  We identify 45 protostellar outflows in CO maps of the Orion A giant
molecular cloud from the CARMA-NRO Orion survey. Our sample includes 11 newly
detected outflows. We measure the mass and energetics of the outflows,
including material at low-velocities by correcting for cloud contributions. The
total momentum and kinetic energy injection rates of outflows is comparable to
the turbulent dissipation rate of the cloud. We also compare the outflow
position angles to the orientation of C$^{18}$O filaments. We find that the
full sample of outflows is consistent with being randomly oriented with respect
to the filaments. A subsample of the most reliable measurements shows a
moderately perpendicular outflow-filament alignment which may reflect accretion
of mass across filaments and onto the protostellar cores.
