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M.R. Stemkowski, C.W. Smith & B.J. Vasquez

The Two-Dimensional Autocorrelation Function for Turbulence as Spatial Scales Near the Ion Dissipation Scale. M.R. Stemkowski, C.W. Smith & B.J. Vasquez. University of New Hampshire, Durham, NH. SHINE session: The Dissipation of Solar Wind Turbulence.

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M.R. Stemkowski, C.W. Smith & B.J. Vasquez

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  1. The Two-Dimensional Autocorrelation Function for Turbulence as Spatial Scales Near the Ion Dissipation Scale M.R. Stemkowski, C.W. Smith & B.J. Vasquez University of New Hampshire, Durham, NH SHINE session: The Dissipation of Solar Wind Turbulence • Multi-D correlation fns. show Np and Tp match magnetic and velocity turbulence. • Magnetic corr. fns. at small scales are no longer wind-speed dependent. • Dissipation range results show dominance of parallel wave vectors.

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