Internal tides, generated by barotropic tides flowing over rough topography, are a primary source of energy into the internal wavefield. As internal tides propagate away from generation sites, they can dephase from the equilibrium tide, becoming nonstationary. Here, we examine how low-frequency quasigeostrophic background flows scatter and dephase internal tides in the Tasman Sea. We demonstrate that a semi-idealized internal-tide model (the Coupled-mode Shallow Water Model; CSW) must include two background-flow effects to replicate the in-situ internal-tide energy fluxes observed during the Tasmanian Internal-Tide Beam Experiment (TBeam). The first effect is internal-tide advection by the background flow, which strongly depends on the spatial scale of the background flow, and is largest at the smaller scales resolved in the background-flow model (i.e., 50-400 km). Internal-tide advection is also shown to scatter internal-tides from vertical mode-1 to mode-2 at a rate of about 1 mW m−2. The second effect is internal-tide refraction due to background-flow perturbations to the mode-1 eigenspeed. This effect primarily dephases the internal-tide, attenuating stationary energy at a rate of up to 5 mW m−2. Detailed analysis of the stationary internal-tide momentum and energy balances indicate that background-flow effects on the stationary internal tide can be accurately parameterized using an eddy diffusivity derived from a 1D random walk model. In summary, the results identify an efficient way to model the stationary internal tide and quantify its loss of stationarity.