Nonlinear Cosmic Ray Diffusion Theories

· Astrophysics and Space Science Library 362. књига · Springer Science & Business Media
Π•-књига
199
Π‘Ρ‚Ρ€Π°Π½ΠΈΡ†Π°
ΠžΡ†Π΅Π½Π΅ ΠΈ Ρ€Π΅Ρ†Π΅Π½Π·ΠΈΡ˜Π΅ нису Π²Π΅Ρ€ΠΈΡ„ΠΈΠΊΠΎΠ²Π°Π½Π΅ Β Π‘Π°Π·Π½Π°Ρ˜Ρ‚Π΅ вишС

О овој С-књизи

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.

ΠžΡ†Π΅Π½ΠΈΡ‚Π΅ ΠΎΠ²Ρƒ Π΅-ΠΊΡšΠΈΠ³Ρƒ

ΠˆΠ°Π²ΠΈΡ‚Π΅ Π½Π°ΠΌ својС ΠΌΠΈΡˆΡ™Π΅ΡšΠ΅.

Π˜Π½Ρ„ΠΎΡ€ΠΌΠ°Ρ†ΠΈΡ˜Π΅ ΠΎ Ρ‡ΠΈΡ‚Π°ΡšΡƒ

ΠŸΠ°ΠΌΠ΅Ρ‚Π½ΠΈ Ρ‚Π΅Π»Π΅Ρ„ΠΎΠ½ΠΈ ΠΈ Ρ‚Π°Π±Π»Π΅Ρ‚ΠΈ
Π˜Π½ΡΡ‚Π°Π»ΠΈΡ€Π°Ρ˜Ρ‚Π΅ Π°ΠΏΠ»ΠΈΠΊΠ°Ρ†ΠΈΡ˜Ρƒ Google Play књигС Π·Π° Android ΠΈ iPad/iPhone. Аутоматски сС ΡΠΈΠ½Ρ…Ρ€ΠΎΠ½ΠΈΠ·ΡƒΡ˜Π΅ са Π½Π°Π»ΠΎΠ³ΠΎΠΌ ΠΈ ΠΎΠΌΠΎΠ³ΡƒΡ›Π°Π²Π° Π²Π°ΠΌ Π΄Π° Ρ‡ΠΈΡ‚Π°Ρ‚Π΅ онлајн ΠΈ ΠΎΡ„Π»Π°Ρ˜Π½ Π³Π΄Π΅ Π³ΠΎΠ΄ Π΄Π° сС Π½Π°Π»Π°Π·ΠΈΡ‚Π΅.
Π›Π°ΠΏΡ‚ΠΎΠΏΠΎΠ²ΠΈ ΠΈ Ρ€Π°Ρ‡ΡƒΠ½Π°Ρ€ΠΈ
ΠœΠΎΠΆΠ΅Ρ‚Π΅ Π΄Π° ΡΠ»ΡƒΡˆΠ°Ρ‚Π΅ Π°ΡƒΠ΄ΠΈΠΎ-књигС ΠΊΡƒΠΏΡ™Π΅Π½Π΅ Π½Π° Google Play-Ρƒ ΠΏΠΎΠΌΠΎΡ›Ρƒ Π²Π΅Π±-ΠΏΡ€Π΅Π³Π»Π΅Π΄Π°Ρ‡Π° Π½Π° Ρ€Π°Ρ‡ΡƒΠ½Π°Ρ€Ρƒ.
Π•-Ρ‡ΠΈΡ‚Π°Ρ‡ΠΈ ΠΈ Π΄Ρ€ΡƒΠ³ΠΈ ΡƒΡ€Π΅Ρ’Π°Ρ˜ΠΈ
Π”Π° бистС Ρ‡ΠΈΡ‚Π°Π»ΠΈ Π½Π° ΡƒΡ€Π΅Ρ’Π°Ρ˜ΠΈΠΌΠ° којС користС Π΅-мастило, ΠΊΠ°ΠΎ ΡˆΡ‚ΠΎ су Kobo Π΅-Ρ‡ΠΈΡ‚Π°Ρ‡ΠΈ, Ρ‚Ρ€Π΅Π±Π° Π΄Π° ΠΏΡ€Π΅ΡƒΠ·ΠΌΠ΅Ρ‚Π΅ Ρ„Π°Ρ˜Π» ΠΈ прСнСсСтС Π³Π° Π½Π° ΡƒΡ€Π΅Ρ’Π°Ρ˜. ΠŸΡ€Π°Ρ‚ΠΈΡ‚Π΅ Π΄Π΅Ρ‚Π°Ρ™Π½Π° упутства ΠΈΠ· Ρ†Π΅Π½Ρ‚Ρ€Π° Π·Π° ΠΏΠΎΠΌΠΎΡ› Π΄Π° бистС ΠΏΡ€Π΅Π½Π΅Π»ΠΈ Ρ„Π°Ρ˜Π»ΠΎΠ²Π΅ Ρƒ ΠΏΠΎΠ΄Ρ€ΠΆΠ°Π½Π΅ Π΅-Ρ‡ΠΈΡ‚Π°Ρ‡Π΅.