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<p> is the scale height of the disk, and  is a free parameter between zero (no accretion) and approximately one. In a turbulent medium , where  is the velocity of turbulent cells relative to the mean gas motion, and  is the size of the largest turbulent cells, which is estimated as  and , where  is the Keplerian orbital angular velocity,  is the radial distance from the central object of mass . By using the equation of <a href="page.php?w=hydrostatic_equilibrium">hydrostatic equilibrium</a>, combined with conservation of <a href="page.php?w=angular_momentum">angular momentum</a></p><p>
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