Heliospheric Solar Wind Turbulence Model with Implications for Latitudinal Transport of Cosmic Rays

Details Heliospheric Solar Wind Turbulence Model with Implications for Latitudinal Transport of Cosmic Rays Heliospheric Solar Wind Turbulence Model with Implications for Latitudinal Transport of Cosmic Rays

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....7.3795p&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

1

Scientific paper

A global solar wind turbulence model is discussed considering the governing equations for magnetic correlation length, magnetic variance, and plasma temperature. The model is integrated with the present version of our abinitio modulation code. Thus the diffusion coefficients which determine the final makeup of the abinitio modulation model are calculated from the first principles. By formulating such a theory for solar wind turbulence we describe its implications for latitudinal transport of cosmic rays by appropriately varying the variance and correlation length latitudinally.

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