Transport and turbulence modeling of solar wind fluctuations

Details Transport and turbulence modeling of solar wind fluctuations Transport and turbulence modeling of solar wind fluctuations

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....9510291z&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 95, July 1, 1990, p. 10291-10311. Research supported by NASA and Bartol R

Physics

122

Fluctuation Theory, Homogeneous Turbulence, Magnetohydrodynamic Turbulence, Magnetohydrodynamic Waves, Radiation Transport, Solar Wind, Periodic Variations, Perturbation Theory, Poisson Equation, Power Spectra, Spatial Distribution

Scientific paper

A detailed derivation of a transport model for MHD fluctuations in the solar wind is presented. Dynamical equations based on a two-length scale expansion are derived from which the evolution of various wavenumber spectra may be computed, including magnetic and kinetic energies, cross helicity, induced electric field, and the corresponding helicities. Several simple analytic solutions of the equations are consistent with Helios and Voyager predictions.

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