Cosmic-Ray Plasma Coupling in the Outer Heliosphere

Details Cosmic-Ray Plasma Coupling in the Outer Heliosphere Cosmic-Ray Plasma Coupling in the Outer Heliosphere

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..719..353l&link_type=abstract

PHYSICS OF THE OUTER HELIOSPHERE. AIP Conference Proceedings, Volume 719, pp. 353-358 (2004).

Physics

8

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

The transport equation describing the coupling of cosmic rays to the heliospheric plasma is presented, together with an illustrative solution valid at high energies for the solar modulation of galactic cosmic rays (GCR) in both the solar wind and the heliosheath. The nonlinear backreaction of GCR and the anomalous cosmic ray component on the heliospheric flows and magnetic fluctuation spectra are described briefly. Finally, a calculation is presented, which shows that care must be taken in the interpretation of a large component of the particle flux normal to the magnetic field as evidence of a large perpendicular diffusion coefficient.

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