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. 2022 Apr 20;21(3):1029–1041. doi: 10.1007/s10237-022-01579-0

Fig. 5.

Fig. 5

Power spectral density of the turbulent kinetic energy in axisymmetric and eccentric cases at Re=2100. The black, green and red lines respectively correspond to 60%, 50% and 25% stenosis degrees. Each column shows the PSD at x=1,2,3 and 4 diameters downstream of stenosis respectively during the blowing stage. Each rows from left to right shows PSD for oscillation frequencies of ω1, ω2 and ω3 respectively. The solid, dotted and dashed lines have slope of -53, -103 and -7