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Synopsis
I have felt the need for a book on the theory of solar magnetic fields for some time now. Most books about the Sun are written by observers or by theorists from other branches of solar physics, whereas those on magnetohydrodynamics do not deal extensively with solar applications. I had thought of waiting a few decades before attempting to put pen to paper, but one summer Josip Kleczek encouraged an im- mediate start 'while your ideas are still fresh'. The book grew out of a postgraduate lecture course at St Andrews, and the resulting period of gestation or 'being with monograph' has lasted several years. The Sun is an amazing object, which has continued to reveal completely unexpected features when observed in greater detail or at new wavelengths. What riches would be in store for us if we could view other stars with as much precision! Stellar physics itself is benefiting greatly from solar discoveries, but, in tum, our understanding of many solar phenomena (such as sunspots, sunspot cycles, the corona and the solar wind) will undoubtedly increase in the future due to their observation under different conditions in other stars. In the 'old days' the solar atmosphere was regarded as a static, plane-parallel structure, heated by the dissipation of sound waves and with its upper layer expanding in a spherically symmetric manner as the solar wind. Outside of sunspots the magnetic field was thOUght to be unimportant with a weak uniform value of a few gauss.
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Solar Magnetohydrodynamics
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D. Reidel, 1984
ISBN 10 : 9027718334
ISBN 13 : 9789027718334
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Etat : Very Good. 500 pp., hardcover, previous owner's name to front pastedown, a small inscription to rear pastedown else very good in a chipped and lightly worn dust jacket. - If you are reading this, this item is actually (physically) in our stock and ready for shipment once ordered. We are not bookjackers. Buyer is responsible for any additional duties, taxes, or fees required by recipient's country. N° de réf. du vendeur ZB1332647
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Solar Magnetohydrodynamics (Volume 21)
Edité par
D. Reidel Publishing Company, 2000
ISBN 10 : 9027718334
ISBN 13 : 9789027718334
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Couverture souple
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Etat : Fair. Volume 21. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. In fair condition, suitable as a study copy. Library sticker on front cover. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,850grams, ISBN:9789027718334. N° de réf. du vendeur 9997080
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Solar Magnetohydrodynamics
Edité par
D. Reidel Publishing, 1984
ISBN 10 : 9027718334
ISBN 13 : 9789027718334
Ancien ou d'occasion
Softcover
Vendeur : curtis paul books, inc., Northridge, CA, Etats-Unis
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Softcover. Etat : Very Good+. Second Edition. Paperback shows light wear to edges and some fading to spine. PON (mathematician Paul H. Roberts) inside front cover. ; Geophysics And Astrophysics Monographs, 21; 9.2 X 6.1 X 1.3 inches. N° de réf. du vendeur 38803
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Solar Magnetohydrodynamics
Edité par
D. Reidel Publishing Company, 2000
ISBN 10 : 9027718334
ISBN 13 : 9789027718334
Ancien ou d'occasion
Couverture souple
Vendeur : Anybook.com, Lincoln, Royaume-Uni
Évaluation du vendeur 5 sur 5 étoiles
Etat : Good. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. In good all round condition. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,1000grams, ISBN:9789027718334. N° de réf. du vendeur 9093733
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Solar Magnetohydrodynamics (Geophysics and Astrophysics Monographs, 21)
Edité par
Springer, 1984
ISBN 10 : 9027718334
ISBN 13 : 9789027718334
Ancien ou d'occasion
Paperback
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Paperback. Etat : Good. Connecting readers with great books since 1972! Used textbooks may not include companion materials such as access codes, etc. May have some wear or writing/highlighting. We ship orders daily and Customer Service is our top priority! N° de réf. du vendeur S_332388193
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Solar Magnetohydrodynamics
Edité par
Springer Netherlands, 1984
ISBN 10 : 9027718334
ISBN 13 : 9789027718334
Neuf
Kartoniert / Broschiert
Vendeur : moluna, Greven, Allemagne
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Kartoniert / Broschiert. Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. I have felt the need for a book on the theory of solar magnetic fields for some time now. Most books about the Sun are written by observers or by theorists from other branches of solar physics, whereas those on magnetohydrodynamics do not deal extensively w. N° de réf. du vendeur 5814993
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Solar Magnetohydrodynamics (Geophysics and Astrophysics Monographs, 21)
Vendeur : Ria Christie Collections, Uxbridge, Royaume-Uni
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Etat : New. In. N° de réf. du vendeur ria9789027718334_new
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Solar Magnetic Hydrodynamics
Vendeur : GreatBookPrices, Columbia, MD, Etats-Unis
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Etat : New. N° de réf. du vendeur 3351734-n
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Solar Magnetohydrodynamics (Paperback)
Edité par
Springer, Dordrecht, 1984
ISBN 10 : 9027718334
ISBN 13 : 9789027718334
Neuf
Paperback
Edition originale
Vendeur : Grand Eagle Retail, Bensenville, IL, Etats-Unis
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Paperback. Etat : new. Paperback. I have felt the need for a book on the theory of solar magnetic fields for some time now. Most books about the Sun are written by observers or by theorists from other branches of solar physics, whereas those on magnetohydrodynamics do not deal extensively with solar applications. I had thought of waiting a few decades before attempting to put pen to paper, but one summer Josip Kleczek encouraged an im mediate start 'while your ideas are still fresh'. The book grew out of a postgraduate lecture course at St Andrews, and the resulting period of gestation or 'being with monograph' has lasted several years. The Sun is an amazing object, which has continued to reveal completely unexpected features when observed in greater detail or at new wavelengths. What riches would be in store for us if we could view other stars with as much precision! Stellar physics itself is benefiting greatly from solar discoveries, but, in tum, our understanding of many solar phenomena (such as sunspots, sunspot cycles, the corona and the solar wind) will undoubtedly increase in the future due to their observation under different conditions in other stars. In the 'old days' the solar atmosphere was regarded as a static, plane-parallel structure, heated by the dissipation of sound waves and with its upper layer expanding in a spherically symmetric manner as the solar wind. Outside of sunspots the magnetic field was thOUght to be unimportant with a weak uniform value of a few gauss. Stellar physics itself is benefiting greatly from solar discoveries, but, in tum, our understanding of many solar phenomena (such as sunspots, sunspot cycles, the corona and the solar wind) will undoubtedly increase in the future due to their observation under different conditions in other stars. Shipping may be from multiple locations in the US or from the UK, depending on stock availability. N° de réf. du vendeur 9789027718334
Quantité disponible : 1 disponible(s)
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Solar Magnetohydrodynamics
Edité par
Springer Netherlands Jul 1984, 1984
ISBN 10 : 9027718334
ISBN 13 : 9789027718334
Neuf
Taschenbuch
Vendeur : BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Allemagne
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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -I have felt the need for a book on the theory of solar magnetic fields for some time now. Most books about the Sun are written by observers or by theorists from other branches of solar physics, whereas those on magnetohydrodynamics do not deal extensively with solar applications. I had thought of waiting a few decades before attempting to put pen to paper, but one summer Josip Kleczek encouraged an im mediate start 'while your ideas are still fresh'. The book grew out of a postgraduate lecture course at St Andrews, and the resulting period of gestation or 'being with monograph' has lasted several years. The Sun is an amazing object, which has continued to reveal completely unexpected features when observed in greater detail or at new wavelengths. What riches would be in store for us if we could view other stars with as much precision! Stellar physics itself is benefiting greatly from solar discoveries, but, in tum, our understanding of many solar phenomena (such as sunspots, sunspot cycles, the corona and the solar wind) will undoubtedly increase in the future due to their observation under different conditions in other stars. In the 'old days' the solar atmosphere was regarded as a static, plane-parallel structure, heated by the dissipation of sound waves and with its upper layer expanding in a spherically symmetric manner as the solar wind. Outside of sunspots the magnetic field was thOUght to be unimportant with a weak uniform value of a few gauss. 500 pp. Englisch. N° de réf. du vendeur 9789027718334
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