N. O. Weiss is Emeritus Professor of Mathematical Physics at the University of Cambridge and a Fellow of Clare College. He is a Fellow of the Royal Society and a former President of the Royal Astronomical Society, which awarded him a Gold Medal in 2007. His research has centred on astrophysical fluid dynamics and especially on nonlinear magnetohydrodynamic interactions between convection and magnetic fields in the Sun and other stars, as well as in the Earth.
Inhaltsangabe
Preface 1. Introduction 2. Basic MHD 3. Linearized Boussinesq magnetoconvection 4. The nonlinear regime 5. 2D Boussinesq magnetoconvection 6. 3D Boussinesq magnetoconvection 7. Magnetoconvection, rotation and the dynamo 8. Compressible magnetoconvection 9. Solar and stellar magnetic fields Appendix A. The Boussinesq and anelastic approximations Appendix B. Chaotic systems Appendix C. Double-diffusive convection Appendix D. Magnetic buoyancy and the magneto-Boussinesq approximation References Index.
Preface 1. Introduction 2. Basic MHD 3. Linearized Boussinesq magnetoconvection 4. The nonlinear regime 5. 2D Boussinesq magnetoconvection 6. 3D Boussinesq magnetoconvection 7. Magnetoconvection, rotation and the dynamo 8. Compressible magnetoconvection 9. Solar and stellar magnetic fields Appendix A. The Boussinesq and anelastic approximations Appendix B. Chaotic systems Appendix C. Double-diffusive convection Appendix D. Magnetic buoyancy and the magneto-Boussinesq approximation References Index.
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