Distribution of the rotational kinetic energy (normalized by the maximum initial value) of the Balsara vortex after one advective time, t_adv, at Ṽ = 10⁻³ and β_K = 1. The top panels show the vortices obtained with the HLLD flux function as a function of resolution, while the plots in the bottom panels are obtained with LHLLD. The insets show the fraction of rotational kinetic energy that has been dissipated by the end of the simulation: /(E_R,t=0)_tot − 1.