Top to bottom: cosmic-ray flux-weighted mean Mach number , CR flux-weighted mean CR-to-thermal pressure ratio X_CR, and dissipated energy flux-weighted efficiencies , and ζ(θ_B) as a function of time for the simulation with (red) and without (green) obliquity dependency. We recall that η₀ = 0.1 is used in those simulations and that ξ is a function of and X_CR as extrapolated from the values of Kang & Ryu (2013).