This paper presents comprehensive energy calculations for astrophysical plasmas across multiple scales, from supermassive black holes to solar ejection events, using the APCCE (Al-Mahaqari Plasmagnetic Critical Current Engine) framework. The calculations span 24 orders of magnitude in energy and are validated against observational data from NASA missions, ground-based observatories, and helioseismology. Key results include: M87* black hole magnetic energy 1.6 × 10⁵⁴ J, ratio EB/Eg = 0.006, FL/Fg = 1.35 × 10⁵⁸; Sgr A* black hole magnetic energy 7.0 × 10⁵¹ J, FL/Fg = 4.10 × 10⁴⁸; Quasar 3C 273 radiated power 1.8 × 10⁴⁶ W; Solar CIV braking energy 1.8 × 10³⁵ J, mass loss ∼0.13% solar mass; Jupiter magnetic energy 1.3 × 10²⁵ J, induced current I = 5.0 × 10⁶ A; Saturn magnetic energy 1.6 × 10²³ J, induced current I = 1.0 × 10⁵ A; Earth magnetic energy 1.0 × 10²⁰ J. All calculations show excellent agreement with observations, confirming the universality of the APCCE framework. The paper includes 600 simulation runs, 12 solar system bodies, 8 elements, and 5 sensitivity analyses. Testable predictions are provided for future missions.
Al-Mahaqari et al. (Sun,) studied this question.