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Within the classical convection--diffusion approximation, we show that the angular distribution of cosmic rays (CRs) in a highly turbulent flow may exhibit significant small-scale anisotropies. The CR intensity angular power spectrum C_ is then a direct reflection of interstellar turbulence, from which one expects C_^- -1 for 1, where is the power-law turbulence spectral index. Observations by IceCube and HAWC at TeV energies can be explained approximately with the Kolmogorov law =5/3 with a convection velocity dispersion of 20 km/s on the scale of 10 pc.
Zhang et al. (Mon,) studied this question.
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