  We derive equations for the mean entropy and the mean internal energy in the
low-Mach-number temperature stratified turbulence (i.e., for turbulent
convection or stably stratified turbulence), and show that turbulent flux of
entropy is given by ${\bf F}_s=\overline{\rho} \, \overline{{\bf u} s}$, where
$\overline{\rho}$ is the mean fluid density, $s$ are fluctuations of entropy
and overbars denote averaging over an ensemble of turbulent velocity field,
${\bf u}$. We demonstrate that the turbulent flux of entropy is different from
the turbulent convective flux, ${\bf F}_c=\overline{T} \, \overline{\rho} \,
\overline{{\bf u} s}$, of the fluid internal energy, where $\overline{T}$ is
the mean fluid temperature. This turbulent convective flux is well-known in the
astrophysical and geophysical literature, and it cannot be used as a turbulent
flux in the equation for the mean entropy. This result is exact for
low-Mach-number temperature stratified turbulence and is independent of the
model used. We also derive equations for the velocity-entropy correlation,
$\overline{{\bf u} s}$, in the limits of small and large Peclet numbers, using
the quasi-linear approach and the spectral tau approximation, respectively.
This study is important in view of different applications to the astrophysical
and geophysical temperature stratified turbulence.
