Journal
GEOPHYSICAL RESEARCH LETTERS
Volume 31, Issue 12, Pages -Publisher
AMER GEOPHYSICAL UNION
DOI: 10.1029/2004GL019645
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A transport theory including cross helicity, magnetohydrodynamic (MHD) turbulence, and driving by shear and pickup ions, is applied to the radial evolution of the solar wind. The radial decrease of cross helicity observed in the solar wind can be accounted for when sufficient driving is included to overcome the inherent tendency for MHD turbulence to produce Alfvenic states.
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