Introduction to Modeling Convection in Planets and Stars : Magnetic Field, Density Stratification, Rotation /
This book provides readers with the skills they need to write computer codes that simulate convection, internal gravity waves, and magnetic field generation in the interiors and atmospheres of rotating planets and stars. Using a teaching method perfected in the classroom, Gary Glatzmaier begins by o...
Clasificación: | Libro Electrónico |
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Autor principal: | |
Formato: | Electrónico eBook |
Idioma: | Inglés |
Publicado: |
Princeton, NJ :
Princeton University Press,
[2013]
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Edición: | Course Book |
Colección: | Princeton Series in Astrophysics ;
24 |
Temas: | |
Acceso en línea: | Texto completo Texto completo |
Tabla de Contenidos:
- Frontmatter
- Contents
- Preface
- PART 1. The Fundamentals
- Chapter One. A Model of Rayleigh-Bénard Convection
- Chapter Two. Numerical Method
- Chapter Three. Linear Stability Analysis
- Chapter Four. Nonlinear Finite-Amplitude Dynamics
- Chapter Five. Postprocessing
- Chapter Six. Internal Gravity Waves
- Chapter Seven. Double-Diffusive Convection
- PART 2. Additional Numerical Methods
- Chapter Eight. Time Integration Schemes
- Chapter Nine. Spatial Discretizations
- Chapter Ten. Boundaries and Geometries
- PART 3. Additional Physics
- Chapter Eleven. Magnetic Field
- Chapter Twelve. Density Stratification
- Chapter Thirteen. Rotation
- Appendix A. A Tridiagonal Matrix Solver
- Appendix B. Making Computer-Graphical Movies
- Appendix C. Legendre Functions and the Gaussian Quadrature
- Appendix D. Parallel Processing: OpenMP
- Appendix E. Parallel Processing: MPI
- Bibliography
- Index