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Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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hardcover. Zustand: Good. Ex-library copy with usual markings.
Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Hardcover. Zustand: new.
Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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ISBN 10: 3642003087ISBN 13: 9783642003080
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Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Zustand: Good. Good condition. This is the average used book, that has all pages or leaves present, but may include writing. Book may be ex-library with stamps and stickers.
Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Verlag: Springer Berlin Heidelberg Jun 2009, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Buch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -If charged particles move through the interplanetary or interstellar medium, they interact with a large-scale magnetic eld such as the magnetic eld of the Sun or the Galactic magnetic eld. As these background elds are usually nearly constant in time and space, they can be approximated by a homogeneous eld. If there are no additional elds, the particle trajectory is a perfect helix along which the par- cle moves at a constant speed. In reality, however, there are turbulent electric and magnetic elds dueto the interstellaror solar wind plasma. These elds lead to sc- tering of the cosmic rays parallel and perpendicular to the background eld. These scattering effects, which usually are of diffusive nature, can be described by s- tial diffusion coef cients or, alternatively, by mean free paths. The knowledge of these parameters is essential for describing cosmic ray propagation as well as d- fusive shock acceleration. The latter process is responsible for the high cosmic ray energies that have been observed. The layout of this book is as follows. In Chap. 1, the general physical scenario is presented. We discuss fundamental processes such as cosmic ray propagation and acceleration in different systems such as the solar system or the interst- lar space. These processes are a consequence of the interaction between charged cosmic particles and an astrophysical plasma (turbulence). The properties of such plasmas are therefore the subject of Chap. 2. 216 pp. Englisch.
Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Zustand: As New. Unread book in perfect condition.
Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Verlag: Springer Berlin, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Zustand: Sehr gut. 2009. Neubindung, Buchschnitt verkürzt, Ausgabe 2009 5172324/12.
Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Verlag: Springer Berlin Heidelberg, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Buch Print-on-Demand
Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. A science monograph presenting the forefront of cosmic ray diffusion theoryIf charged particles move through the interplanetary or interstellar medium, they interact with a large-scale magnetic ?eld such as the magnetic ?eld of the Sun or the Gal.
Verlag: Springer Berlin Heidelberg, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch
Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - If charged particles move through the interplanetary or interstellar medium, they interact with a large-scale magnetic eld such as the magnetic eld of the Sun or the Galactic magnetic eld. As these background elds are usually nearly constant in time and space, they can be approximated by a homogeneous eld. If there are no additional elds, the particle trajectory is a perfect helix along which the par- cle moves at a constant speed. In reality, however, there are turbulent electric and magnetic elds dueto the interstellaror solar wind plasma. These elds lead to sc- tering of the cosmic rays parallel and perpendicular to the background eld. These scattering effects, which usually are of diffusive nature, can be described by s- tial diffusion coef cients or, alternatively, by mean free paths. The knowledge of these parameters is essential for describing cosmic ray propagation as well as d- fusive shock acceleration. The latter process is responsible for the high cosmic ray energies that have been observed. The layout of this book is as follows. In Chap. 1, the general physical scenario is presented. We discuss fundamental processes such as cosmic ray propagation and acceleration in different systems such as the solar system or the interst- lar space. These processes are a consequence of the interaction between charged cosmic particles and an astrophysical plasma (turbulence). The properties of such plasmas are therefore the subject of Chap. 2.
Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
Anbieter: GreatBookPricesUK, Castle Donington, DERBY, Vereinigtes Königreich
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Zustand: As New. Unread book in perfect condition.
Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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Verlag: Springer, 2009
ISBN 10: 3642003087ISBN 13: 9783642003080
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