SPEC3D: a three-dimensional radiative transfer code for astrophysical and laboratory applications

Details SPEC3D: a three-dimensional radiative transfer code for astrophysical and laboratory applications SPEC3D: a three-dimensional radiative transfer code for astrophysical and laboratory applications

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sf2a.conf..485i&link_type=abstract

SF2A-2011: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: G. Alecian, K. Belkacem,

Astronomy and Astrophysics

Astrophysics

Radiative Transfer, Quantitative Spectroscopy, Methods: Numerical, Laboratory Astrophysics, Shock Waves

Scientific paper

We have developed a generic three-dimensional radiative transfer code, SPEC3D, aimed at post-processing 3D radiation magnetohydrodynamics simulations. SPEC3D solves the monochromatic 3D radiative transfer equation. The numerical approach and the major features of the code are presented. The wide range of applications includes the modeling of a number of astrophysical objects and structures, such as accretion shocks around young stellar objects, stellar and exoplanets atmospheres, cosmological structures, but also the modeling of laboratory astrophysics experiments such as magnetohydrodynamics jets and radiative shocks.

Affiliated with

Also associated with

No associations

Rating

SPEC3D: a three-dimensional radiative transfer code for astrophysical and laboratory applications does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with SPEC3D: a three-dimensional radiative transfer code for astrophysical and laboratory applications, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SPEC3D: a three-dimensional radiative transfer code for astrophysical and laboratory applications will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1439564