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Synopsis
It is well established and appreciated by now that more than 99% of the baryonic matter in the universe is in the plasma state. Most astrophysical systems could be approximated as conducting fluids in a gravitational field. It is the combined effect of these two that gives rise to the mind boggling variety of configurations in the form of filaments, loops, jets and arches. The plasma structures that cannot last for more than a second or less in a laboratory remain intact for astronomical time and spatial scales in an astrophysical setting. The case in point is the well known extragalactic jets whose collimation and stability has remained an enigma inspite of the efforts of many for many long years. The high energy radiation sources such as the active galactic nuclei again summon the coherent plasma radiation processes for their exceptionally large output from regions of relatively small physical sizes. The generation of magnetic field, anomalous transport of angular momentum with decisive bearing on star formation processes, the ubiquitous MHD turbulence under conditions irreproducible in terrestrial laboratories are some of the generic issues still awaiting a concerted effort for their understanding. Quantum Plasmas, pair plasmas and pair-ion plasmas exist under extreme conditions in planetary interiors and exotic stars. In this workshop plasma physicists, astrophysicists and plasma astrophysicists are brought together to discuss these issues.
Les informations fournies dans la section « Synopsis » peuvent faire référence à une autre édition de ce titre.
À propos de l'auteur
The Editor, Prof. S.S. Hasan is the Director of the Indian Institute of Astrophysics.
Les informations fournies dans la section « A propos du livre » peuvent faire référence à une autre édition de ce titre.
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Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes (eng)
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Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes
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Springer Netherlands, 2010
ISBN 10 : 9048180112
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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Provides and up to date review of the fieldEach chapter presents research problems and contains a pedagogical componentThe Editor, Prof. S.S. Hasan is the Director of the Indian Institute of Astrophysics.It is well established and a. N° de réf. du vendeur 5821844
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Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes
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Springer Netherlands Okt 2010, 2010
ISBN 10 : 9048180112
ISBN 13 : 9789048180110
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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -It is well established and appreciated by now that more than 99% of the baryonic matter in the universe is in the plasma state. Most astrophysical systems could be approximated as conducting fluids in a gravitational field. It is the combined effect of these two that gives rise to the mind boggling variety of configurations in the form of filaments, loops, jets and arches. The plasma structures that cannot last for more than a second or less in a laboratory remain intact for astronomical time and spatial scales in an astrophysical setting. The case in point is the well known extragalactic jets whose collimation and stability has remained an enigma inspite of the efforts of many for many long years. The high energy radiation sources such as the active galactic nuclei again summon the coherent plasma radiation processes for their exceptionally large output from regions of relatively small physical sizes. The generation of magnetic field, anomalous transport of angular momentum with decisive bearing on star formation processes, the ubiquitous MHD turbulence under conditions irreproducible in terrestrial laboratories are some of the generic issues still awaiting a concerted effort for their understanding. Quantum Plasmas, pair plasmas and pair-ion plasmas exist under extreme conditions in planetary interiors and exotic stars. In this workshop plasma physicists, astrophysicists and plasma astrophysicists are brought together to discuss these issues. 356 pp. Englisch. N° de réf. du vendeur 9789048180110
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Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes | First Kodai-Trieste Workshop on Plasma Astrophysics held at the Kodaikanal Observatory, India, August 27 - September 7, 2007
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Taschenbuch. Etat : Neu. Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes | First Kodai-Trieste Workshop on Plasma Astrophysics held at the Kodaikanal Observatory, India, August 27 - September 7, 2007 | S. S. Hasan (u. a.) | Taschenbuch | Astrophysics and Space Science Proceedings | xiii | Englisch | 2010 | Springer | EAN 9789048180110 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. N° de réf. du vendeur 107168302
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Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes : First Kodai-Trieste Workshop on Plasma Astrophysics held at the Kodaikanal Observatory, India, August 27 - September 7, 2007
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Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - It is well established and appreciated by now that more than 99% of the baryonic matter in the universe is in the plasma state. Most astrophysical systems could be approximated as conducting fluids in a gravitational field. It is the combined effect of these two that gives rise to the mind boggling variety of configurations in the form of filaments, loops, jets and arches. The plasma structures that cannot last for more than a second or less in a laboratory remain intact for astronomical time and spatial scales in an astrophysical setting. The case in point is the well known extragalactic jets whose collimation and stability has remained an enigma inspite of the efforts of many for many long years. The high energy radiation sources such as the active galactic nuclei again summon the coherent plasma radiation processes for their exceptionally large output from regions of relatively small physical sizes. The generation of magnetic field, anomalous transport of angular momentum with decisive bearing on star formation processes, the ubiquitous MHD turbulence under conditions irreproducible in terrestrial laboratories are some of the generic issues still awaiting a concerted effort for their understanding. Quantum Plasmas, pair plasmas and pair-ion plasmas exist under extreme conditions in planetary interiors and exotic stars. In this workshop plasma physicists, astrophysicists and plasma astrophysicists are brought together to discuss these issues. N° de réf. du vendeur 9789048180110
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Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes
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Springer, Springer Okt 2010, 2010
ISBN 10 : 9048180112
ISBN 13 : 9789048180110
Neuf
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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -It is well established and appreciated by now that more than 99% of the baryonic matter in the universe is in the plasma state. Most astrophysical systems could be approximated as conducting fluids in a gravitational field. It is the combined effect of these two that gives rise to the mind boggling variety of configurations in the form of filaments, loops, jets and arches. The plasma structures that cannot last for more than a second or less in a laboratory remain intact for astronomical time and spatial scales in an astrophysical setting. The case in point is the well known extragalactic jets whose collimation and stability has remained an enigma inspite of the efforts of many for many long years. The high energy radiation sources such as the active galactic nuclei again summon the coherent plasma radiation processes for their exceptionally large output from regions of relatively small physical sizes. The generation of magnetic field, anomalous transport of angular momentum with decisive bearing on star formation processes, the ubiquitous MHD turbulence under conditions irreproducible in terrestrial laboratories are some of the generic issues still awaiting a concerted effort for their understanding. Quantum Plasmas, pair plasmas and pair-ion plasmas exist under extreme conditions in planetary interiors and exotic stars. In this workshop plasma physicists, astrophysicists and plasma astrophysicists are brought together to discuss these issues.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 356 pp. Englisch. N° de réf. du vendeur 9789048180110
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Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes: First Kodai-Trieste Workshop on Plasma Astrophysics held at the . (Astrophysics and Space Science Proceedings)
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