Radial evolution of the energy density of solar wind fluctuations

Details Radial evolution of the energy density of solar wind fluctuations Radial evolution of the energy density of solar wind fluctuations

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf..106z&link_type=abstract

Delaware Univ., International Solar Wind 8 Conference, p. 106

Physics

Flux Density, Magnetohydrodynamics, Solar Wind, Radial Distribution, Cosmic Rays, Magnetohydrodynamic Turbulence, Transport Theory, Plasma Heating, Interstellar Matter

Scientific paper

On the basis of transport theories appropriate to a radially expanding solar wind, we describe new results for the radial evolution of the energy density in solar wind fluctuations at MHD scales. These models include the effects of 'mixing' and driving as well as the possibility of non-isotropic MHD turbulence. Implications of these results for solar wind heating, cosmic ray diffusion and interstellar pick-up ions will also be addressed.

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