  In this work we construct a family of spherically symmetric, static, charged
regular black hole metrics in the context of Einstein-nonlinear electrodynamics
theory. The construction of the charged regular black hole metrics is based on
three requirements: (a) the weak energy condition should be satisfied, (b) the
energy-momentum tensor should have the symmetry $T^{0}_{0}=T^{1}_{1}$, and (c)
these metrics have to asymptotically behave as the Reissner-Nordstr\"{o}m black
hole metric. In addition, these charged regular black hole metrics depend on
two parameters which for specific values yield regular black hole metrics that
already exist in the literature. Furthermore, by relaxing the third
requirement, we construct more general regular black hole metrics which do not
behave asymptotically as a Reissner-Nordstr\"{o}m black hole metric.
