Toolkit for creating plots and computing stable equipotential surfaces of fluids orbiting a compact stellar object (see Zarotti: Relativistic Hydrodynamics))
Implement a 3D visualization for the tori. Needed is the transformation of spherical to cartesian coordinates. Implement wireframe and surface switch. Also variate the number of setpoints, and put half a donut (phi from 0 to pi) as default.
Implement a 3D visualization for the tori. Needed is the transformation of spherical to cartesian coordinates. Implement wireframe and surface switch. Also variate the number of setpoints, and put half a donut (phi from 0 to pi) as default.