The angular power spectrum of TeV cosmic-ray anisotropies from turbulent convection is shown to scale as ℓ^{-γ-1} even for purely parallel diffusion, matching the isotropic model.
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Convection Anisotropies of Cosmic Rays in Highly Magnetized Plasma
The angular power spectrum of TeV cosmic-ray anisotropies from turbulent convection is shown to scale as ℓ^{-γ-1} even for purely parallel diffusion, matching the isotropic model.