ABSTRACT

The physics of plasmas is an extremely rich and complex subject as the variety of topics addressed in this book demonstrates. This richness and complexity demands new and powerful techniques for investigating plasma physics. An outgrowth from his graduate course teaching, now with corrections, Tajima's text provides not only a lucid introduction to computational plasma physics, but also offers the reader many examples of the way numerical modeling, properly handled, can provide valuable physical understanding of the nonlinear aspects so often encountered in both laboratory and astrophysical plasmas. Included here are computational methods for modern nonlinear physics as applied to hydrodynamic turbulence, solitons, fast reconnection of magnetic fields, anomalous transports, dynamics of the sun, and more. The text contains examples of problems now solved using computational techniques including those concerning finite-size particles, spectral techniques, implicit differencing, gyrokinetic approaches, and particle simulation.

chapter 1|36 pages

Introduction

chapter 2|14 pages

Finite Size Particle Method

chapter 3|23 pages

Time Integration

chapter 4|31 pages

Grid Method

chapter 5|31 pages

Electromagnetic Model

chapter 6|53 pages

Magnetohydro-Dynamic Model of Plasmas

chapter 7|38 pages

Guiding-Center Method

chapter 8|11 pages

Hybrid Models of Plasmas

chapter 9|30 pages

Implicit Particle Codes

chapter 10|30 pages

Geometry

chapter 11|35 pages

Information and Computation

chapter 12|34 pages

Interaction between Radiation and A Plasma

chapter 13|38 pages

Drift Waves And Plasma Turbulence

chapter 14|52 pages

Magnetic Reconnection

chapter 15|29 pages

Transport

chapter |2 pages

Epilogue: Numerical Laboratory