“…The differences between the present LES, available URANS [8], [13] and experimental results were discussed [7], [8]. Furthermore, we provided a detailed analysis and comparison of the available numerical (LES and direct numerical simulations, DNS) and experimental data for the flows past CC ( [14], [15], [16], [17], [18], [4], [19] ) and SC ( [20], [21], [22], [23], [9], [24], [11], [25]) to compensate the limitation of HC experimental data to the integral flow parameters only.…”