  The inductive electric field is unjustifiably neglected in most models for
pulsar electrodynamics; it cannot be screened by the magnetospheric plasma, and
it is not small in comparison with the corotation electric field. The
perpendicular component of the inductive electric field implies a drift motion
that is inconsistent with corotation at any angular velocity. Some implications
of the inductive electric field and the associated drift motion are discussed.
