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[ascl:1404.006] TORUS: Radiation transport and hydrodynamics code

TORUS is a flexible radiation transfer and radiation-hydrodynamics code. The code has a basic infrastructure that includes the AMR mesh scheme that is used by several physics modules including atomic line transfer in a moving medium, molecular line transfer, photoionization, radiation hydrodynamics and radiative equilibrium. TORUS is useful for a variety of problems, including magnetospheric accretion onto T Tauri stars, spiral nebulae around Wolf-Rayet stars, discs around Herbig AeBe stars, structured winds of O supergiants and Raman-scattered line formation in symbiotic binaries, and dust emission and molecular line formation in star forming clusters. The code is written in Fortran 2003 and is compiled using a standard Gnu makefile. The code is parallelized using both MPI and OMP, and can use these parallel sections either separately or in a hybrid mode.

Code site:
http://www.astro.ex.ac.uk/people/th2/torus_html/homepage.html
Used in:
http://adsabs.harvard.edu/abs/2012MNRAS.422..241A
Described in:
http://adsabs.harvard.edu/abs/2000MNRAS.315..722H
Bibcode:
2014ascl.soft04006H

Views: 1961

ascl:1404.006
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