The user randomly selects \(N_{star}\) points across the factor space using
either Sobol' Quasi Random Numbers (type = "QRN"
) or random numbers (type = "R"
).
These are the star centres and their location can be denoted as
\(\mathbf{s}_v = s_{v_1},...,s_{v_i}, ..., s_{v_k}\), where \(v=1,2,...,N_{star}\).
Then, for each star centre, the function generates a cross section of equally spaced points
\(\Delta h\) apart for each of the \(k\) model inputs, including and passing through the
star centre. The cross section is produced by fixing \(\mathbf{s}_{v_{\sim i}}\) and varying \(s_i\).
Finally, for each factor all pairs of points with \(h\) values of \(\Delta h, 2\Delta h, 3\Delta h\)
and so on are extracted. The total computational cost of this design is
\(N_t=N_{star} (k (\frac{1}{\Delta h} - 1) + 1)\).