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A Survey of General Relativistic Magnetohydrodynamic Models for Black Hole Accretion Systems

  • Authors: Vedant Dhruv, Cora Prather, George N. Wong, Charles F. Gammie

Vedant Dhruv et al 2025 The Astrophysical Journal Supplement Series 277 .

  • Provider: AAS Journals

Caption: Figure 17.

A heat map of the radial component of the magnetic field Br at the event horizon for the SANE a* = −0.5 simulation. Top panel: Br at a specific instant in time. Bottom panel: Br averaged over the interval t = [25, 30] × 103tg. In both panels, note that Br changes polarity within each hemisphere. This behavior is not accounted for in Equation (12), leading to an overestimation of ΦBH.

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