Models of inertial range spectra of interplanetary magnetohydrodynamic turbulence

Details Models of inertial range spectra of interplanetary magnetohydrodynamic turbulence Models of inertial range spectra of interplanetary magnetohydrodynamic turbulence

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....9514881z&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 95, Sept. 1, 1990, p. 14881-14892. Research supported by NASA.

Physics

106

Interplanetary Medium, Magnetohydrodynamic Turbulence, Turbulence Models, Energy Spectra, Interplanetary Space, Solar Wind, Transport Properties

Scientific paper

A framework based on turbulence theory is presented to develop approximations for the local turbulence effects that are required in transport models. An approach based on Kolmogoroff-style dimensional analysis is presented as well as one based on a wave-number diffusion picture. Particular attention is given to the case of MHD turbulence with arbitrary cross helicity and with arbitrary ratios of the Alfven time scale and the nonlinear time scale.

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