A non-conservative radiation field around a luminous inner corona generates magnetic fields up to roughly 10^5 Gauss, about five percent of equipartition, over the viscous infall time.
M., Contopoulos, I., & Kazanas, D
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Generation of magnetic fields around black hole accretion discs due to non conservative radiation fields
A non-conservative radiation field around a luminous inner corona generates magnetic fields up to roughly 10^5 Gauss, about five percent of equipartition, over the viscous infall time.