A kinetic model of jet-corona coupling in accreting black holes

Open Access

Fig. 6.

Top: Time series of Poynting flux entering (escaping) our integration surface – depicted in Fig. 3 – on open field lines threading the BH, ${\dot{E}}_{inj, BH - Inf}$ $\dot{\mathcal{E}}_{\mathrm{inj,BH-Inf}}$ ( ${\dot{E}}_{out, BH - Inf}$ $\dot{\mathcal{E}}_{\mathrm{out,BH-Inf}}$ ), and disk, ${\dot{E}}_{inj, Disk - Inf}$ $\dot{\mathcal{E}}_{\mathrm{inj,Disk-Inf}}$ ( ${\dot{E}}_{out, Disk - Inf}$ $\dot{\mathcal{E}}_{\mathrm{out,Disk-Inf}}$ ). Bottom: Time series of open (BH-Inf), closed (BH-Disk), and total horizon-piercing magnetic flux as in Fig. 4.

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