Introduction to Modeling Convection in Planets and Stars: Magnetic Field, Density Stratification, Rotation
Gary A. Glatzmaier
ISBN 10: 069114172X ISBN 13: 9780691141725
Editore: Princeton University Press, 2013
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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. This book describes how to create codes that simulate the internal dynamics of planets and stars. Series: Princeton Series in Astrophysics. Num Pages: 328 pages, 16 color illus. 19 halftones. 23 line illus. 2 tables. BIC Classification: PBWH; PGC; PHVB. Category: (P) Professional & Vocational; (U) Tertiary Education (US: College). Dimension: 229 x 152. Weight in Grams: 685. . 2013. 1st Edition. Hardcover. . . . . Codice articolo V9780691141725
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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.
- 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
Informazioni sull?autore: Gary A. Glatzmaier is professor of earth and planetary sciences at the University of California, Santa Cruz. He is a fellow of the American Academy of Arts and Sciences and a member of the National Academy of Sciences.
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Titolo: Introduction to Modeling Convection in ...
Casa editrice: Princeton University Press
Data di pubblicazione: 2013
Legatura: Rilegato
Condizione: New
Edizione: prima edizione
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Introduction to Modeling Convection in Planets and Stars: Magnetic Field, Density Stratification, Rotation (Princeton Series in Astrophysics)
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Introduction to Modeling Convection in Planets and Stars Magnetic Field, Density Stratification, Rotation (Princeton Series in Astrophysics, 24) Glatzmaier, Gary A.
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Princeton University Press, 2013
ISBN 10: 069114172X
ISBN 13: 9780691141725
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Introduction to Modeling Convection in Planets and Stars: Magnetic Field, Density Stratification, Rotation (Princeton Series in Astrophysics)
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Princeton University Press, 2013
ISBN 10: 069114172X
ISBN 13: 9780691141725
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Introduction to Modeling Convection in Planets and Stars
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Princeton University Press, US, 2013
ISBN 10: 069114172X
ISBN 13: 9780691141725
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Hardback. Condizione: New. 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. Codice articolo LU-9780691141725
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Introduction to Modeling Convection in Planets and Stars
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Princeton University Press, US, 2013
ISBN 10: 069114172X
ISBN 13: 9780691141725
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Hardback. Condizione: New. 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. Codice articolo LU-9780691141725
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Introduction to Modeling Convection in Planets and Stars
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Princeton University Press, US, 2013
ISBN 10: 069114172X
ISBN 13: 9780691141725
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Hardback. Condizione: New. 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. Codice articolo LU-9780691141725
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Introduction to Modeling Convection in Planets and Stars
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Princeton University Press, US, 2013
ISBN 10: 069114172X
ISBN 13: 9780691141725
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Hardback. Condizione: New. 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. Codice articolo LU-9780691141725
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