The study of precession-driven flows in ellipsoidal containers has excited over the years a great although not constant interest. The first investigations related to this matter date back to Poincare' (1910). After Poincare', geophysics was the main motivation for further investigations on precession driven flows in connection with the origin of the Earth's magnetic field (Bullard, 1949). Nowadays it is generally accepted that the Earth's magnetic field is generated by motions in the liquid outer core, but the details of this process are still matter of investigation. The generation of magnetic fields by motions in an electrically conducting fluid is called dynamo action. Most geophysicists regard convection driven by thermal or chemical buoyancy as the most likely source of energy for the geodynamo, but the possibility of a dynamo driven by the Earth's precession cannot be rejected. The research work presented in this book intends to examine the fluid motions existing in precessing ellipsoidal cavities and eventually investigate whether the generated velocity fields are suitable to support dynamo action.
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Dr. Silvia Lorenzani is Assistant Professor at the Politecnico di Milano. She graduated at the University of Bologna in Theoretical Physics and obtained the PhD degree from the University of Goettingen. She is the author of several articles in the field of turbulence, hydrodynamic instabilities and rarefied gas dynamics.
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Taschenbuch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The study of precession-driven flows in ellipsoidal containers has excited over the years a great although not constant interest. The first investigations related to this matter date back to Poincare' (1910). After Poincare', geophysics was the main motivation for further investigations on precession driven flows in connection with the origin of the Earth's magnetic field (Bullard, 1949). Nowadays it is generally accepted that the Earth's magnetic field is generated by motions in the liquid outer core, but the details of this process are still matter of investigation. The generation of magnetic fields by motions in an electrically conducting fluid is called dynamo action. Most geophysicists regard convection driven by thermal or chemical buoyancy as the most likely source of energy for the geodynamo, but the possibility of a dynamo driven by the Earth's precession cannot be rejected. The research work presented in this book intends to examine the fluid motions existing in precessing ellipsoidal cavities and eventually investigate whether the generated velocity fields are suitable to support dynamo action. 144 pp. Englisch. Bestandsnummer des Verkäufers 9783846540015
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Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Lorenzani SilviaDr. Silvia Lorenzani is Assistant Professor at the Politecnico di Milano. She graduated at the University of Bologna in Theoretical Physics and obtained the PhD degree from the University of Goettingen. She is the aut. Bestandsnummer des Verkäufers 5497708
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Taschenbuch. Zustand: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - The study of precession-driven flows in ellipsoidal containers has excited over the years a great although not constant interest. The first investigations related to this matter date back to Poincare' (1910). After Poincare', geophysics was the main motivation for further investigations on precession driven flows in connection with the origin of the Earth's magnetic field (Bullard, 1949). Nowadays it is generally accepted that the Earth's magnetic field is generated by motions in the liquid outer core, but the details of this process are still matter of investigation. The generation of magnetic fields by motions in an electrically conducting fluid is called dynamo action. Most geophysicists regard convection driven by thermal or chemical buoyancy as the most likely source of energy for the geodynamo, but the possibility of a dynamo driven by the Earth's precession cannot be rejected. The research work presented in this book intends to examine the fluid motions existing in precessing ellipsoidal cavities and eventually investigate whether the generated velocity fields are suitable to support dynamo action. Bestandsnummer des Verkäufers 9783846540015
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Taschenbuch. Zustand: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The study of precession-driven flows in ellipsoidal containers has excited over the years a great although not constant interest. The first investigations related to this matter date back to Poincare' (1910). After Poincare', geophysics was the main motivation for further investigations on precession driven flows in connection with the origin of the Earth's magnetic field (Bullard, 1949). Nowadays it is generally accepted that the Earth's magnetic field is generated by motions in the liquid outer core, but the details of this process are still matter of investigation. The generation of magnetic fields by motions in an electrically conducting fluid is called dynamo action. Most geophysicists regard convection driven by thermal or chemical buoyancy as the most likely source of energy for the geodynamo, but the possibility of a dynamo driven by the Earth's precession cannot be rejected. The research work presented in this book intends to examine the fluid motions existing in precessing ellipsoidal cavities and eventually investigate whether the generated velocity fields are suitable to support dynamo action.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 144 pp. Englisch. Bestandsnummer des Verkäufers 9783846540015
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Taschenbuch. Zustand: Neu. Fluid instabilities in precessing ellipsoidal shells | Theoretical background and numerical modeling | Silvia Lorenzani | Taschenbuch | 144 S. | Englisch | 2012 | LAP LAMBERT Academic Publishing | EAN 9783846540015 | Verantwortliche Person für die EU: BoD - Books on Demand, In de Tarpen 42, 22848 Norderstedt, info[at]bod[dot]de | Anbieter: preigu. Bestandsnummer des Verkäufers 106572444
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