The time duration when no ionization activity is detectable during consecutive, separate positive streamer corona bursts in long air gap experiments is generally referred to as the dark period (Gallimberti, 1979). The dark period is explained by the reduction of the electric field around the highly stressed positive electrode by the space charge left behind after a streamer stops propagating (Les Renardières Group, 1974). This electrostatic shielding effect has been assumed to inhibit the further development of ionization, usually detected in camera images as a dark period without visible illumination. However, if the applied voltage continues increasing, the electric field distribution will also augment until a new streamer is again initiated, ending the dark period. It can take place multiple times both before and after the initiation of a stable positive leader discharge, when it is referred to as the primary or the secondary dark period respectively (Carrara & Thione, 1976). Observe that the dark period that