Fig. 10.
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Convective stability analysis. The result is obtained according to Equation (16) based on simulation data at 4.5tB. The red solid lines mark the density scale height of accretion flows, as shown in Figure 2. Panel (A): Runs R22 (left) and R23 (right). Panel (B): Runs R24 (left) and N24 (right). The black regions are unstable.
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