Abstract
We present results of a study of the mid-infrared emission of broad absorption line (BAL)|quasars to determine how they are related to the general population of quasars. We use|the CLUMPY program code to create models of the tori that surround Active Galactic|Nuclei. We compare these models to mid-infrared spectra of both BAL and non-BAL|quasars obtained with the Spitzer Space Telescope. We find the BALQSOs have an|average equivalent width 40% larger and an average MIR-optical luminosity ratio 40%|smaller than the ControlQSOs. We explore the physical meaning behind these results.