“…where i, j, k represent the cell index, W and R are the vector of conservative variables and flux residual respectively and V i,j,k is the volume of the cell i,j,k. Greater detail on the numerical techniques employed can be found within the previous investigations conducted using HMB3 (12,13,14,20,21,22,23,24) . Several turbulence models, of both URANS and hybrid LES/URANS families, are available in the HMB3 solver.…”