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We investigate static inhomogeneous charged planar black hole solutions ofthe Einstein-Maxwell system in an asymptotically anti-de Sitter spacetime.Within the framework of linear perturbations, the solutions are numerically andanalytically constructed from the Reissner-Nordstr\"{o}m-AdS black holesolution. The perturbation analysis predicts that the Cauchy horizon alwaysdisappears for any wavelength perturbation, supporting the strong cosmiccensorship conjecture. For extremal black holes, we analytically show that anobserver freely falling into the black hole feels infinite tidal force at thehorizon for any long wavelength perturbation, even though the Kretschmannscalar curvature invariant remains small.

Inhomogeneous charged black hole solutions in asymptotically anti-de Sitter spacetime