We examine the influence of the Reynolds stress as the main contribution of
turbulence on the oscillation frequencies of the solar p-modes. We regard
the radial oscillations as well as the nonradial ones in order to study the
influence depending on the degree l of the modes.
For the radial modes we find that the influence of the turbulence gives cor
rections that reduce significantly the difference between observed and theo
retical calculated frequencies. Regarding the nonradial modes we find, addi
tionally, an increase in the corrections with the harmonic degree l which i
s in good agreement with the observations.
We consider turbulent corrections appearing in the oscillation equations as
well as the changes of the model itself for consistency. For radial and no
nradial modes we find that the changes of the model are of minor importance
compared to the turbulence terms appearing directly in the equations of th
e oscillation.