“…Over the past decade, SPMHD has been used to simulate the evolution and impact of magnetic fields in a wide variety of astrophysical problems, such as the study of single and binary star formation (Bürzle et al, 2011a;Bürzle et al, 2011b;Price et al, 2012;Bate et al, 2014;Tsukamoto et al, 2015a;Tsukamoto et al, 2015b;Lewis et al, 2015;Tricco 10.3389/fspas.2023.1288219 Wurster et al, 2016;Wurster et al, 2017;Lewis and Bate, 2017;Wurster et al, 2018a;Wurster et al, 2018b;Tsukamoto et al, 2018;Tsukamoto et al, 2020;Wurster et al, 2021;Wurster et al, 2022), star cluster formation (Wurster et al, 2019;Dobbs and Wurster, 2021), star formation rates in spiral galaxies (Herrington et al, 2023), accretion discs (Forgan et al, 2017), tidal disruption events (Bonnerot et al, 2017), the magnetic field structure of spiral galaxies (Dobbs et al, 2016;Wissing and Shen, 2023), and galaxy cluster formation (Barnes et al, 2012;Barnes et al, 2018). It has been shown to yield correct behaviour for the small-scale dynamo amplification of magnetic fields (Tricco et al, 2016b), and can sustain turbulence incited by the magnetorotational instability (MRI) (Deng et al, 2019;Wissing et al, 2022).…”