Heliospheric propagation of galactic cosmic rays depending on the scattering characteristics of the turbulent interplanetary magnetic field.

Autor:	Shakhov, B., Kolesnik, Yu.
Zdroj:	Kinematics & Physics of Celestial Bodies; Dec2008, Vol. 24 Issue 6, p280-292, 13p
Abstrakt:	The effect of the solar wind on the spectrum of cosmic rays accelerated in the Galaxy is studied. The coefficient of cosmic-ray diffusion in the interplanetary turbulent magnetic field is assumed to be independent of the particle energy and a power-law function of the distance from the Sun. The particle spectrum at the heliospheric boundary is specified as a power-law function of the total particle energy. [ABSTRACT FROM AUTHOR]
Databáze:	Complementary Index
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