We study the vertical structure of a radiation-pressure-dominated disc with
a hot corona. We include all the relevant processes like bound-free opacit
y and convection. We show that the presence of the corona modifies consider
ably the density and the opacity of the disc surface layers, which are impo
rtant from the point of view of spectrum formation. The surface of the disc
with a corona is much denser and less ionized than the surface of a bare d
isc. Such a disc is likely to produce a neutral reflection and a local spec
trum close to a blackbody. This effect will help to reconcile the predictio
ns of accretion disc models with the observational data since a neutral ref
lection and a lack of Lyman edge are generally seen in active galactic nucl
ei.