Anisotropic turbulence in the solar wind

Details Anisotropic turbulence in the solar wind Anisotropic turbulence in the solar wind

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..256m&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 256

Computer Science

1

Solar Wind Plasma, Sources Of Solar Wind, Plasma Turbulence, Magnetohydrodynamic And Fluid Equation

Scientific paper

Recent investigations indicate that the solar wind turbulence spectrum may contain a significant admixture of two dimensional fluctuations, having variations mainly perpendicular to the local magnetic field. These indications come from simulations, from the theory of nearly incompressible MHD, from cosmic ray transport studies and from transport theory for solar wind turbulence, and from interpretations of direct observations.

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