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...
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Princeton
Princeton University Press
[2014]
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| Schlagworte: | |
| Zusammenfassung: | "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: | Description based on print version record |
| Beschreibung: | 1 online resource (342 pages) illustrations |
| ISBN: | 9780691141725 9780691141732 9781400848904 |
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| 100 | 1 | |a Glatzmaier, Gary A. |d 1949- |e Verfasser |4 aut | |
| 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] | |
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| 500 | |a Description based on print version record | ||
| 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 "-- | ||
| 650 | 4 | |a Mathematisches Modell | |
| 650 | 4 | |a Convection (Astrophysics) |x Computer simulation | |
| 650 | 4 | |a Convection (Astrophysics) |x Mathematical models | |
| 650 | 4 | |a Planets |x Atmospheres | |
| 650 | 4 | |a Stars |x Atmospheres | |
| 776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |a Glatzmaier, Gary A |t . Introduction to modeling convection in planets and stars : magnetic field, density stratification, rotation |
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Datensatz im Suchindex
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|---|---|
| any_adam_object | |
| author | Glatzmaier, Gary A. 1949- |
| author_facet | Glatzmaier, Gary A. 1949- |
| author_role | aut |
| author_sort | Glatzmaier, Gary A. 1949- |
| author_variant | g a g ga gag |
| building | Verbundindex |
| bvnumber | BV044063905 |
| collection | ZDB-30-PAD ZDB-38-ESG |
| ctrlnum | (ZDB-30-PAD)EBC1458382 (ZDB-89-EBL)EBL1458382 (ZDB-38-EBR)ebr10783690 (OCoLC)1165552448 (DE-599)BVBBV044063905 |
| dewey-full | 523.4 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.4 |
| dewey-search | 523.4 |
| dewey-sort | 3523.4 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| format | Electronic eBook |
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| id | DE-604.BV044063905 |
| illustrated | Illustrated |
| indexdate | 2024-07-10T07:42:34Z |
| institution | BVB |
| isbn | 9780691141725 9780691141732 9781400848904 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-029470750 |
| oclc_num | 1165552448 |
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| physical | 1 online resource (342 pages) illustrations |
| psigel | ZDB-30-PAD ZDB-38-ESG |
| publishDate | 2014 |
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| publishDateSort | 2014 |
| publisher | Princeton University Press |
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| spelling | Glatzmaier, Gary A. 1949- Verfasser aut Introduction to modeling convection in planets and stars magnetic field, density stratification, rotation Gary A. Glatzmaier Princeton Princeton University Press [2014] © 2014 1 online resource (342 pages) illustrations txt rdacontent c rdamedia cr rdacarrier Description based on print version record "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 Erscheint auch als Druck-Ausgabe Glatzmaier, Gary A . Introduction to modeling convection in planets and stars : magnetic field, density stratification, rotation |
| spellingShingle | Glatzmaier, Gary A. 1949- 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 |
| work_keys_str_mv | AT glatzmaiergarya introductiontomodelingconvectioninplanetsandstarsmagneticfielddensitystratificationrotation |