Zonal wind velocity as a function of equilibrium temperature computed by Menou (2012) (purple), Rogers & Komacek (2014) (yellow), Koll & Komacek (2018) (green), and this work (red). Our solid line indicates the equatorial wind velocity as computed by Menou (2012) and our dashed line indicates the mean zonal wind velocity as computed by Rogers & Komacek (2014) and Koll & Komacek (2018). The planetary parameters of HD 209458 b and a magnetic field of B = 15 G were held constant throughout our simulation. The velocity measurements are taken from Snellen et al. (2010) (HD 209458 b), Louden & Wheatley (2015) (HD 189733 b), Seidel et al. (2021) (WASP-76 b), and Cauley et al. (2021) (WASP-33 b).