Abstract
We present preliminary results of a study of the near infrared emission of broad absorption line (BAL) quasars to determine how they are related to the general population of quasars. We will be using the Clumpy program code to create models of the tori that surround Active Galactic Nuclei. We will compare these models to actual spectra obtained through the Spitzer Space Telescope. We intend to determine what effect the orientation and geometrical qualities of the tori have on the spectrum that is collected about the AGN. We will be studying both BAL as well as regular Quasars to ascertain any correlations between the two.