We study complete sample of spiral galaxies brighter than M B ∼ -18.4 in three Abell clusters: A85 (z = 0.055), A496 (z = 0.033) and A2670 (z = 0.076). This work is based on a large volume limited, blind Hi-survey (21cm, NRAO-VLA), on optical imaging (CFHT) and on the search for dynamical substructures. Our goal is to explore the effects of local environment on the Hi gas properties and this, in turn, on the star formation activity and quenching of individual galaxies. We report significant differences among the HI properties of these clusters and we discuss the role played by the large scale structure and by the dynamical evolution of each cluster accounting for the observational evidence.