Comparison of the cosmic-ray fluxes (top) and wave spectra (bottom) obtained with the default parameter sets. In the Kolmogorov case, we choose A = 10³⁶ cm⁻⁵ g⁻³ s², α = 4.25, η = 0.03, v_A = 25 km s⁻¹, B₀ = 1.6 μG, ﹩H=4\,\mathrm{kpc},\,\mathrm{and}\,{k}_{0}^{-1}=50\,\mathrm{pc}﹩, whereas for Kraichnan, it is A = 10^34.5 cm⁻⁵ g⁻³ s², α = 4.08, η = 0.04, v_A = 1 km s⁻¹, B₀ = 1.5 μG, H = 4 kpc, and ﹩{k}_{0}^{-1}=50\,﹩pc.