Figure 16From: Technologies for supporting high-order geodesic mesh frameworks for computational astrophysics and space sciencesLeft: velocity magnitude isosurfaces from the manufactured solution problem. The solution has a resemblance to an interaction between a stellar wind an a uniform flow. A fourth order scheme was used on division 6 mesh with 64 radial shells. Right: density error distribution in a spherical layer at \(r=2.75\)Back to article page