  Using our theory for the production of relativistic outflows, we estimate the
jet launching radius and the inferred mass accretion rate for 52 low-power
radio-loud AGNs based on the observed jet powers. Our analysis indicates that
(1) a significant fraction of the accreted energy is required to convert the
accreted mass to relativistic energy particles for the production of the jets
near the event horizon, (2) the jets launching radius moves radially toward the
horizon as the mass accretion rate or jets power increases, and (3) no
jet/outflow formation is possible beyond 44 gravitational radii.
