Transport of cross helicity and radial evolution of Alfvénicity in the solar wind

Details Transport of cross helicity and radial evolution of Alfvénicity in the solar wind Transport of cross helicity and radial evolution of Alfvénicity in the solar wind

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004georl..3112803m&link_type=abstract

Geophysical Research Letters, Volume 31, Issue 12, CiteID L12803

Physics

Plasma Physics

24

Interplanetary Physics: Interplanetary Magnetic Fields, Interplanetary Physics: Mhd Waves And Turbulence, Interplanetary Physics: Solar Wind Plasma, Space Plasma Physics: Nonlinear Phenomena, Space Plasma Physics: Transport Processes

Scientific paper

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 Alfvénic states.

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