Estimates of the magnetic field following equipartition () and magnetostrophic () scalings as in Augustson et al. (2019), with KE being the mixing length value of the kinetic energy at the radius where ν_conv is taken from each stellar structure model. The red squares/triangles denote the equipartition/magnetostropic bounds of the estimates for the γ Dor stars and the blue circles/triangles those for the SPB stars, with the two bounding values connected via a dotted line for each star in the two samples.