Parallel and Perpendicular Transport of Heliospheric Cosmic Rays in an Improved Dynamical Turbulence Model

Details Parallel and Perpendicular Transport of Heliospheric Cosmic Rays in an Improved Dynamical Turbulence Model Parallel and Perpendicular Transport of Heliospheric Cosmic Rays in an Improved Dynamical Turbulence Model

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006apj...642..230s&link_type=abstract

The Astrophysical Journal, Volume 642, Issue 1, pp. 230-243.

Astronomy and Astrophysics

Astronomy

51

Ism: Cosmic Rays, Diffusion, Turbulence

Scientific paper

By applying a new model for the dynamical magnetic turbulence, we calculate parallel and perpendicular mean free paths of heliospheric cosmic rays. The results are compared with different observations and previous theoretical calculations. It is the main conclusion of this paper that we can achieve agreement between theory and observations if we employ realistic turbulence parameters. Motivated by previous work, we also discuss nonlinear effects in cosmic-ray transport theory.

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