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.
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.
Editor's Foreword Foreword Preface Introduction Finite Size Particle Method Time Integration Grid Method Electromagnetic Model Magnetohydro-Dynamic Model of Plasmas Guiding-Center Method Hybrid Models of Plasmas Implicit Particle Codes Geometry Information and Computation Interaction between Radiation and A Plasma Drift Waves And Plasma Turbulence Magnetic Reconnection Transport Epilogue: Numerical Laboratory Credits
Editor's Foreword Foreword Preface Introduction Finite Size Particle Method Time Integration Grid Method Electromagnetic Model Magnetohydro-Dynamic Model of Plasmas Guiding-Center Method Hybrid Models of Plasmas Implicit Particle Codes Geometry Information and Computation Interaction between Radiation and A Plasma Drift Waves And Plasma Turbulence Magnetic Reconnection Transport Epilogue: Numerical Laboratory Credits
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