We study the time evolution of classical spin systems with purely rela
xational dynamics, quenched from T much greater than T-c to the critic
al point, in the semi-infinite geometry. Shortly after the quench, as
in the bulk, a nonequilibrium regime governed by universal power laws
is also found near the surface. We show for ''ordinary'' and ''special
'' transitions that the corresponding critical exponents differ from t
heir bulk values, but can be expressed via scaling relations in terms
of known bulk and surface exponents. To corroborate our scaling analys
is, we present perturbative (E-expansion) and Monte Carlo results.