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Verlag: Springer, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
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hardcover. Zustand: Good. Ex- library book with stamps/ stickers.
Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
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Verlag: Springer, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
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Hardcover. Zustand: new.
Verlag: Springer, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
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Zustand: New.
Verlag: Springer, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
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Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
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Buch Print-on-Demand
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Verlag: Springer, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
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Buch Print-on-Demand
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Verlag: Springer Berlin Heidelberg Dez 2009, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
Anbieter: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Deutschland
Buch Print-on-Demand
Buch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Accretion flows, winds and jets of compact astrophysical objects and stars are generally described within the framework of hydrodynamical and magnetohydrodynamical (MHD) flows. Analytical analysis of the problem provides profound physical insights, which are essential for interpreting and understanding the results of numerical simulations. Providing such a physical understanding of MHD Flows in Compact Astrophysical Objects is the main goal of this book, which is an updated translation of a successful Russian graduate textbook. The book provides the first detailed introduction into the method of the Grad-Shafranov equation, describing analytically the very broad class of hydrodynamical and MHD flows. It starts with the classical examples of hydrodynamical accretion onto relativistic and nonrelativistic objects. The force-free limit of the Grad-Shafranov equation allows us to analyze in detail the physics of the magnetospheres of radio pulsars and black holes, including the Blandford-Znajek process of energy extraction from a rotating black hole immersed in an external magnetic field. Finally, on the basis of the full MHD version of the Grad-Shafranov equation the author discusses the problems of jet collimation and particle acceleration in Active Galactic Nuclei, radio pulsars, and Young Stellar Objects. The comparison of the analytical results with numerical simulations demonstrates their good agreement. Assuming that the reader is familiar with the basic physical and mathematical concepts of General Relativity, the author uses the 3+1 split approach which allows the formulation of all results in terms of physically clear language of three dimensional vectors. The book contains detailed derivations of equations, numerous exercises, and an extensive bibliography. It therefore serves as both an introductory text for graduate students and a valuable reference work for researchers in the field. 448 pp. Englisch.
Verlag: Springer, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
Anbieter: GreatBookPricesUK, Castle Donington, DERBY, Vereinigtes Königreich
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Zustand: New.
Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
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Soft Cover. Zustand: new.
Verlag: Springer Berlin Heidelberg, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
Anbieter: moluna, Greven, Deutschland
Buch Print-on-Demand
Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. A didactic approach to understanding accretion flows, winds and jets of Astrophysical Compact ObjectsAnalytical treatment of the hydrodynamic and magnetohydrodynamic problem reveals physical concepts and provides better understanding of numerical .
Verlag: Springer Berlin Heidelberg, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch
Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Accretion flows, winds and jets of compact astrophysical objects and stars are generally described within the framework of hydrodynamical and magnetohydrodynamical (MHD) flows. Analytical analysis of the problem provides profound physical insights, which are essential for interpreting and understanding the results of numerical simulations. Providing such a physical understanding of MHD Flows in Compact Astrophysical Objects is the main goal of this book, which is an updated translation of a successful Russian graduate textbook. The book provides the first detailed introduction into the method of the Grad-Shafranov equation, describing analytically the very broad class of hydrodynamical and MHD flows. It starts with the classical examples of hydrodynamical accretion onto relativistic and nonrelativistic objects. The force-free limit of the Grad-Shafranov equation allows us to analyze in detail the physics of the magnetospheres of radio pulsars and black holes, including the Blandford-Znajek process of energy extraction from a rotating black hole immersed in an external magnetic field. Finally, on the basis of the full MHD version of the Grad-Shafranov equation the author discusses the problems of jet collimation and particle acceleration in Active Galactic Nuclei, radio pulsars, and Young Stellar Objects. The comparison of the analytical results with numerical simulations demonstrates their good agreement. Assuming that the reader is familiar with the basic physical and mathematical concepts of General Relativity, the author uses the 3+1 split approach which allows the formulation of all results in terms of physically clear language of three dimensional vectors. The book contains detailed derivations of equations, numerous exercises, and an extensive bibliography. It therefore serves as both an introductory text for graduate students and a valuable reference work for researchers in the field.
Verlag: Springer Berlin Heidelberg Mrz 2012, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
Anbieter: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Deutschland
Buch Print-on-Demand
Taschenbuch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Accretion flows, winds and jets of compact astrophysical objects and stars are generally described within the framework of hydrodynamical and magnetohydrodynamical (MHD) flows. Analytical analysis of the problem provides profound physical insights, which are essential for interpreting and understanding the results of numerical simulations. Providing such a physical understanding of MHD Flows in Compact Astrophysical Objects is the main goal of this book, which is an updated translation of a successful Russian graduate textbook. The book provides the first detailed introduction into the method of the Grad-Shafranov equation, describing analytically the very broad class of hydrodynamical and MHD flows. It starts with the classical examples of hydrodynamical accretion onto relativistic and nonrelativistic objects. The force-free limit of the Grad-Shafranov equation allows us to analyze in detail the physics of the magnetospheres of radio pulsars and black holes, including the Blandford-Znajek process of energy extraction from a rotating black hole immersed in an external magnetic field. Finally, on the basis of the full MHD version of the Grad-Shafranov equation the author discusses the problems of jet collimation and particle acceleration in Active Galactic Nuclei, radio pulsars, and Young Stellar Objects. The comparison of the analytical results with numerical simulations demonstrates their good agreement. Assuming that the reader is familiar with the basic physical and mathematical concepts of General Relativity, the author uses the 3+1 split approach which allows the formulation of all results in terms of physically clear language of three dimensional vectors. The book contains detailed derivations of equations, numerous exercises, and an extensive bibliography. It therefore serves as both an introductory text for graduate students and a valuable reference work for researchers in the field. 448 pp. Englisch.
Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
Anbieter: Lucky's Textbooks, Dallas, TX, USA
Buch
Zustand: New.
Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
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Zustand: Fine. Book is in Used-LikeNew condition. Pages and cover are clean and intact. Used items may not include supplementary materials such as CDs or access codes. May show signs of minor shelf wear.
Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
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Buch
Zustand: Very Good. Book is in Used-VeryGood condition. Pages and cover are clean and intact. Used items may not include supplementary materials such as CDs or access codes. May show signs of minor shelf wear and contain very limited notes and highlighting.
Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
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Zustand: New. Buy with confidence! Book is in new, never-used condition.
Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
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Zustand: Good. Good condition. This is the average used book, that has all pages or leaves present, but may include writing. Book may be ex-library with stamps and stickers.
Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
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Buch
Zustand: New. New! This book is in the same immaculate condition as when it was published.
Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
Anbieter: Book Deals, Tucson, AZ, USA
Buch
Zustand: Fine. Like New condition. Great condition, but not exactly fully crisp. The book may have been opened and read, but there are no defects to the book, jacket or pages.
Verlag: Springer, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
Anbieter: Book Deals, Tucson, AZ, USA
Buch
Zustand: Very Good. Very Good condition. Shows only minor signs of wear, and very minimal markings inside (if any).
Verlag: Springer Berlin Heidelberg, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
Anbieter: moluna, Greven, Deutschland
Buch Print-on-Demand
Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. A didactic approach to understanding accretion flows, winds and jets of Astrophysical Compact ObjectsAnalytical treatment of the hydrodynamic and magnetohydrodynamic problem reveals physical concepts and provides better understanding of numerical .
Verlag: Springer Berlin Heidelberg, 2012
ISBN 10: 3642261779ISBN 13: 9783642261770
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch
Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Accretion flows, winds and jets of compact astrophysical objects and stars are generally described within the framework of hydrodynamical and magnetohydrodynamical (MHD) flows. Analytical analysis of the problem provides profound physical insights, which are essential for interpreting and understanding the results of numerical simulations. Providing such a physical understanding of MHD Flows in Compact Astrophysical Objects is the main goal of this book, which is an updated translation of a successful Russian graduate textbook. The book provides the first detailed introduction into the method of the Grad-Shafranov equation, describing analytically the very broad class of hydrodynamical and MHD flows. It starts with the classical examples of hydrodynamical accretion onto relativistic and nonrelativistic objects. The force-free limit of the Grad-Shafranov equation allows us to analyze in detail the physics of the magnetospheres of radio pulsars and black holes, including the Blandford-Znajek process of energy extraction from a rotating black hole immersed in an external magnetic field. Finally, on the basis of the full MHD version of the Grad-Shafranov equation the author discusses the problems of jet collimation and particle acceleration in Active Galactic Nuclei, radio pulsars, and Young Stellar Objects. The comparison of the analytical results with numerical simulations demonstrates their good agreement. Assuming that the reader is familiar with the basic physical and mathematical concepts of General Relativity, the author uses the 3+1 split approach which allows the formulation of all results in terms of physically clear language of three dimensional vectors. The book contains detailed derivations of equations, numerous exercises, and an extensive bibliography. It therefore serves as both an introductory text for graduate students and a valuable reference work for researchers in the field.
Verlag: Springer New York Jan 2016, 2016
ISBN 10: 1493935496ISBN 13: 9781493935499
Anbieter: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Deutschland
Buch Print-on-Demand
Buch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This volume extends the ISSI series on magnetic fields in the Universe into the domain of what are by far the strongest fields in the Universe, and stronger than any field that could be produced on Earth. The chapters describe the magnetic fields in non-degenerate strongly magnetized stars, in degenerate stars (such as white dwarfs and neutron stars), exotic members called magnetars, and in their environments, as well as magnetic fields in the environments of black holes. These strong fields have a profound effect on the behavior of matter, visible in particular in highly variable processes like radiation in all known wavelengths, including Gamma-Ray bursts. The generation and structure of such strong magnetic fields and effects on the environment are also described. 596 pp. Englisch.
Verlag: Springer New York Mrz 2018, 2018
ISBN 10: 1493980750ISBN 13: 9781493980758
Anbieter: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Deutschland
Buch Print-on-Demand
Taschenbuch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This volume extends the ISSI series on magnetic fields in the Universe into the domain of what are by far the strongest fields in the Universe, and stronger than any field that could be produced on Earth. The chapters describe the magnetic fields in non-degenerate strongly magnetized stars, in degenerate stars (such as white dwarfs and neutron stars), exotic members called magnetars, and in their environments, as well as magnetic fields in the environments of black holes. These strong fields have a profound effect on the behavior of matter, visible in particular in highly variable processes like radiation in all known wavelengths, including Gamma-Ray bursts. The generation and structure of such strong magnetic fields and effects on the environment are also described. 596 pp. Englisch.
Verlag: Springer New York, 2016
ISBN 10: 1493935496ISBN 13: 9781493935499
Anbieter: moluna, Greven, Deutschland
Buch Print-on-Demand
Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Describes strong magnetic fields in non-degenerate anddegenerate stars and in their environments as well as magnetic fields in the environment of black holesDetails the generation, structure and environmental effectsof strong magnetic fields.
Verlag: Springer New York, 2018
ISBN 10: 1493980750ISBN 13: 9781493980758
Anbieter: moluna, Greven, Deutschland
Buch Print-on-Demand
Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Describes strong magnetic fields in non-degenerate anddegenerate stars and in their environments as well as magnetic fields in the environment of black holesDetails the generation, structure and environmental effectsof strong magnetic fields.
Verlag: Springer, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
Anbieter: GreatBookPricesUK, Castle Donington, DERBY, Vereinigtes Königreich
Buch
Zustand: As New. Unread book in perfect condition.
Verlag: Springer, 2009
ISBN 10: 3642012892ISBN 13: 9783642012891
Anbieter: Mispah books, Redhill, SURRE, Vereinigtes Königreich
Buch
Hardcover. Zustand: Like New. Like New. book.
Verlag: Springer, 2018
ISBN 10: 1493980750ISBN 13: 9781493980758
Anbieter: GF Books, Inc., Hawthorne, CA, USA
Buch
Zustand: Fine. Book is in Used-LikeNew condition. Pages and cover are clean and intact. Used items may not include supplementary materials such as CDs or access codes. May show signs of minor shelf wear.