STOKES
Modeling Radiative Transfer and Polarization

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Sample input.par files for STOKES are given below. For a more detailed description and details of the dust models see the manual.


1) Modeling continuum radiation coming from an electron-dominated disk inside the funnel of a dusty torus. The dust composition for the torus is based on observations of Active Galactic Nuclei..
example1-input-v1.0.par
example1-input-v1.2.par



2) Modeling continuum and Ha line emission for an electron disk with polar outflow and a surrounding broad line region. Farther out, a dusty narrow line region is present, its dust composition is based on observations of the Milky Way.
example2-input-v1.0.par
example2-input-v1.2.par



3) Modeling [OIII] line emission coming from a point-source at the center of an expanding electron shell. The shell is surrounded by a few singular dust clouds. Their dust composition is based on observations of the Milky Way
example3.input-v1.0.par
example3.input-v1.2.par


4) Modeling a radiation-supported, equatorial Thomson scattering disk with a flared geometry. The model is run in imaging mode and produces 30x30 pixel images of the total flux and polarization properties.
example4.input-v1.2.par