Spectroscopic Hinode Observables from Turbulent Heating and Cooling of Coronal Loops

We present a model of coronal loop turbulence allowing the fast computation of heating in a loop at high Reynolds numbers. We also consider the coupling of both heating and cooling processes in loops, including for the first time a feedback of the cooling on the heating: the heating computed by the shell-models used as an input of a hydrodynamic model of a loop with thermal conduction and a self-consistent treatment of radiation. We forward-model spectroscopic variables that can be compared to Hinode observations.