The evolution of the inter cluster medium over cosmic time, and its interaction with galaxies within those clusters, is key to understanding galaxy evolution and quenching processes. We present spatially resolved ALMA observations of 24 galaxies across three clusters at z=1.6, the largest such sample of cluster galaxies observed at this redshift. We find signs of interaction with the ICM, through the influence of ram pressure stripping, to be affecting the molecular gas in these galaxies. We find signs of enhanced molecular gas fractions, kinematic disturbances in the disk, and asymmetric head-tail morphologies, consistent with observations of ram pressure stripped galaxies at low redshift. We present preliminary results of our spatial and kinematic analysis of these galaxies, and compare the properties of galaxies in these clusters to low-redshift clusters in which the effects of ram pressure have been observed.