Parallel and perpendicular transport of cosmic rays in the heliosphere

Details Parallel and perpendicular transport of cosmic rays in the heliosphere Parallel and perpendicular transport of cosmic rays in the heliosphere

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..858..207s&link_type=abstract

PHYSICS OF THE INNER HELIOSHEATH: Voyager Observations, Theory, and Future Prospects; 5th Annual IGPP International Astrophysics

Astronomy and Astrophysics

Astrophysics

Particle Acceleration, Energetic Particles

Scientific paper

A key problem of cosmic ray astrophysics is the explanation of measured parallel and perpendicular mean free paths in the heliosphere. Previous approaches used quasilinear theory in combination with simple turbulence models to reproduce heliospheric observations. Because of recent progress in transport and turbulence theory we present linear and nonlinear diffusion coefficients within an improved dynamical turbulence model to demonstrate that the observed mean free paths can indeed be reproduced theoretically.

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