Local Magnetic Turbulence and TeV–PeV Cosmic Ray Anisotropies
Local Magnetic Turbulence and TeV–PeV Cosmic Ray Anisotropies
In the energy range from ∼10(12) eV to ∼10(15) eV, the Galactic cosmic ray flux has anisotropies both on large scales, with an amplitude of the order of 0.1%, and on scales between ≃10° and ≃30°, with amplitudes smaller by a factor of a few. With a diffusion coefficient inferred …