The warm Chaplygin inflationary universe model in the context of the effective field theory of loop quantum cosmology (LQC) is studied. In the slow-roll phase of inflation primordial perturbation spectrums, tensor-to-scalar ratio and spectral indices of our model are presented. Using chaotic potential, we present the main characteristics of this model in great detail. The parameters of the model are restricted by recent observational results i.e. WMAP9 and Planck data.
