... result[*]
If $\nu_{\rm Mag} $ is too small, then magnetic fields are frozen-in to the gas approximately. In this case $B \sim \rho^{2/3}$, and B must increase inwards, irrespectively, whether the disk is standard or advection-dominated.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
... advection-dominated[*]
The flow is said to be advection-dominated if transport via fluid-motion dominates viscous re-distribution.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
Copyright ESO 2002