The prediction of the temperature distribution in a gas turbine rotor
containing gas-filled closed cavities, for example between two disks,
has to account for the heat transfer conditions encountered inside the
se cavities. In an entirely closed annulus no forced convection is pre
sent, but a strong natural convection flow occurs induced by a nonunif
orm density distribution in the centrifugal force field. A computer co
de has been developed and applied to a rotating annulus with square cr
oss section as a base case. The co-axial heat flux from one side wall
to the other was modeled assuming constant temperature distribution at
each wall but at different temperature levels. Additionally the inner
and outer walls were assumed to be adiabatic. The code was first veri
fied for the annulus approaching the plane square cavity in the gravit
ational field, i.e., the ratio of the radius r over the distance h bet
ween outer and inner cylindrical wall was set very large. The results
obtained agree with De Vahl Davis' benchmark solution. By reducing the
inner radius to zero, the results could be compared with Chew's compu
tation of a closed rotating cylinder, and again good agreement was fou
nd. Parametric studies were carried out varying the Grashof number Gr,
the rotational Reynolds number Re, and the r/h ratio, i.e., the curva
ture of the annulus. A decrease of this ratio at constant Gr and Re nu
mber results in a decrease of heat transfer due to the Coriolis forces
attenuating the relative gas velocity. The same effect can be obtaine
d by increasing the Re number with the h/r ratio and the Gr number bei
ng constant. By inserting radial walls into the cavity the influence o
f the Coriolis forces is reduced, resulting in an increase of heat tra
nsfer.