Characteristic phenomena of magnetohydrodynamic turbulence

Details Characteristic phenomena of magnetohydrodynamic turbulence Characteristic phenomena of magnetohydrodynamic turbulence

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.235..175m&link_type=abstract

In ESA Future Missions in Solar, Heliospheric and Space Plasma Physics p 175-179 (SEE N86-27330 18-12)

Physics

Magnetohydrodynamic Turbulence, Magnetohydrodynamics, Solar Physics, Theoretical Physics, Plasma Decay, Quadrupoles, Spectral Methods, Vortex Filaments, Vortices

Scientific paper

Magnetohydrodynamic (MHD) turbulence theory is reviewed. Mangetic X points, vorticity quadropoles, concentrated current filaments, highly anisotropic spectra, selective decay and dynamic alignment phenomena (charaterized by highly unequal dissipation rates for global ideal invariants), and kinking turbulence for plasmas which carry strong currents are reviewed. The most useful tool for obtaining accurate information about turbulent dynamics is numerical solution of the MHD equations.

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