Image Details
Caption: Figure 4.
Similar to Figure 3 but now plotting the contribution of various components of the fluxes (see Equations (15), (16), (17), (18), (19), and (20)). We see that magnetic fields have little-to-no contribution toward ﹩\dot{L}﹩ and ﹩\dot{E}﹩ in the SANE models. In the MAD models, the trend in total flux closely matches the trend observed in the electromagnetic components.
© 2025. The Author(s). Published by the American Astronomical Society.