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We study the profile of a thin disk configuration as described by anaxisymmetric ideal magnetohydrodynamics steady equilibrium. We consider thedisk like a differentially rotating system dominated by the Keplerian term, butallowing for a non-zero radial and vertical matter flux. As a result, thesteady state allows for the existence of local peaks for the vertical velocityof the plasma particles, though it prevents the radial matter accretion rate.This ideal magnetohydrodynamics scheme is therefore unable to solve the angularmomentum-transport problem, but we suggest that it provides a mechanism for thegeneration of matter-jet seeds.

Emergence of High Peaks in the Axial Velocity for an Ideal Magnetohydrodynamics Disk Configuration