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 ?… Mehr…
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. Books > Physics eBook, Springer Shop<
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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 ?… Mehr…
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., Springer<
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Physics; Astrophysics and Astroparticles; Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics); Particle and Nuclear Physics; Particle Acceleration and Detection, Beam Physics; Atoms and Molecules in Strong Fields, Laser Matter Interaction; Plasma Physics Cosmic Rays, Diffusion Theory, Diffusive Shock Acceleration, Interstellar Medium, Nonlinear Transport Theory, Plasma, Quasilinear Transport Theory, Solar Wind, stellar Books eBook, Springer Shop<
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This book deals with the physics of cosmic ray diffusion theory, focusing on the physics of nonlinear transport of cosmic rays through turbulent interplanetary or interstellar plasma. The author proposes future research that could advance the field. Versandkosten:zzgl. Versandkosten. Details...
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This book deals with the physics of cosmic ray diffusion theory, focusing on the physics of nonlinear transport of cosmic rays through turbulent interplanetary or interstellar plasma. The… Mehr…
This book deals with the physics of cosmic ray diffusion theory, focusing on the physics of nonlinear transport of cosmic rays through turbulent interplanetary or interstellar plasma. The author proposes future research that could advance the field.; PDF; Scientific, Technical and Medical > Physics > Atomic & molecular physics, Springer Berlin Heidelberg<
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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 ?… Mehr…
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. Books > Physics eBook, Springer Shop<
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 ?… Mehr…
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., Springer<
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Physics; Astrophysics and Astroparticles; Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics); Particle and Nuclear Physics; Particle Acceleration and … Mehr…
Physics; Astrophysics and Astroparticles; Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics); Particle and Nuclear Physics; Particle Acceleration and Detection, Beam Physics; Atoms and Molecules in Strong Fields, Laser Matter Interaction; Plasma Physics Cosmic Rays, Diffusion Theory, Diffusive Shock Acceleration, Interstellar Medium, Nonlinear Transport Theory, Plasma, Quasilinear Transport Theory, Solar Wind, stellar Books eBook, Springer Science+Business Media<
- This book deals with the physics of cosmic ray diffusion theory, focusing on the physics of nonlinear transport of cosmic rays through turbulent interplanetary or interstellar plasma. The author proposes future research that could advance the field. Versandkosten: EUR 0.00
Physics; Astrophysics and Astroparticles; Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics); Particle and Nuclear Physics; Particle Acceleration and … Mehr…
Physics; Astrophysics and Astroparticles; Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics); Particle and Nuclear Physics; Particle Acceleration and Detection, Beam Physics; Atoms and Molecules in Strong Fields, Laser Matter Interaction; Plasma Physics Cosmic Rays, Diffusion Theory, Diffusive Shock Acceleration, Interstellar Medium, Nonlinear Transport Theory, Plasma, Quasilinear Transport Theory, Solar Wind, stellar Books eBook, Springer Shop<
- This book deals with the physics of cosmic ray diffusion theory, focusing on the physics of nonlinear transport of cosmic rays through turbulent interplanetary or interstellar plasma. The author proposes future research that could advance the field. Versandkosten:zzgl. Versandkosten.
This book deals with the physics of cosmic ray diffusion theory, focusing on the physics of nonlinear transport of cosmic rays through turbulent interplanetary or interstellar plasma. The… Mehr…
This book deals with the physics of cosmic ray diffusion theory, focusing on the physics of nonlinear transport of cosmic rays through turbulent interplanetary or interstellar plasma. The author proposes future research that could advance the field.; PDF; Scientific, Technical and Medical > Physics > Atomic & molecular physics, Springer Berlin Heidelberg<
- No. 9783642003097. Versandkosten:Instock, Despatched same working day before 3pm, zzgl. Versandkosten.
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Detailangaben zum Buch - Nonlinear Cosmic Ray Diffusion Theories
EAN (ISBN-13): 9783642003097 ISBN (ISBN-10): 3642003095 Erscheinungsjahr: 2009 Herausgeber: Springer Berlin 199 Seiten Sprache: eng/Englisch
Buch in der Datenbank seit 2010-07-05T21:48:11+02:00 (Zurich) Detailseite zuletzt geändert am 2023-11-28T11:51:18+01:00 (Zurich) ISBN/EAN: 3642003095
ISBN - alternative Schreibweisen: 3-642-00309-5, 978-3-642-00309-7 Alternative Schreibweisen und verwandte Suchbegriffe: Titel des Buches: ray
Daten vom Verlag:
Autor/in: Andreas Shalchi Titel: Astrophysics and Space Science Library; Nonlinear Cosmic Ray Diffusion Theories Verlag: Springer; Springer Berlin 199 Seiten Erscheinungsjahr: 2009-06-04 Berlin; Heidelberg; DE Sprache: Englisch 96,29 € (DE) 99,00 € (AT) 118,00 CHF (CH) Available XIII, 199 p. 49 illus.
EA; E107; eBook; Nonbooks, PBS / Physik, Astronomie/Astronomie; Astrophysik; Verstehen; Cosmic Rays; Diffusion Theory; Diffusive Shock Acceleration; Interstellar Medium; Nonlinear Transport Theory; Plasma; Quasilinear Transport Theory; Solar Wind; stellar; C; Astrophysics; Space Physics; Nuclear and Particle Physics; Accelerator Physics; Atoms and molecules in external fields; Plasma Physics; Physics and Astronomy; Angewandte Physik; Sonnensystem: Sonne und Planeten; Physik; Teilchen- und Hochenergiephysik; Atom- und Molekularphysik; Plasmaphysik; BB
The General scenario.- On Astrophysical Turbulence.- The Quasilinear Theory.- The Nonlinear Guiding Center Theory.- The Weakly Nonlinear Theory.- The Second-Order QLT.- The Extended Nonlinear Guiding Center Theory.- Applications.- Summary and Outlook. A science monograph presenting the forefront of cosmic ray diffusion theory
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