  Standard solar models (SSM) constructed in accord with low metal abundances
disagree with the seismically inferred results. We constructed rotating solar
models with low metal abundances that included enhanced settling and convection
overshoot. In one of our rotating models, \textbf{AGSSr2a}, the convection
overshoot allowed us to recover the radius of the base of convection zone (CZ)
at a level of $1\sigma$. The rotational mixing almost completely counteracts
the enhanced settling for the surface helium abundance, but only partially for
the surface heavy-element abundance. At the level of $1\sigma$, the combination
of rotation and enhanced settling brings the surface helium abundance into
agreement with the seismically inferred value of $0.2485\pm0.0035$, and makes
the model have better sound-speed and density profiles than SSM constructed in
accordance with high metal abundances. The radius of the base of the CZ and the
surface helium abundance of \textbf{AGSSr2a} are $0.713$ $R_{\odot}$ and
$0.2472$, respectively; the absolute values of the relative differences in
sound speed and density between it and the Sun are less than $0.0025$ and
$0.015$, respectively. Moreover, predicted neutrino fluxes of our model are
comparable with the predictions of previous research works.
