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Computational Plasma Physics: With Applications To Fusion And Astrophysics: Frontiers in Physics

Autor Toshi Tajima
en Limba Engleză Paperback – 13 feb 2004
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.
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Specificații

ISBN-13: 9780813342115
ISBN-10: 0813342112
Pagini: 528
Dimensiuni: 156 x 234 x 30 mm
Greutate: 0.7 kg
Ediția:Revised
Editura: CRC Press
Colecția CRC Press
Seria Frontiers in Physics


Cuprins

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

Descriere

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.