Energy densities of Alfven waves between 0.7 and 1.6 AU

Physics

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Interplanetary Medium, Magnetohydrodynamic Waves, Particle Flux Density, Plasma Oscillations, Radial Distribution, Solar Wind, Mariner Space Probes, Periodic Variations, Solar Corona, Solar Temperature

Scientific paper

Plasma and field data from Mariner 4 and 5 between 0.7 and 1.6 AU are used to study the radial dependence of the levels of microscale fluctuation associated with interplanetary Alfven waves. The observed decrease of these levels with increasing distance from the sun is consistent with little or no local generation or damping of the ambient Alfven waves over this range of radial distance.

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