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Nonlinear Cosmic Ray Diffusion Theories (Hardcover, 2009 ed.)
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Nonlinear Cosmic Ray Diffusion Theories (Hardcover, 2009 ed.)
Series: Astrophysics and Space Science Library, 362
Expected to ship within 10 - 15 working days
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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 ?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.
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