MC3D: Monte-Carlo 3D Radiative Transfer Code
Sebastian Wolf -
Brief Description
- 3D continuum radiative transfer code - based on the Monte Carlo method
- Self-consistent calculation of the temperature distribution in 3D dust configurations
- Simulation of images, polarization maps, and spectral energy distribution
- Previous and current applications cover the simulation of images, SEDs, and polarization of protoplanetary and debris disks, Bok globules, AGN tori, ...
Download
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The public version of MC3D is available on demand (contact:
).
- An executable for Linux (SuSE 9.0)
- Source Code (Fortran 90), Makefiles, Compiling instructions
- Integrated help files + Example
- Simulation Analysis Tools (IDL)
- S. Wolf, "MC3D - 3D Continuum Radiative Transfer, Version 2", 2003, Comp. Phys. Comm. 150, 99
- S. Wolf, Th. Henning, B. Stecklum, "Multidimensional Self-Consistent Radiative Transfer based on the Monte Carlo Method", 1999, Astron. & Astroph. 349, 839
This version allows to consider 1D/2D/3D configurations (spherical coordinate system).
Those who are already working with the MC3D may want to check for an update of the code the >following page<.
MC3D comes along with
Distribution Policy
If you use this version of MC3D or parts of the code, please refer to
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