Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....7.3859p&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
Scientific paper
Cross-helicity affects magnetic variance and correlation length which are vital in the calculation of diffusion tensor needed for solar modulation of cosmic rays. A global solar wind turbulence model is discussed through the governing turbulence equations which consider magnetic variance, magnetic correlation length, plasma temperature, and cross-helicity. Developing such model we study the effect of the cross-helicity on the formulation of an abinitio theory for solar modulation of cosmic rays. For this the po orly understood perpendicular diffusion is considered to have been derived from the use of velocity-correlation functions using Green-Kub o-Taylor formalism.
Bieber John W.
Burger R. A.
Matthaeus William H.
Parhi S.
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