A Further Study of Relative longitude shift of Pulsar Beams

Abstract

It is of great important to study pulsar beam shapes if we are concerned with emission theories and pulsar birth rate. Both observations and/or the inverse Compton scattering model show that different emission components are emitted from different heights. The relative longitude phase shifts due to different heights of emission components and to the toroidal velocity of electron are considered in this paper. Several possible observational features arising from the phase shift effects are presented. The emission beams may not have circular cross sections although the emission regions may be symmetric with respect to the magnetic axes.