m.r. stemkowski, c.w. smith & b.j. vasquez
Post on 30-Dec-2015
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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. - PowerPoint PPT Presentation
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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
• 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.
SHINE session: The Dissipation of Solar Wind Turbulence
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