  We investigate the impact of turbulent suppression of parallel heat
conduction on the cooling of post-flare coronal loops. Depending on the value
of the mean free path $\lambda_T$ associated with the turbulent scattering
process, we identify four main cooling scenarios. The overall temperature
evolution, from an initial temperature in excess of $10^7$~K, is modeled in
each case, highlighting the evolution of the dominant cooling mechanism
throughout the cooling process. Comparison with observed cooling times allows
the value of $\lambda_T$ to be constrained, and interestingly this range
corresponds to situations where collision-dominated conduction plays a very
limited role, or even no role at all, in the cooling of post-flare coronal
loops.
