期刊
GEOPHYSICAL RESEARCH LETTERS
卷 31, 期 12, 页码 -出版社
AMER GEOPHYSICAL UNION
DOI: 10.1029/2004GL019645
关键词
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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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