Can we understand the turbulent solar wind via turbulent simulations?

Details Can we understand the turbulent solar wind via turbulent simulations? Can we understand the turbulent solar wind via turbulent simulations?

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.confr..39g&link_type=abstract

Observatoire de Paris-Meudon, International Solar Wind 8 Conference, p. 39

Physics

Solar Wind, Magnetohydrodynamic Waves, Magnetohydrodynamic Turbulence, Solar Physics, Sun, Computerized Simulation, Mathematical Models, Solar Magnetic Field, Transport Properties, Anisotropy

Scientific paper

We attempt to assess the present understanding of the turbulent solar wind using numerical simulations. The solar wind may be considered as a kind of wind tunnel with peculiar properties: the tunnel is spherical; the source of the wind is rotating; and the medium is a plasma containing a large-scale magnetic field. These constraints lead to anisotropic dynamics of the fluctuations on the one hand, and to non-standard (turbulent?) transport properties of the global plasma on the other hand. How much of this rich physics can we approach today via numerical simulations?

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