Voronoi maps showing the 3D Jeans model fit to the LMC velocity dispersion field from the Gaia DR3 kinematic data. The first column represents the data in the X, Y, and LOS directions, respectively. Each Voronoi bin is colour-coded according to the maximum likelihood velocity dispersion of all stars that fall into it, taking into account their individual velocity uncertainties. The second column represents the Jeans model results and the third column the model residuals. PMs are converted into linear velocities. The velocity scale is kept constant amongst all maps for consistency and easier comparison.