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The Integral and Correlation Scales of Solar Wind Turbulence

  • Authors: Jean C. Perez, Sofiane Bourouaine, Mason Dorseth

Jean C. Perez et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 3.

Estimated ACF (normalized) ﹩{\hat{R}}_{b}(\ell )={\hat{C}}_{b}(\ell )/{\hat{C}}_{b}(0)﹩ and ﹩{\hat{R}}_{h}(\ell )={\hat{C}}_{h}(\ell )/{\hat{C}}_{h}(0)﹩ vs. τ = ℓδt, with signal centered around the local mean (LM) vs. global mean (GM) for different interval lengths T. Note that the unbiased ACF is estimated up to a maximum lag equal to half the selected interval length. Top left: estimated ﹩{\hat{R}}_{b}(\ell )﹩ calculated with magnetic field interval centered around its own (local) mean. Top right: estimated ﹩{\hat{R}}_{b}(\ell )﹩ calculated with magnetic field interval centered around the ensemble (global) mean. Bottom left: estimated ﹩{\hat{R}}_{h}(\ell )﹩ calculated with magnetic field interval centered around its own (local) mean. Bottom right: estimated ﹩{\hat{R}}_{h}(\ell )﹩ calculated with magnetic field interval centered around the ensemble (global) mean.

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