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Synopsis
Most of the visible matter in the universe exists in the plasma state. Plasmas are of major importance for space physics, solar physics, and astrophysics. On Earth they are essential for magnetic controlled thermonuclear fusion.
This textbook collects lecture notes from a one-semester course taught at the K.U. Leuven to advanced undergraduate students in applied mathematics and physics. A particular strength of this book is that it provides a low threshold introduction to plasmas with an emphasis on first principles and fundamental concepts and properties.
The discussion of plasma models is to a large extent limited to Magnetohydrodynamics (MHD) with its merits and limitations clearly explained. MHD provides the students on their first encounter with plasmas, with a powerful plasma model that they can link to familiar classic fluid dynamics. The solar wind is studied as an example of hydrodynamics and MHD at work in solar physics and astrophysics.
Les informations fournies dans la section « Synopsis » peuvent faire référence à une autre édition de ce titre.
- ÉditeurSpringer-Verlag New York Inc.
- Date d'édition2003
- ISBN 10 1402014295
- ISBN 13 9781402014291
- ReliureRelié
- Langueanglais
- Nombre de pages203
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AN INTRODUCTION TO PLASMA ASTROPHYSICS AND MAGNETOHYDRODYNAMICS
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Kluwer Academic Publishers, Dordrecht, 2003
ISBN 10 : 1402014295
ISBN 13 : 9781402014291
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Hardcover. Etat : Near fine. First Edition. ".provides a low threshold introduction to plasmas with an emphasis on first principles and fundamental concepts and properties." Astrophysics and Space Science Library, Volume 294. Octavo: 203 p. with several textual figures. Original glossy boards; issued without a dust jacket. Very light bumping to the corners and tips; else a crisp and clean copy. Near fine. N° de réf. du vendeur 74787
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An Introduction To Plasma Astrophysics And Magnetohydrodynamics
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An Introduction To Plasma Astrophysics And Magnetohydrodynamics
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An Introduction to Plasma Astrophysics and Magnetohydrodynamics (Astrophysics and Space Science Library, 294)
Edité par
Springer, 2003
ISBN 10 : 1402014295
ISBN 13 : 9781402014291
Ancien ou d'occasion
Couverture rigide
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hardcover. Etat : Very Good. Hardcover shows only light cover wear. Text is unmarked and binding tight. Ships FAST! N° de réf. du vendeur 2412260055
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An Introduction to Plasma Astrophysics and Magnetohydrodynamics
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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Most of the visible matter in the universe exists in the plasma state. Plasmas are of major importance for space physics, solar physics, and astrophysics. On Earth they are essential for magnetic controlled thermonuclear fusion. This textbook coll. N° de réf. du vendeur 4092558
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An Introduction to Plasma Astrophysics and Magnetohydrodynamics
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Springer Netherlands Aug 2003, 2003
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Buch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Most of the visible matter in the universe exists in the plasma state. Plasmas are of major importance for space physics, solar physics, and astrophysics. On Earth they are essential for magnetic controlled thermonuclear fusion. This textbook collects lecture notes from a one-semester course taught at the K.U. Leuven to advanced undergraduate students in applied mathematics and physics. A particular strength of this book is that it provides a low threshold introduction to plasmas with an emphasis on first principles and fundamental concepts and properties. The discussion of plasma models is to a large extent limited to Magnetohydrodynamics (MHD) with its merits and limitations clearly explained. MHD provides the students on their first encounter with plasmas, with a powerful plasma model that they can link to familiar classic fluid dynamics. The solar wind is studied as an example of hydrodynamics and MHD at work in solar physics and astrophysics. 216 pp. Englisch. N° de réf. du vendeur 9781402014291
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An Introduction to Plasma Astrophysics and Magnetohydrodynamics
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An Introduction to Plasma Astrophysics and Magnetohydrodynamics
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Springer Netherlands, Springer Netherlands Aug 2003, 2003
ISBN 10 : 1402014295
ISBN 13 : 9781402014291
Neuf
Couverture rigide
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Buch. Etat : Neu. Neuware -Most of the visible matter in the universe exists in the plasma state. Plasmas are of major importance for space physics, solar physics, and astrophysics. On Earth they are essential for magnetic controlled thermonuclear fusion.This textbook collects lecture notes from a one-semester course taught at the K.U. Leuven to advanced undergraduate students in applied mathematics and physics. A particular strength of this book is that it provides a low threshold introduction to plasmas with an emphasis on first principles and fundamental concepts and properties.The discussion of plasma models is to a large extent limited to Magnetohydrodynamics (MHD) with its merits and limitations clearly explained. MHD provides the students on their first encounter with plasmas, with a powerful plasma model that they can link to familiar classic fluid dynamics. The solar wind is studied as an example of hydrodynamics and MHD at work in solar physics and astrophysics.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 216 pp. Englisch. N° de réf. du vendeur 9781402014291
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An Introduction to Plasma Astrophysics and Magnetohydrodynamics (Astrophysics and Space Science Library, 294)
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An Introduction to Plasma Astrophysics and Magnetohydrodynamics
Edité par
Springer Netherlands, Springer Netherlands, 2003
ISBN 10 : 1402014295
ISBN 13 : 9781402014291
Neuf
Couverture rigide
Vendeur : AHA-BUCH GmbH, Einbeck, Allemagne
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Buch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - Most of the visible matter in the universe exists in the plasma state. Plasmas are of major importance for space physics, solar physics, and astrophysics. On Earth they are essential for magnetic controlled thermonuclear fusion. This textbook collects lecture notes from a one-semester course taught at the K.U. Leuven to advanced undergraduate students in applied mathematics and physics. A particular strength of this book is that it provides a low threshold introduction to plasmas with an emphasis on first principles and fundamental concepts and properties. The discussion of plasma models is to a large extent limited to Magnetohydrodynamics (MHD) with its merits and limitations clearly explained. MHD provides the students on their first encounter with plasmas, with a powerful plasma model that they can link to familiar classic fluid dynamics. The solar wind is studied as an example of hydrodynamics and MHD at work in solar physics and astrophysics. N° de réf. du vendeur 9781402014291
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