“…Relatively few studies have deal with solar reactor modeling and simulation (Abanades et al, 2007;Agrafiotis et al, 2007;Petrasch and Steinfeld, 2007;Kogan et al, 2007;Palumbo et al, 2004;Meier et al, 1996). Some of those studies have been focused on radiative heat transfer within particle suspension exposed to concentrated solar radiation, included, steady state models based on the discrete ordinates methods, Monte Carlo (MC) methods and transient models based on the MC and Rosseland approximations and diffusion approach (Evans et al, 1987;Miller and Koenigsdorff, 1991;Mischler and Steinfeld, 1995;Hirsch and Steinfeld, 2004b;Osinaga et al, 2004;Lipinski and Steinfeld, 2004;Dombrovsky, 2002;Dombrovsky et al, 2007;Klein et al, 2007;Müller and Steinfeld, 2007). Other models and simulations have been developed in order to describe the temperature profile in the reactor and to have a multiphase flow method in the case of solid particle dissociation reaction (Abanades et al, 2007) and for the description of the thermochemical cycles for hydrogen production inside a honeycomb monolithic reactor under the influx of solar radiation on its front face (Agrafiotis et al, 2007;2005).…”