  By combining data from different published 3-D simulations of Keplerian
shearing boxes unstable to the magnetorotational instability (MRI), we
highlight tight anti-correlations between the total effective inferred angular
momentum transport parameter, $\alpha_{tot}$, its separate Maxwell and Reynolds
contributions $\alpha_{mag}$ and $\alpha_{kin}$, and the kinetic to magnetic
pressure ratio $\beta$, defined with the initial or saturated (when available)
thermal pressure.
  Plots of $Log (\alpha_{kin}), Log (\alpha_{mag})$, and $Log (\alpha_{tot})$
vs $Log (\beta)$ are well fit by straight lines even as $\alpha_{kin}$,
$\alpha_{mag}$,and $\alpha_{tot}$ vary by four orders of magnitude over the
simulations included. The ratio $\alpha_{kin}/\alpha_{mag}$ and the product
$\alpha_{tot}\beta$ are quite constant and largely independent of the presence
or absence of weak mean fields, the choice of initial and boundary conditions,
and the resolution. In short, simulations have more strongly constrained the
product $\alpha_{tot}\beta$ than $\alpha_{tot}$ itself.
