Remarks on transport theories of interplanetary fluctuations

Details Remarks on transport theories of interplanetary fluctuations Remarks on transport theories of interplanetary fluctuations

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....9514863z&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 95, Sept. 1, 1990, p. 14863-14871. Research supported by NASA.

Physics

27

Interplanetary Space, Magnetohydrodynamic Turbulence, Transport Properties, Interplanetary Magnetic Fields, Magnetohydrodynamic Waves, Solar Wind, Wentzel-Kramer-Brillouin Method

Scientific paper

The structure of a transport theory presented by Zhou and Matthaeus (1989), in which coupling of 'inward' and 'outward'-type fluctuations appears in the leading order, is studied. Allowance is made for the dynamic behavior of the 'fast' scale variables, which are averaged over to obtain slow-scale transport equations. The relationship of the two-scale transport models to transport models derived from the WKB approximation (Jeffreys and Jeffreys, 1980: Weinberg 1962; Dewar, 1970) as it has been applied to the solar wind MHD wave problem (Parker, 1965; Hollweg, 1973, 1974) is discussed.

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