2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/175242We consider observational and theoretical estimates of the accretion disc viscosity parameter $α$. We find that in thin, fully-ionized discs, the best observational evidence suggests a typical range $α\sim 0.1 - 0.4$, whereas the relevant numerical simulations tend to derive estimates for $α$ which are an order of magnitude smaller. We discuss possible reasons for this apparent discrepancy.MNRAS, in pressAstrophysicstext