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0067-0057 ble 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 accelerati978-3-642-10139-7978-3-642-00309-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
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Astrophysics and Space Science Libraryhttp://image.papertrans.cn/n/image/667380.jpg
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https://doi.org/10.1007/978-3-642-00309-7Cosmic Rays; Diffusion Theory; Diffusive Shock Acceleration; Interstellar Medium; Nonlinear Transport Th
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Nonlinear Cosmic Ray Diffusion Theories978-3-642-00309-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
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Andreas ShalchiA science monograph presenting the forefront of cosmic ray diffusion theory
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0067-0057 lar 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 traje
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Book 2009of 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 reali
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