I n t r o d u c t o r y n o t e s
|
Approach | Applicability range | Speed | Accuracy | Source and dust configurations | Polarized radiation |
---|---|---|---|---|---|
Single scattering approximation (tau<<1) | tau < 0.1-0.5 (depends on albedo, g) | very fast (depends on albedo, g or scatterer shape?) | may be not accurate | any 3D configuration | yes |
Double scattering approximation | tau<1 (depends on albebo, g?) | rather fast | not very accurate | any 3D configuration | yes |
Lambda-iteration mathod (generalization of 1,2,...-scattering approximations) | taumax ~ albedo, g? | quick (if number scattering is small) | depends on the numbers of itarations and scatterings? | any 3D configuration | yes |
Numerical methods developed for a given geometry | any tau | not fast | not very exact? | usually 1D configurations | no |
Grid-point methods | ? | very slow | ? | 3D configurations | yes |
Monte Carlo method | tau about 1-100? | not fast (depends on tau and configuration) | not very accurate | any 3D configuration | yes |
Author(s) | Method | Particles | Geometry | Output | Applications |
Leung [1976] | MoM, quasi-diffusion approximation | homogeneous and coated spheres | 1D (sphere) | intensity, SED | dust clouds with central source, CS shells |
Witt [1977] | MC | spheres, HG phase function | plane-parallel layer | intensity | RN |
White [1979] | Doubling method | MRN mixture | homogeneous layer (optically thick but geometrically thin) | intensity, polarization | RN |
Daniel [1980] | MC | single size spheres | homogeneous sphere | polarization | cool stars |
Yorke [1980] | MoM | single size spheres | 1D (sphere), isotropic scattering | SED | cocoon stars |
Rowan-Robinson [1980] | Ray tracing method | single size homogeneous and coated spheres | 1D (inhomogeneous sphere), isotropic scattering | SED, intensity profiles | hot-centred interstellar clouds, M giants and supergiants |
Lefevre et al. [1982] | MC | graphite and silicate spheres | inhomogeneous sphere, anisotropic scattering | SED | late-type stars |
Lefevre et al. [1983] | MC | graphite and silicate spheres | homogeneous ellipsoid, anisotropic scattering | SED,images | young and late-type stars |
Warren-Smith [1983] | MC | spheres of different sizes | plane layers | surface brightness, polarization | RN |
Spagna and Leung [1983] | Newton-Raphson iterative scheme | spheres (up to 5 constituents) | 1D (homogeneous sphere) | SED | CS shells, clouds |
Rogers and Martin [1986] | Half-range MoM | spheres | 1D (sphere) with power density distribution | SED | CS shells (IRC +10 216) |
Chini et al. [1986] | MoM | MRN mixture | 1D (sphere) with power density distribution | SED | CS shells |
Wolfire and Cassinelli [1986] | Modified MoM | MRN mixture | 1D (sphere) with power density distribution | SED | protostars |
Spagna and Leung [1987] | MoM, quasi-diffusion approximation | homogeneous and coated spheres | 2D (disks) | intensity, SED | disk dust clouds, CS disks, disk galaxies |
Bastien and Menard [1988] | MC | spheres | 3D, arbitrary geometry, inhomogeneous density distribution | images, polarization maps | YSO, CS shells |
Egan et al. [1988] | Updated and comprehensive versions of codes of Leung [1976] and Spagna and Leung [1983] for one-dimensional geometries (sphere, plane-parallel, cylindrical) | ||||
Efstathiou and Rowan-Robinson [1990] | Ray tracing method | single and multi-component mixtures of spheres | 2D axisymmetric inhomogeneous configurations (disks, ellipsoids, tori) | SED | late type stars, AGN |
Hoefflich [1991] | MC | Thomson scattering | axisymmetric photospheres | polarization | SN 1987A |
Collison and Fix [1991] | Iterative scheme | single size silicate spheres | 2D axisymmetric inhomogeneous shells, isotropic scattering | SED, images | CS shells |
Whitney and Hartmann [1992] | MC | spheres, HG phase function | 3D (disks) | images, polarization maps | PMS objects |
Pier and Krolik [1992] | Multi-dimensional Newton-Raphson technique | MRN mixture | 2D (homogeneous torus) | SED | AGN, Seyfert galaxies |
Bosma [1993a], [1993b] | New iterative scheme in MoM | anisotropic scattering, randomly oriented particles | 1D (sphere) | intensity and polarization | |
Fischer [1993] | MC | MRN mixture | 3D, arbitrary geometry, inhomogeneous density distribution | images, polarization maps | protostellar sources |
Groenewegen [1993] | Iterative scheme | spheres | 1D (sphere) with power density distribution, isotropic scattering, determination of inner radius as dust condensation boundary | SED | shells around AGB stars |
Voshchinnikov and Karjukin [1994] | MC, method of symmetrized trajectories | spheres (Rayleigh, MRN mixture) | 2D (inhomogeneous spheroid) | intensity, polarization | CS shells around young stars |
Code and Whitney [1995] | MC | electrons, spherical particles | 3D (illuminated spherical blobs) | intensity, polarization | supergiants, RCB stars, DGL, RN |
Sonnhalter et al. [1995] | Frequency dependent flux-limited diffusion approximation | mixture of carbon, silicate and silicate-ice spheres | 2D axially-symmetric dusty disks with different density distribution | intensities, images at different wavelengths | |
Lopez et al. [1996] | MC | carbon spheres | inhomogeneous axisymmetric shell, anisotropic scattering | SED, images | AGB stars, Red Rectangle |
Steinacker and Henning [1996]1 | Direct solution to discretized radiative transfer equation | spheres | 3D arbitrary configuration | SED, images | CS shells, YSO |
Men'shchikov and Henning [1997] | MoM | spheres of different sizes and materials | 2D axially-symmetric CS disks with arbitrary density distribution | SED, images | CS shells, YSO |
Ivezic and Elitzur [1997] | Numerical integration | spheres (6 types of materials and 2 size distributions) | 1D (sphere and plane-parallel slab) | SED | CS shells, clouds, YSO |
Varosi and Dwek [1999] | Analytical approximation and MC | spheres | spherically-symmetric two-phase clumpy medium | fluxes | star-forming regions, starburst galaxies |
Wolf and Henning [2000] | MC including calculations of dust temperature | spheres of different sizes and materials | 3D, arbitrary number, shape and geometrical configuration of illuminating sources and dust density distribution | SED, images, polarization maps | CS shells, YSO, AGN |
Gordon et al. [2001] and Misselt et al. [2001] | MC | mixture of carbonaceous and silicate grains, polycyclic aromatic hydrocarbons (PAHs) | 3D, arbitrary distribution of stars and dust | SED, images, polarization maps | RN, clusters of stars, galaxies |
Wolf et al. [2002] 1 | Dissemination of MC code of Wolf and Henning [2000] on non-spherical particles |
Notes: 1. First results only. 2. All notations are explained in the text above the table. |