Sample input.par files for STOKES are given below. For a more detailed description and details of the dust models see the manual.
example1-input.par: 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..
example2-input.par: 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.
example3.input.par: 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
