# citations = 112
citations vs. year [year,citations]
[2001,3][2002,11][2003,5][2004,5][2005,13][2006,10][2007,2][2008,5][2009,7][2010,9][2011,10][2012,10][2013,9][2014,5][2015,6][2016,2]
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: http://www.stsci.edu/~kgordon/papers/2001ApJ...551..269G.html
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We present the DIRTY (DustI Radiative Transfer, Yeah!) radiative transfer model in this paper and a companion paper. This model computes the polarized radiative transfer of photons from arbitrary distributions of stars through arbitrary distributions of dust using Monte Carlo techniques. The dust re-emission is done self-consistently with the dust absorption and scattering and includes all three important emission paths: equilibrium thermal emission, nonequilibrium thermal emission, and the aromatic features emission. The algorithm used for the radiative transfer allows for the efficient computation of the appearance of a model system as seen from any viewing direction. We present a simple method for computing an upper limit on the output quantity uncertainties for Monte Carlo radiative transfer models that use the weighted photon approach.
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# citations = 112
citations vs. year [year,citations]
[2001,3][2002,11][2003,5][2004,5][2005,13][2006,10][2007,2][2008,5][2009,7][2010,9][2011,10][2012,10][2013,9][2014,5][2015,6][2016,2]
Copyright © 2012 Karl D. Gordon All Rights Reserved