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Fig. 2.
Time evolution for six simulations with kturb = 2 of the clumping factor of the gas density n (top panel), the cosmic-ray energy density ECR (middle panel), and the Alfvénic Mach number 
(bottom panel). The clumping factor C(X) of a quantity X is defined as C(X) = ⟨X2⟩∕⟨X⟩2.
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