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Table 1.

Summary of recurring model parameters.

Parameter Definition Comments
Regulates the scaling between the magnetic stress μ = 0 → Pmag ∝ Ptot
μ and the thermal pressure: μ = 0.5 →
μ = 1 → Pmag ∝ Pgas

α0 Proportionality constant of the viscosity law (see above) Small influence on LX − LUV

f(r) Fraction of accretion power dissipated in the corona f(r) for μ ≠ 0

fmax Maximum value of f(r) Impacts the normalization of the LX − LUV

f Mean value of a f(r) profile Real fraction of bolometric power emitted by the corona

η Fraction of f emitted downward back to the disk Exact value impacts the normalization of the LX − LUV

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