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Magnetic fields play a crucial role in the dynamics and evolution of our Sun and other stars. A common method used to model the magnetic fields in solar and stellar atmospheres is the potential field source surface (PFSS) model (Altschuler & Newkirk, 1969; Schatten, Wilcox, & Ness, 1969). The PFSS equations assume that there is zero electrical current in the domain of interest, leading to the equations

pfsspy: A Python package for potential field source surface modelling