Fig. 6: Calibration of the grain architecture model.

Comparison of characteristics of the Laguerre tessellation fitted to FIB-EBSD data and the stochastic grain architecture model. Pair correlation function of seed points (a), probability densities of nearest neighbor distances (b) and additive weights (c), and two-dimensional (joint) density of additive weights and nearest neighbor distances of seed points (d). All distances are given in terms of the voxel length scale of FIB-EBSD data.