A discontinuity at the base of the transition layer located between the Keplerian accretion disk and the compact object

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Fig. 2.

Dependence of the ratio of the TL height to that of the disk h₁/h₂ on the Reynolds number γ₂ = Ṁ/4πh₂η₂ and temperature in the TL T₁ for the ratio of turbulent viscosities η₂/η₁ = 45. All other calculations were carried out along the diagonal line, which reflects the transition between the high/soft and low/hard states.

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