Relativistic winds from pulsar and black hole magnetospheres

The present consideration of the extraction of the rotational energy stored in a Kerr black hole by a large-scale MHD wind as a possible source for AGN jet energy proceeds by viewing both the ingoing and outgoing winds as propagating toward asymptotic infinities and transporting the conserved mass, angular momentum, and energy fluxes established by the source region. It is judged that the field-line rotation rate or total voltage drop across the system must also be determined by the dissipative process that injects plasma onto the magnetospheric field lines.