The Magnetic Universe
Geophysical and Astrophysical Magnetodynamics and Dynamo Theory
(Sprache: Englisch)
Magnetism is one of the most pervasive features of the Universe, with planets, stars and entire galaxies all having associated magnetic fields. All of these fields are generated by the motion of electrically conducting fluids, the so-called dynamo effect.
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Magnetism is one of the most pervasive features of the Universe, with planets, stars and entire galaxies all having associated magnetic fields. All of these fields are generated by the motion of electrically conducting fluids, the so-called dynamo effect.
Klappentext zu „The Magnetic Universe “
Ausgehend von den Begriffen der Magnetohydrodynamik entwickeln die Autoren Konzepte, Experimente und Berechnungen zur Sternen- und Planetenentstehung, dem galaktischen Dynamo und zu starken kosmischen Magnetfeldern. Die Gültigkeit dieser Simulationen und Algorithmen für die moderne Astrophysik kann durch aktuelle experimentelle Ergebnisse gezeigt werden. Eine umfassende Darstellung des Fachgebiets, dass sich an Astro- und Geophysiker, Wissenschaftler und Studenten gleichermaßen richtet.
Ausgehend von den Begriffen der Magnetohydrodynamik entwickeln die Autoren Konzepte, Experimente und Berechnungen zur Sternen- und Planetenentstehung, dem galaktischen Dynamo und zu starken kosmischen Magnetfeldern. Die Gültigkeit dieser Simulationen und Algorithmen für die moderne Astrophysik kann durch aktuelle experimentelle Ergebnisse gezeigt werden. Eine umfassende Darstellung des Fachgebiets, dass sich an Astro- und Geophysiker, Wissenschaftler und Studenten gleichermaßen richtet.
Magnetism is one of the most pervasive features of the Universe, with planets, stars and entire galaxies all having associated magnetic fields. All of these fields are generated by the motion of electrically conducting fluids, the so-called dynamo effect. The precise details of what drives the motion, and indeed what the fluid consists of, differ widely though. In this work the authors draw upon their expertise in geophysical and astrophysical MHD to explore some of these phenomena, and describe the similarities and differences between different magnetized objects. They also explain why magnetic fields are crucial in the formation of the stars, and discuss promising experiments currently being designed to study some of the relevant physics in the laboratory. This interdisciplinary approach makes the book appealing to a wide audience in physics, astrophysics and geophysics
Magnetism is one of the most pervasive features of the Universe, with planets, stars and entire galaxies all having associated magnetic fields. All of these fields are generated by the motion of electrically conducting fluids, the so-called dynamo effect. The precise details of what drives the motion, and indeed what the fluid consists of, differ widely though. In this work the authors draw upon their expertise in geophysical and astrophysical MHD to explore some of these phenomena, and describe the similarities and differences between different magnetized objects. They also explain why magnetic fields are crucial in the formation of the stars, and discuss promising experiments currently being designed to study some of the relevant physics in the laboratory. This interdisciplinary approach makes the book appealing to a wide audience in physics, astrophysics and geophysics
Inhaltsverzeichnis zu „The Magnetic Universe “
IntroductionEarth and Planets
Differential Rotation Theory
The Stellar Dynamo
The Magnetorotational Instability
The Galactic Dynamo
Neutron Star MagnetismThe Magnetic Taylor-Couette Flow
Autoren-Porträt von Günther Rüdiger, Rainer Hollerbach
Guenther Ruediger received his PhD from the University of Jena, Germany. He is Professor at the Astrophysical Institute Potsdam, and lectures at the University of Potsdam. He worked at the University of Goettingen, and the High Altitude Observatory in Boulder, Colorado. He is also a former visiting professor at the University of Newcastle upon Tyne, England.Rainer Hollerbach is Reader in Applied Mathematics at the University of Glasgow, Scotland. He has a PhD in Geophysics from the University of California, San Diego. He recently spent a year in Germany as a Research Fellow of the Alexander von Humboldt Foundation.
Bibliographische Angaben
- Autoren: Günther Rüdiger , Rainer Hollerbach
- 2004, 1. Auflage, XI, 332 Seiten, 31 farbige Abbildungen, 161 Schwarz-Weiß-Abbildungen, Maße: 17,9 x 24,6 cm, Gebunden, Englisch
- Verlag: Wiley-VCH
- ISBN-10: 3527404090
- ISBN-13: 9783527404094
- Erscheinungsdatum: 24.06.2004
Sprache:
Englisch
Pressezitat
"Researchers and advanced students will greatly profit from this book."Rainer Beck, Max-Planck-Institut für Radioastronomie, Bonn
"The authors do a good job of conveying the excitement of the subject and of bringing together much of the research of important topics, a welcome addition to the bookshelves."
The Observatory
"Ruediger and Hollerbach have brought together the significant research on this topic ... will be of interest to both the geophysicist and the astro-physicist, and perhaps the physicist or engineer ..."
E-STREAMS
"... does contain many deep insights and there is valuable material...that is not easily accessible elsewhere.."
Geophysical and Astrophysical Fluid Dynamics
"...a valuable book to have and study...an encyclopedic guide to some of the most interesting problems in astrophysics...should be savored over many sittings."
Physics Today
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