.png){kind=logo}
24%OFF
Stock image for illustration purposes only - book cover, edition or condition may vary.
Introduction to Modeling Convection in Planets and Stars: Magnetic Field, Density Stratification, Rotation
Gary A. Glatzmaier
€ 140.31
€ 106.53
FREE Delivery in Ireland
Description for Introduction to Modeling Convection in Planets and Stars: Magnetic Field, Density Stratification, Rotation
Hardback. 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.
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 ... Read more
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 ... Read more
Product Details
Format
Hardback
Publication date
2013
Publisher
Princeton University Press United States
Number of pages
344
Condition
New
Series
Princeton Series in Astrophysics
Number of Pages
328
Place of Publication
New Jersey, United States
ISBN
9780691141725
SKU
V9780691141725
Shipping Time
Usually ships in 7 to 11 working days
Ref
99-1
About Gary A. Glatzmaier
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.
Reviews for 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. It is very useful for readers having a basic understanding of classical physics, vector calculus, partial differential equations, and simple computer programming."
Claudia-Veronika Meister, Zentralblatt MATH
Claudia-Veronika Meister, Zentralblatt MATH