Based on the work of Luo & Melrose (1992), a maser curvature emission mechanism in the presence of curvature drift is used to explain the optical pulsations from anomalous X-ray pulsars (AXPs). The model comprises a rotating neutron star with a strong surface magnetic field, i.e., a magnetar. Assuming the space charge-limited flow acceleration mechanism, in which the strongly magnetized neutron...