Monochromatic, Rosseland mean, and Planck mean opacity routine

Details Monochromatic, Rosseland mean, and Planck mean opacity routine Monochromatic, Rosseland mean, and Planck mean opacity routine

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006asd..soft...25s&link_type=abstract

Astrophysics Software Database, CAU Kiel, Germany (http://www1.astrophysik.uni-kiel.de/asd/).

Astronomy and Astrophysics

Astrophysics

Fortran

Scientific paper

Several FORTRAN77 codes were developed to compute frequency-dependent, Rosseland and Planck mean opacities of gas and dust in protoplanetary disks. The opacities can be computed for an ensemble of dust grains having various compositions (ices, silicates, organics, etc), sizes, topologies (homogeneous/composite aggregates, homogeneous/layered/composite spheres, etc.), porosities, and dust-to-gas ratio. Several examples are available. In addition, a very fast opacity routine to be used in modeling of the radiative transfer in hydro simulations of disks is available upon request (10^8 routine calls require about 30s on Pentium 4 3.0GHz).

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