Dynamics and emission properties of flux ropes from two-temperature GRMHD simulations with multiple magnetic loops

Open Access

Fig. 2.

Time evolution of (a) mass accretion rate (Ṁ) and (b) magnetic flux rate ( $Φ_{B} / \sqrt{\dot{M}}$ $\Phi_{\mathrm{B}}/\sqrt{\dot{M}}$ ) onto the event horizon in both M20a3D (black) and M80a3D (blue).

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