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9789048180110: 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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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.

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The Editor, Prof. S.S. Hasan is the Director of the Indian Institute of Astrophysics.

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9781402088674: 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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Hasan, S. S.|Gangadhara, R.|Krishan, V.
Publicado por Springer Netherlands (2010)
ISBN 10: 9048180112 ISBN 13: 9789048180110
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Descripción Condición: 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. Nº de ref. del artículo: 5821844

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S. S. Hasan
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ISBN 10: 9048180112 ISBN 13: 9789048180110
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Descripción Taschenbuch. Condición: 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. Nº de ref. del artículo: 9789048180110

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S. S. Hasan
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ISBN 10: 9048180112 ISBN 13: 9789048180110
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Descripción Taschenbuch. Condición: 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. Nº de ref. del artículo: 9789048180110

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Hasan, S.S. (Edited by)/ Gangadhara, R. (Edited by)/ Krishan, V. (Edited by)
Publicado por Springer (2010)
ISBN 10: 9048180112 ISBN 13: 9789048180110
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Descripción Paperback. Condición: Brand New. 342 pages. 9.00x6.00x0.84 inches. In Stock. Nº de ref. del artículo: zk9048180112

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