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To explain the pulsed emission of the rotation powered pulsars from radio togamma-ray, the polar cap models, the slot gap models, and the outer gap modelsare proposed. The recent observations suggest that these models are likely toco-exist in the same magnetosphere. If so, their mutual relation is known to betroublesome (Harding 2009) due to the boundary conditions and the direction ofthe current which are properly assumed in each acceleration models. Weperformed a particle simulation for the global magnetospheric structure. Basedon the simulation, we present a new picture of the global structure of thepulsar magnetosphere. It is found that a new dead zone is formed along thecurrent neutral line which separates the oppositely directed current. We shallcall this the current- neutral zone. We suggest that the polar cap acceleratorsand the slot gaps locate above the current-neutral zone, and the outer gapexist between the current neutral zone and the traditional dead zone. We alsogive an estimate of the super-rotation region.

A Particle Simulation for the Pulsar Magnetosphere: Relationship of Polar Cap, Slot Gap, and Outer Gap