Image Details
Caption: Figure 2.
Time series of all models showing horizon-penetrating magnetic flux (a), jet power (b), upper-hemisphere magnetic-field coherency (c), lower-hemisphere magnetic-field coherency (d), mass accretion rate (e), and the dimensionless horizon-penetrating magnetic flux, i.e., the magnetically arrested disk (MAD) parameter (f).
© 2026. The Author(s). Published by the American Astronomical Society.