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Verlag: Kluwer Academic Publishers, Dordrecht, 2002
ISBN 10: 1402006950ISBN 13: 9781402006951
Anbieter: johnson rare books & archives, ABAA, Covina, CA, USA
Buch
Hardcover. Zustand: Very good. Second Edition. "This thoroughly revised textbook is a basic introduction to plasma phenomena in solar and stellar coronae emphasizing non-MHD aspects." Astrophysics and Space Science Library, Volume 279. Octavo: 301 p. with textual figures and tables. Original glossy boards; issued without a dust jacket. Mild bumping to the corners and tips; else a crisp and clean copy. Better than very good.
Verlag: Springer, 2002
ISBN 10: 1402006950ISBN 13: 9781402006951
Anbieter: Lucky's Textbooks, Dallas, TX, USA
Buch
Zustand: New.
Verlag: Springer, 2002
ISBN 10: 1402006950ISBN 13: 9781402006951
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
Buch Print-on-Demand
Zustand: New. PRINT ON DEMAND Book; New; Fast Shipping from the UK. No. book.
Verlag: Springer Netherlands Jun 2002, 2002
ISBN 10: 1402006950ISBN 13: 9781402006951
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 textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to observational astronomers, graduate students, and advanced undergraduates without a ba- ground in plasma physics. Coronal physics is today a vast field with many different aims and goals. So- ing out the really important aspects of an observed phenomenon and using the physics best suited for the case is a formidable problem. There are already several excellent books, oriented toward the interests of astrophysicists, that deal with the magnetohydrodynamics of stellar atmospheres, radiation transport, and radiation theory. In kinetic processes, the different particle velocities play an important role. This is the case when particle collisions can be neglected, for example in very brief phenomena - such as one period of a high-frequency wave - or in effects produced by energetic particles with very long collision times. Some of the most persistent problems of solar physics, like coronal heating, shock waves, flare energy release, and particle acceleration, are likely to be at least partially related to such p- cesses. Study of the Sun is not regarded here as an end in itself, but as the source of information for more general stellar applications. Our understanding of stellar processes relies heavily, in turn, on our understanding of solar processes. Thus an introduction to what is happening in hot, dilute coronae necessarily starts with the plasma physics of our nearest star. 332 pp. Englisch.
Verlag: Springer Netherlands, 2002
ISBN 10: 1402006950ISBN 13: 9781402006951
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. This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to observational astronomers, graduate students, and advanced undergraduates without a ba- ground in plasma physi.
Verlag: Springer Netherlands, 2002
ISBN 10: 1402006950ISBN 13: 9781402006951
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch
Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to observational astronomers, graduate students, and advanced undergraduates without a ba- ground in plasma physics. Coronal physics is today a vast field with many different aims and goals. So- ing out the really important aspects of an observed phenomenon and using the physics best suited for the case is a formidable problem. There are already several excellent books, oriented toward the interests of astrophysicists, that deal with the magnetohydrodynamics of stellar atmospheres, radiation transport, and radiation theory. In kinetic processes, the different particle velocities play an important role. This is the case when particle collisions can be neglected, for example in very brief phenomena - such as one period of a high-frequency wave - or in effects produced by energetic particles with very long collision times. Some of the most persistent problems of solar physics, like coronal heating, shock waves, flare energy release, and particle acceleration, are likely to be at least partially related to such p- cesses. Study of the Sun is not regarded here as an end in itself, but as the source of information for more general stellar applications. Our understanding of stellar processes relies heavily, in turn, on our understanding of solar processes. Thus an introduction to what is happening in hot, dilute coronae necessarily starts with the plasma physics of our nearest star.
Verlag: Springer, 2002
ISBN 10: 1402006950ISBN 13: 9781402006951
Anbieter: Books Puddle, New York, NY, USA
Buch
Zustand: New. pp. 324 2nd Edition.
Verlag: Springer, 2002
ISBN 10: 1402006950ISBN 13: 9781402006951
Anbieter: Majestic Books, Hounslow, Vereinigtes Königreich
Buch Print-on-Demand
Zustand: New. Print on Demand pp. 324 Illus.