  We present an analytical class of equilibrium solutions for the structure of
relativistic sheared and rotating magnetized jets that contain no boundary
current sheets. We demonstrate the overall dynamical stability of these
solutions and, most importantly, a better numerical resistive stability than
the commonly employed force-free structures which inevitably require the
presence of dissipative surface currents. The jet is volumetrically confined by
the external pressure, with no pressure gradient on the surface. We calculate
the expected observed properties of such jets. Given the simplicity of these
solution we suggest them as useful initial conditions for relativistic jet
simulations.
