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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...

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Detalles Bibliográficos
Autor principal: Glatzmaier, Gary
Lenguaje:eng
Publicado: Princeton University Press 2013
Materias:
Acceso en línea:http://cds.cern.ch/record/1985442
Descripción
Sumario: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 offering a step-by-step guide on how to design codes for simulating nonlinear time-dependent thermal convection in a two-dimensional box using Fourier expansions in the horizontal direction and finite differences in the vertical direction. He then describes how to implement more efficient and accura