Evolution of turbulent magnetic fluctuation power with heliocentric distance

Details Evolution of turbulent magnetic fluctuation power with heliocentric distance Evolution of turbulent magnetic fluctuation power with heliocentric distance

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..630z&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 630

Physics

2

Solar Wind Plasma, Sources Of Solar Wind, Interplanetary Magnetic Fields, Magnetohydrodynamics And Plasmas

Scientific paper

On the basis of transport theories appropriate to a radially expanding solar wind, new results for the radial evolution of the energy density in solar wind fluctuations at MHD scales are derived. The models, which represent a departure from the well-known WKB description, include the effects of ``mixing'', driving by stream-stream interactions and interstellar pick-up ion generated waves as well as non-isotropic MHD turbulence.

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