We present here simulations of the HDO cycle on Mars, using an updated version of the LMD Mars GCM. This is a follow-up from Rossi et al. (2021), this time including more physical processes: microphysics of cloud formation, radiatively active clouds, effect of kinetics during fractionnation by condensation. The simulations pertain to the climatology and Martian year 34 dust scenarios. There are different types of files: * yearly files (Ls=0-360 for the climatology dust scenario). Outputs are expressed in terms of altitude above areoid, latitude and longitude, and time (solar longitude). * monthly files (9th martian month, with different model settings), expressed in terms of pressure, latitude and longitude, and time (solar longitude). * GCM outputs colocated to the coordinates of TGO/ACS-MIR observations, in altitude above areoid and time (Ls=180-360 for MY34). * GCM outputs colocated to the coordinates of MRO/MCS observations, in pressure and time (Ls=240-300 for MY34). * Two ACS/MIR datasets, one provided by Anna Fedorova (Fedorova et al. 2020), the other processed by Mikhail Luginin (https://data.mendeley.com/datasets/rkszdmpdcy/1), reinterpolated vertically and stored in a netcdf