Magnetohydrodynamic turbulence in the solar wind

Details Magnetohydrodynamic turbulence in the solar wind Magnetohydrodynamic turbulence in the solar wind

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280..73m&link_type=abstract

In JPL Solar Wind Five p 73-80 (SEE N84-13067 03-92)

Physics

Fluid Dynamics

6

Magnetohydrodynamic Turbulence, Nonlinearity, Solar Wind, Space-Time Functions, Fluid Dynamics, Interplanetary Medium, Magnetic Field Configurations, Reynolds Number, Velocity Distribution

Scientific paper

Recent work in describing the solar wind as an MHD turbulent fluid has shown that the magnetic fluctuations are adequately described as time stationary and to some extent as spatially homogeneous. Spectra of the three rugged invariants of incompressible MHD are the principal quantities used to characterize the velocity and magnetic field fluctuations. Unresolved issues concerning the existence of actively developing turbulence are discussed.

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