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Dynamics of charged particles in the vicinity of a rotating black holeembedded in the external large-scale magnetic field is numericallyinvestigated. In particular, we consider a non-axisymmetric model in which theasymptotically uniform magnetic field is inclined with respect to the axis ofrotation. We study the effect of inclination onto the prevailing dynamic regimeof particle motion, i.e. we ask whether the inclined field allows regulartrajectories or if instead, the deterministic chaos dominates the motion. Inthis contribution we further discuss the role of initial condition,particularly, the initial azimuthal angle. To characterize the measure ofchaoticness we compute maximal Lyapunov exponents and employ the method ofRecurrence Quantification Analysis.

Regular and chaotic motion in general relativity: The case of an inclined black hole magnetosphere