Articoli correlati a Magnetohydrodynamics of the Sun
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This advanced textbook reviews the complex interaction between the Sun's plasma atmosphere and its magnetic field.
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Informazioni sull?autore
Eric Priest completed his PhD thesis with T. G. Cowling at Leeds in 1969, having moved to a tenured position at St Andrews University in 1968. He gradually built up an internationally renowned Solar MHD group there and is now a highly active Emeritus Professor. He has edited fifteen books and written over 450 research papers. His book Solar Magnetohydrodynamics (1982) became a standard text in the field and has been completely rewritten from scratch to be reborn as Magnetohydrodynamics of the Sun. Honours include being elected a Fellow of the Royal Society (2002) and being awarded the Hale Prize of the American Astronomical Society (2002) and the Gold Medal of the Royal Astronomical Society (2009).
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- EditoreCambridge University Press
- Data di pubblicazione2014
- ISBN 10 0521854717
- ISBN 13 9780521854719
- RilegaturaCopertina rigida
- LinguaInglese
- Numero di pagine576
- Contatto del produttorenon disponibile
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Magnetohydrodynamics of the Sun
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Cambridge University Press, 2014
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ISBN 13: 9780521854719
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Gebunden. Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. This advanced textbook provides a detailed account of our progress towards answering many key unsolved puzzles in solar physics. Developed for a graduate course, is essential reading for graduate students and researchers in solar physics, astronomy, plasma . Codice articolo 594765213
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Magnetohydrodynamics of the Sun (Hardcover)
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ISBN 10: 0521854717
ISBN 13: 9780521854719
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Hardcover. Condizione: new. Hardcover. Magnetohydrodynamics of the Sun is a completely new up-to-date rewrite from scratch of the 1982 book Solar Magnetohydrodynamics, taking account of enormous advances in understanding since that date. It describes the subtle and complex interaction between the Sun's plasma atmosphere and its magnetic field, which is responsible for many fascinating dynamic phenomena. Chapters cover the generation of the Sun's magnetic field by dynamo action, magnetoconvection and the nature of photospheric flux tubes such as sunspots, the heating of the outer atmosphere by waves or reconnection, the structure of prominences, the nature of eruptive instability and magnetic reconnection in solar flares and coronal mass ejections, and the acceleration of the solar wind by reconnection or wave-turbulence. It is essential reading for graduate students and researchers in solar physics and related fields of astronomy, plasma physics and fluid dynamics. Problem sets and other resources are available at This advanced textbook provides a detailed account of our progress towards answering many key unsolved puzzles in solar physics. Developed for a graduate course, is essential reading for graduate students and researchers in solar physics, astronomy, plasma physics and fluid dynamics. Problem sets and other resources are available at Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability. Codice articolo 9780521854719
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Magnetohydrodynamics of the Sun
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ISBN 13: 9780521854719
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Magnetohydrodynamics of the Sun (Hardcover)
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Cambridge University Press, Cambridge, 2014
ISBN 10: 0521854717
ISBN 13: 9780521854719
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Hardcover. Condizione: new. Hardcover. Magnetohydrodynamics of the Sun is a completely new up-to-date rewrite from scratch of the 1982 book Solar Magnetohydrodynamics, taking account of enormous advances in understanding since that date. It describes the subtle and complex interaction between the Sun's plasma atmosphere and its magnetic field, which is responsible for many fascinating dynamic phenomena. Chapters cover the generation of the Sun's magnetic field by dynamo action, magnetoconvection and the nature of photospheric flux tubes such as sunspots, the heating of the outer atmosphere by waves or reconnection, the structure of prominences, the nature of eruptive instability and magnetic reconnection in solar flares and coronal mass ejections, and the acceleration of the solar wind by reconnection or wave-turbulence. It is essential reading for graduate students and researchers in solar physics and related fields of astronomy, plasma physics and fluid dynamics. Problem sets and other resources are available at This advanced textbook provides a detailed account of our progress towards answering many key unsolved puzzles in solar physics. Developed for a graduate course, is essential reading for graduate students and researchers in solar physics, astronomy, plasma physics and fluid dynamics. Problem sets and other resources are available at Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability. Codice articolo 9780521854719
Quantità: 1 disponibili