Fully developed anisotropic hydromagnetic turbulence in interplanetary space

Details Fully developed anisotropic hydromagnetic turbulence in interplanetary space Fully developed anisotropic hydromagnetic turbulence in interplanetary space

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980phrvl..45..144d&link_type=abstract

Physical Review Letters, vol. 45, July 14, 1980, p. 144-147.

Physics

168

Anisotropic Media, Interplanetary Space, Magnetohydrodynamic Turbulence, Solar Wind, Asymmetry, Propagation Modes, Relaxation (Mechanics), Vortices

Scientific paper

Solar-wind magnetohydrodynamic turbulence is observed to be mainly made of Alfvenic fluctuations propagating away from the sun. It is shown that such an asymmetric state is a general consequence of the evolution of developed magnetohydrodynamic turbulence, which, starting from an initial asymmetry between modes with cross helicity plus 1 and minus 1, tends, as a consequence of nonlinear interactions, towards a state where the only modes left are those initially prevailing (with either cross helicity plus 1 or minus 1).

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