The CKF solution of pulsar magnetospheres

We continue the pulsar magnetosphere calculations of Contopoulos, Kazanas and Fendt ([I]). The assumptions of the model are listed and illustrated. Different grids from 3000 up to 150x150 are used, though high resolution is not so important for determining the source function if only an appropriate convergence scheme is used (substantially different from the [1] approach, to be published elsewhere). We compactify the physical space to carry out integration on a finite grid.