  We present a numerical study of finite-temperature superfluid turbulence
using the vortex filament model for superfluid helium. We examine the
phenomenon of vorticity locking between the normal and superfluid components
across a wide range of temperatures, using two different structures of external
normal fluid drive. We show that vorticity locking increases with temperature
leading to the superfluid flow being more influenced by the characteristics of
the normal fluid. This also results in stronger superfluid polarization and
turbulent intermittency. We also examine how these properties influence the
pressure field and attempt to verify a long-standing $P_k\propto k^{-7/3}$
theoretical quantum signature within the spatial pressure spectrum.
