, by George Parks

1. What is the purpose of the book "Physics Of Space Plasmas: An Introduction, 2nd Ed, by George Parks"?

The purpose of this book is to provide a comprehensive introduction to the physics of space plasmas, which are ionized gases found in the space environment. It covers a wide range of topics including plasma physics, magnetohydrodynamics, and the interactions between plasma and electromagnetic fields.

2. Who is the target audience for this book?

This book is primarily aimed at students and researchers in the fields of space physics, astrophysics, and plasma physics. However, it can also be a valuable resource for anyone with a general interest in the physics of space plasmas.

3. What makes this book unique compared to other textbooks on space plasmas?

This book stands out for its clear and concise explanations of complex concepts, as well as its inclusion of recent research and developments in the field. It also includes numerous examples and exercises to help readers deepen their understanding of the material.

4. Is this book suitable for self-study?

Yes, this book can be used for self-study as it is well-organized and includes a variety of resources such as exercises, solutions, and further reading suggestions. However, it is recommended to have a basic understanding of physics and mathematics before diving into this book.

5. Are there any prerequisites for reading this book?

While there are no strict prerequisites, a basic understanding of calculus and classical mechanics would be beneficial. Some familiarity with electromagnetism and thermodynamics would also be helpful, but not necessary.

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