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Fig. 3


One-dimensional plots of the initial and evolved power spectra of the magnetic field fluctuations as a function of parallel Kx di and perpendicular Kydi normalized wave numbers as a function of the propagation angle. From left to right the plots correspond to parallel θ = 0°, quasi-parallel θ ≤ 30°, and highly oblique propagation at θ ≤ 60°. All cases are initialized with anisotropic spectral slope with different values along Kx and Ky; see Table 1.

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