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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 begin...

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Detalles Bibliográficos
Autor principal: Glatzmaier, Gary A., 1949-
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Princeton : Princeton University Press, [2014]
Colección:Book collections on Project MUSE.
Temas:
Acceso en línea:Texto completo

MARC

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020 |a 9781400848904 
020 |z 9780691141732 
020 |z 9780691141725 
040 |a MdBmJHUP  |c MdBmJHUP 
100 1 |a Glatzmaier, Gary A.,  |d 1949- 
245 1 0 |a Introduction to Modeling Convection in Planets and Stars :   |b Magnetic Field, Density Stratification, Rotation /   |c Gary A. Glatzmaier. 
264 1 |a Princeton :  |b Princeton University Press,  |c [2014] 
264 3 |a Baltimore, Md. :  |b Project MUSE,   |c 0000 
264 4 |c ©[2014] 
300 |a 1 online resource. 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
490 0 |a Princeton series in astrophysics 
500 |a Includes index. 
505 0 |a Part I. The fundamentals -- part II. Additional numerical methods -- part III. Additional physics. 
520 |a "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 "--  |c Provided by publisher. 
546 |a In English. 
588 |a Description based on print version record. 
650 7 |a Stars  |x Atmospheres.  |2 fast  |0 (OCoLC)fst01131653 
650 7 |a Planets  |x Atmospheres.  |2 fast  |0 (OCoLC)fst01065128 
650 7 |a Convection (Astrophysics)  |x Mathematical models.  |2 fast  |0 (OCoLC)fst00877134 
650 7 |a COMPUTERS  |x Data Modeling & Design.  |2 bisacsh 
650 7 |a SCIENCE  |x Astronomy.  |2 bisacsh 
650 6 |a Étoiles  |x Atmospheres. 
650 6 |a Planetes  |x Atmospheres. 
650 6 |a Convection (Astrophysique)  |x Modeles mathematiques. 
650 6 |a Convection (Astrophysique)  |x Simulation par ordinateur. 
650 0 |a Stars  |x Atmospheres. 
650 0 |a Planets  |x Atmospheres. 
650 0 |a Convection (Astrophysics)  |x Mathematical models. 
650 0 |a Convection (Astrophysics)  |x Computer simulation. 
655 0 |a Electronic book. 
655 7 |a Electronic books.   |2 local 
710 2 |a Project Muse.  |e distributor 
830 0 |a Book collections on Project MUSE. 
856 4 0 |z Texto completo  |u https://projectmuse.uam.elogim.com/book/41994/ 
945 |a Project MUSE - Custom Collection