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The measured spectrum of kinetic Alfven wave fluctuations in the turbulentsolar wind plasma is used to calculate the electron and ion distributionfunctions resulting from quasi-linear diffusion. The modified ion distributionfunction is found to be unstable to long wavelength electromagnetic ioncyclotron waves. These waves pitch angle scatter the parallel ion velocity intoperpendicular velocity which effectively increases the perpendicular iontemperature.

Quasilinear Evolution of Kinetic Alfven Wave Turbulence and Perpendicular Ion Heating in the Solar Wind