This document discusses resampling SMOS maps to match the resolution and incidence angles of AQUARIUS in order to enable synergistic analysis between the two missions. It describes using discrete Fourier transforms and Kaiser windows to resample SMOS maps while minimizing interpolation artifacts. The optimal Kaiser window parameters are determined through non-linear optimization to degrade SMOS pixels to equivalent AQUARIUS resolutions. An example resampling of SMOS brightness temperature maps for an overpass is provided. The procedure enables accurate resampling of SMOS maps for direct comparison with AQUARIUS observations.