Hugendubel.info - Die B2B Online-Buchhandlung 

Merkliste
Die Merkliste ist leer.
Bitte warten - die Druckansicht der Seite wird vorbereitet.
Der Druckdialog öffnet sich, sobald die Seite vollständig geladen wurde.
Sollte die Druckvorschau unvollständig sein, bitte schliessen und "Erneut drucken" wählen.
E-BookPDF2 - DRM Adobe / Adobe Ebook ReaderE-Book
356 Seiten
Englisch
Wiley-VCHerschienen am31.08.20131. Auflage
In this work the authors draw upon their expertise in geophysical and astrophysical MHD to explore the motion of electrically conducting fluids, the so-called dynamo effect, and describe the similarities and differences between different magnetized objects. They also explain why magnetic fields are crucial to the formation of the stars, and discuss promising experiments currently being designed to investigate some of the relevant physics in the laboratory. This interdisciplinary approach will appeal to a wide audience in physics, astrophysics and geophysics.
This second edition covers such additional topics as small-scale dynamos, while also presenting the latest results and experiments.


Gunther Rudiger is Professor at the Leibniz Institute for Astrophysics Potsdam, and lectured at the University of Potsdam. He has also worked at the University of Gottingen and is a former Visiting Professor at the University of Newcastle upon Tyne. For the successful
collaboration with the Helmholtz-Center Dresden-Rossendorf regarding the magnetorotational instability experiment PROMISE he was awarded the 2008 Science Prize of the Donor Federation of German Science.
Rainer Hollerbach received his Ph.D. from the University of California, San Diego. He is currently Visiting Professor in the Institute of Geophysics at ETH
Zurich, as part of the European Research Council project ?Magnetostrophic Flow in Experiments and the Core of the
Earth?. He is permanently based in the Department of Applied Mathematics at the University of Leeds, England. He is a Fellow of the American Geophysical Union and the UK Institute of Physics.
Leonid L. Kitchatinov received his Ph.D. from the Ioffe Physical Technical Institute, St Petersburg. He is permanently affiliated to the Institute of Solar-Terrestrial Physics, Irkutsk, and to the Pulkovo
Observatory, St Petersburg. He has repeatedly worked at the Leibniz Institute for Astrophysics Potsdam, supported by both the Deutsche Forschungsgemeinschaft
and by the Alexander von Humboldt Foundation as a Research Fellow for a year. He has also worked at the
University of St Andrews, UK.
mehr
Verfügbare Formate
E-BookPDF2 - DRM Adobe / Adobe Ebook ReaderE-Book
EUR142,99
E-BookEPUB2 - DRM Adobe / EPUBE-Book
EUR142,99

Produkt

KlappentextIn this work the authors draw upon their expertise in geophysical and astrophysical MHD to explore the motion of electrically conducting fluids, the so-called dynamo effect, and describe the similarities and differences between different magnetized objects. They also explain why magnetic fields are crucial to the formation of the stars, and discuss promising experiments currently being designed to investigate some of the relevant physics in the laboratory. This interdisciplinary approach will appeal to a wide audience in physics, astrophysics and geophysics.
This second edition covers such additional topics as small-scale dynamos, while also presenting the latest results and experiments.


Gunther Rudiger is Professor at the Leibniz Institute for Astrophysics Potsdam, and lectured at the University of Potsdam. He has also worked at the University of Gottingen and is a former Visiting Professor at the University of Newcastle upon Tyne. For the successful
collaboration with the Helmholtz-Center Dresden-Rossendorf regarding the magnetorotational instability experiment PROMISE he was awarded the 2008 Science Prize of the Donor Federation of German Science.
Rainer Hollerbach received his Ph.D. from the University of California, San Diego. He is currently Visiting Professor in the Institute of Geophysics at ETH
Zurich, as part of the European Research Council project ?Magnetostrophic Flow in Experiments and the Core of the
Earth?. He is permanently based in the Department of Applied Mathematics at the University of Leeds, England. He is a Fellow of the American Geophysical Union and the UK Institute of Physics.
Leonid L. Kitchatinov received his Ph.D. from the Ioffe Physical Technical Institute, St Petersburg. He is permanently affiliated to the Institute of Solar-Terrestrial Physics, Irkutsk, and to the Pulkovo
Observatory, St Petersburg. He has repeatedly worked at the Leibniz Institute for Astrophysics Potsdam, supported by both the Deutsche Forschungsgemeinschaft
and by the Alexander von Humboldt Foundation as a Research Fellow for a year. He has also worked at the
University of St Andrews, UK.
Details
Weitere ISBN/GTIN9783527648955
ProduktartE-Book
EinbandartE-Book
FormatPDF
FormatFormat mit automatischem Seitenumbruch (reflowable)
Verlag
Erscheinungsjahr2013
Erscheinungsdatum31.08.2013
Auflage1. Auflage
Seiten356 Seiten
SpracheEnglisch
Dateigrösse30524 Kbytes
Artikel-Nr.2913461
Rubriken
Genre9201

Inhalt/Kritik

Inhaltsverzeichnis
1. Differential Rotation of Stars
2. Radiation Zones: Magnetic Stability and Rotation
3. Quasilinear Theory of Driven Turbulence
4. The Galactic Dynamo
5. The Magneto-Rotational Instability (MRI)
6. The Tayler Instability (TI)
7. Magnetic Spherical Couette Flow
mehr