ON THE TOTAL WIDTH OF PULSES AND THE STRUCTURE OF PULSAR MAGNETOSPHERES

Total widhts W0 of pulses were measured for 125 pulsars. It is shown t hat W0 can be a few times greater than W10. Values of W0/W10 decrease when, frequency increases. Angles beta between magnetic field and rota tion axis, relative distances x = (zeta - beta)/theta between the line of sight and the center of emission cone, and levels of emission gene ration at different frequencies were calculated on the base of the W0 values. These parameters were compared with those obtained by using W1 0. New results confirm the conclusion on non-dipolar field in a number of pulsars.