Introduction to Modeling Convection in Planets and Stars

Magnetic Field, Density Stratification, Rotation

Nonfiction, Science & Nature, Science, Physics, Mathematical Physics, Astrophysics & Space Science
Cover of the book Introduction to Modeling Convection in Planets and Stars by Gary A. Glatzmaier, Princeton University Press
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Author: Gary A. Glatzmaier ISBN: 9781400848904
Publisher: Princeton University Press Publication: November 24, 2013
Imprint: Princeton University Press Language: English
Author: Gary A. Glatzmaier
ISBN: 9781400848904
Publisher: Princeton University Press
Publication: November 24, 2013
Imprint: Princeton University Press
Language: English

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 accurate numerical methods and more realistic geometries in two and three dimensions. In the third part of the book, Glatzmaier demonstrates how to incorporate more sophisticated physics, including the effects of magnetic field, density stratification, and rotation.

Featuring numerous exercises throughout, this is an ideal textbook for students and an essential resource for researchers.

  • Describes how to create codes that simulate the internal dynamics of planets and stars
  • Builds on basic concepts and simple methods
  • Shows how to improve the efficiency and accuracy of the numerical methods
  • Describes more relevant geometries and boundary conditions
  • Demonstrates how to incorporate more sophisticated physics
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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 accurate numerical methods and more realistic geometries in two and three dimensions. In the third part of the book, Glatzmaier demonstrates how to incorporate more sophisticated physics, including the effects of magnetic field, density stratification, and rotation.

Featuring numerous exercises throughout, this is an ideal textbook for students and an essential resource for researchers.

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