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Condizione: Wie neu. Condizione sovraccoperta: Sehr guter Umschlag. 0 123 S. mit zahlreichen Lithos, unbenutzt, 350 g schwer, P-2. W.Clemann/C.A.Mann/K.-H.Radler/H.Meyer (Lithos) (illustratore).

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Hardback. Condizione: New. Reprint 2024. No detailed description available for "Mean-Field Magnetohydrodynamics and Dynamo Theory".

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Hardcover. Condizione: Brand New. reprint edition. 272 pages. 6.14x0.75x9.21 inches. In Stock.

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M. 11 Abb. 25 S. OBr. (DAW. Sitzungsberichte d. Klasse f. Mathematik, Physik u. Technik, 1963/1) Sprache: Deutsch 0 gr.

Hardback. Condizione: New. Reprint 2024. No detailed description available for "Mean-Field Magnetohydrodynamics and Dynamo Theory".

Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - This IAU-symposium was the first which was entirely dedicated to dynamo processes, which are fundamental on all cosmical scales. Dynamo theory concerns one of the few truly key questions of recent cosmic physics. There is increasing evidence for the magnetic character of most short-term activity phenomena in astrophysics. Obviously, the tria. ngle 'gravil;y, nuclea. r power, magnetism' dictates cosmic evolution over a very broad scale of magnitudes. A complicated interplay of rotation, magnetism and turbulence, that is hard to resolve, determines stellar and galactic activity for almost all the short and medium time scales. Behind these multiform phenomena, the cosmic dynamo works in various guise. . 'I, all involving inductive and dissipative equilibria in rotating turbulent cosmic plasmas. The Sun, representing the cosmic dynamo par excellence, stands from the be ginning at the centre of interest for those who followed the dynamo idea. Even the first models were able to present an explanation of the typical structural appear ance of the solar magnetic field, i. e. a 22 year cycle, activit. y belts and their zonal migration, antisymmetry of t. he magnetic polarity. However, the solar dynamo still provides topics of further discussions, since confrontation with recent observational data raised and stoill raises new questions, nOll of whicll have yet found a plausible answer. These questions represent a challenge for the development of the basic the ories: Understanding of turbulence, especially Ilsing methods of modern nonlinear physics. Numerical simulations arc promising in the ncar future. …

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Couverture souple. Condizione: bon. R260269812: 1993. In-8. Broché. Très bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 499 pages augmentées de quelques figures en noir et blanc dans texte. . . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.

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Buch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - The 157th IAU Symposium on `The Cosmic Dynamo' was the first which was entirely dedicated to dynamo processes, which are fundamental on all cosmic scales. Dynamo theory concerns one of the few truly key questions of recent cosmic physics. A complicated interplay of rotation, magnetism and turbulence determines stellar and galactic activity for almost all the short and medium time scales. Behind these multiform phenomena, the cosmic dynamo works in various guises, all involving inductive and dissipative equilibria in rotating turbulent cosmic plasmas. This book presents an up-to-date survey on investigations and results of dynamo theory and related observations, and is intended for graduate scientists working in the field of cosmical magnetism and the related problems, especially convection, turbulence and, more general, nonlinear physics.…

Condizione: New. The 157th IAU Symposium on `The Cosmic Dynamo was the first which was entirely dedicated to dynamo processes, which are fundamental on all cosmic scales. Dynamo theory concerns one of the few truly key questions of recent cosmic physics. A complicated inte.

Hardcover. Condizione: Brand New. 532 pages. 10.00x6.75x1.25 inches. In Stock.

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Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. No detailed description available for Mean-Field Magnetohydrodynamics and Dynamo Theory .

Taschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This IAU-symposium was the first which was entirely dedicated to dynamo processes, which are fundamental on all cosmical scales. Dynamo theory concerns one of the few truly key questions of recent cosmic physics. There is increasing evidence for the magnetic character of most short-term activity phenomena in astrophysics. Obviously, the tria. ngle 'gravil;y, nuclea. r power, magnetism' dictates cosmic evolution over a very broad scale of magnitudes. A complicated interplay of rotation, magnetism and turbulence, that is hard to resolve, determines stellar and galactic activity for almost all the short and medium time scales. Behind these multiform phenomena, the cosmic dynamo works in various guise. . 'I, all involving inductive and dissipative equilibria in rotating turbulent cosmic plasmas. The Sun, representing the cosmic dynamo par excellence, stands from the be ginning at the centre of interest for those who followed the dynamo idea. Even the first models were able to present an explanation of the typical structural appear ance of the solar magnetic field, i. e. a 22 year cycle, activit. y belts and their zonal migration, antisymmetry of t. he magnetic polarity. However, the solar dynamo still provides topics of further discussions, since confrontation with recent observational data raised and stoill raises new questions, nOll of whicll have yet found a plausible answer. These questions represent a challenge for the development of the basic the ories: Understanding of turbulence, especially Ilsing methods of modern nonlinear physics. Numerical simulations arc promising in the ncar future. 532 pp. Englisch.…

Kartoniert / Broschiert. Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the 157th Symposium of the International Astronomical Union held in Potsdam, Germany, September 7--11, 1992 Preface. 1. The Solar Dynamo. 2. Long-Term Variability of the Solar Magnetic Cycle. 3. Numerical Simulations of Convecti. …

Buch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -No detailed description available for 'Mean-Field Magnetohydrodynamics and Dynamo Theory'.De Gruyter Mouton, Genthiner Straße 13, 10785 Berlin 272 pp. Englisch.

Taschenbuch. Condizione: Neu. The Cosmic Dynamo | Proceedings of the 157th Symposium of the International Astronomical Union, Held in Potsdam, Germany, September 7-11, 1992 | F. Krause (u. a.) | Taschenbuch | xxxii | Englisch | 1993 | Springer | EAN 9780792325475 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu Print on Demand. …

Taschenbuch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -Preface. 1. The Solar Dynamo. 2. Long-Term Variability of the Solar Magnetic Cycle. 3. Numerical Simulations of Convection and Dynamo Processes. 4. Late-Type and Other Stars. 5. Magnetic Field Generation in Accretion Disks. 6. General Aspects of Dynamo Theory. 7. Magnetic Fields in Galaxies: Observations. 8. Magnetic Fields in Galaxies: Dynamo Theory. 9. Magnetohydrodynamic Phenomena in the Interstellar Medium Related to Dynamo Processes. 10. Geodynamo and Planetary Dynamos. 11. History.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 532 pp. Englisch.…

Buch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The 157th IAU Symposium on `The Cosmic Dynamo' was the first which was entirely dedicated to dynamo processes, which are fundamental on all cosmic scales. Dynamo theory concerns one of the few truly key questions of recent cosmic physics. A complicated interplay of rotation, magnetism and turbulence determines stellar and galactic activity for almost all the short and medium time scales. Behind these multiform phenomena, the cosmic dynamo works in various guises, all involving inductive and dissipative equilibria in rotating turbulent cosmic plasmas. This book presents an up-to-date survey on investigations and results of dynamo theory and related observations, and is intended for graduate scientists working in the field of cosmical magnetism and the related problems, especially convection, turbulence and, more general, nonlinear physics. 532 pp. Englisch.…