Introduction to modeling convection in planets and stars: magnetic field, density stratification, rotation
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Princeton
Princeton University Press
[2014]
|
| Schriftenreihe: | Princeton series in astrophysics
|
| Schlagworte: | |
| Online-Zugang: | FAB01 FAW01 FCO01 FHA01 FKE01 FLA01 UPA01 Volltext |
| Beschreibung: | Includes bibliographical references and index "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 "-- |
| Beschreibung: | 1 Online-Ressource (342 pages) |
| ISBN: | 9781400848904 |
| DOI: | 10.1515/9781400848904 |
Internformat
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| 650 | 4 | |a Planets |x Atmospheres | |
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Datensatz im Suchindex
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| author | Glatzmaier, Gary A. |
| author_facet | Glatzmaier, Gary A. |
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| author_variant | g a g ga gag |
| building | Verbundindex |
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| dewey-full | 523.4 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
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| dewey-search | SCI005000 523.4 |
| dewey-sort | 3523.4 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1515/9781400848904 |
| format | Electronic eBook |
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| institution | BVB |
| isbn | 9781400848904 |
| language | English |
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| publishDate | 2014 |
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| spelling | Glatzmaier, Gary A. Verfasser aut Introduction to modeling convection in planets and stars magnetic field, density stratification, rotation Gary A. Glatzmaier Princeton Princeton University Press [2014] 1 Online-Ressource (342 pages) txt rdacontent c rdamedia cr rdacarrier Princeton series in astrophysics Includes bibliographical references and index "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 "-- Mathematisches Modell Convection (Astrophysics) Computer simulation Convection (Astrophysics) Mathematical models Planets Atmospheres Stars Atmospheres https://doi.org/10.1515/9781400848904 Verlag Volltext |
| spellingShingle | Glatzmaier, Gary A. Introduction to modeling convection in planets and stars magnetic field, density stratification, rotation Mathematisches Modell Convection (Astrophysics) Computer simulation Convection (Astrophysics) Mathematical models Planets Atmospheres Stars Atmospheres |
| title | Introduction to modeling convection in planets and stars magnetic field, density stratification, rotation |
| title_auth | Introduction to modeling convection in planets and stars magnetic field, density stratification, rotation |
| title_exact_search | Introduction to modeling convection in planets and stars magnetic field, density stratification, rotation |
| title_full | Introduction to modeling convection in planets and stars magnetic field, density stratification, rotation Gary A. Glatzmaier |
| title_fullStr | Introduction to modeling convection in planets and stars magnetic field, density stratification, rotation Gary A. Glatzmaier |
| title_full_unstemmed | Introduction to modeling convection in planets and stars magnetic field, density stratification, rotation Gary A. Glatzmaier |
| title_short | Introduction to modeling convection in planets and stars |
| title_sort | introduction to modeling convection in planets and stars magnetic field density stratification rotation |
| title_sub | magnetic field, density stratification, rotation |
| topic | Mathematisches Modell Convection (Astrophysics) Computer simulation Convection (Astrophysics) Mathematical models Planets Atmospheres Stars Atmospheres |
| topic_facet | Mathematisches Modell Convection (Astrophysics) Computer simulation Convection (Astrophysics) Mathematical models Planets Atmospheres Stars Atmospheres |
| url | https://doi.org/10.1515/9781400848904 |
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