Top to bottom: cosmic-ray flux-weighted mean Mach number , CR flux-weighted mean CR-to-thermal pressure ratio XCR, and dissipated energy flux-weighted efficiencies , and ζ(θB) 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 XCR as extrapolated from the values of Kang & Ryu (2013).
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