Figure 9From: Efficient conservative ADER schemes based on WENO reconstruction and space-time predictor in primitive variables Solution of the RMHD rotor problem at time \(\pmb{t=0.4}\) , obtained with the \(\pmb{\mathbb{P}_{0}\mathbb{P}_{3}}\) scheme on a uniform grid with \(\pmb{300\times300}\) cells. Top panels: rest-mass density (left) and thermal pressure (right). Bottom panels: Mach number (left) and magnetic pressure (right).Back to article page