  Two-dimensional hydrodynamical simulations were made to calibrate the mixing
length parameter for modeling red giant's convective envelope. As was briefly
reported in Asida & Tuchman (97), a comparison of simulations starting with
models integrated with different values of the mixing length parameter, has
been made. In this paper more results are presented, including tests of the
spatial resolution and Large Eddy Simulation terms used by the numerical code.
The consistent value of the mixing length parameter was found to be 1.4, for a
red giant of mass 1.2 solar-mass, core mass of 0.96 solar-mass, luminosity of
200 solar-luminosities, and metallicity Z=0.001.

Astrophysics