Figure 6From: Efficient conservative ADER schemes based on WENO reconstruction and space-time predictor in primitive variables Two-dimensional Kelvin-Helmholtz instability obtained with the \(\pmb{\mathbb{P}_{0}\mathbb{P}_{3}}\) scheme and with the Osher flux. Left panels: solution with ADER-Prim. Central panels: solution with ADER-Cons. Right panels: solution with ADER-Char. Top panels: solution at \(t=2.0\). Bottom panels: solution at \(t=2.5\).Back to article page