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We have adapted Coupled Escape Probability, a new exact method of solvingradiative transfer problems, for use in asymmetrical spherical situations. Ourmodel is intended specifically for use in modeling optically thick cometarycomae, although not limited to such use. This method enables the accuratemodeling of comets' spectra even in the potentially optically thick regionsnearest the nucleus, such as those seen in Deep Impact observations of9P/Tempel 1 and EPOXI observations of 103P/Hartley 2.

Coupled Escape Probability for an Asymmetric Spherical Case: Modeling Optically Thick Comets