  A number of observational and theoretical aspects of solar magnetoconvection
are considered in this review. We discuss recent developments in our
understanding of the small-scale structure of the magnetic field on the solar
surface and its interaction with convective flows, which is at the centre of
current research. Topics range from plage areas in active regions over the
magnetic network shaped by supergranulation to the ubiquituous `turbulent'
internetwork fields. On the theoretical side, we focus upon magnetic field
generation by small-scale dynamo action.
