Top: radial profiles of the accretion rate (gray) and the cumulative mass-loss rate due to MHD (dashed green) and photoevaporative winds (dashed yellow) at t = 1 Myr after disk formation. The accretion rate solely due to viscous stress is indicated by blue lines. Model Fid is shown in the left panels, and Vis is shown in the right panels. Bottom: Time evolutions of the accretion rate measured at r = r_in (= 0.01 au; solid gray) and r = 1 au (dashed gray). The total mass-loss rates by the MHD (dashed green lines) and photoevaporative winds (solid yellow) are also shown.