Statistics – Computation
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...350..801b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 350, Feb. 20, 1990, p. 801-818. Research supported by CNRS.
Statistics
Computation
2
Planetary Atmospheres, Radiative Transfer, Three Dimensional Models, Computational Astrophysics, Fourier Series, Radiation Distribution, Transport Properties
Scientific paper
A method for solving the three-dimensional equation of transfer for an inhomogeneous static medium is described. The resolution of the three-dimensional transfer equation is important for studying the planetary atmosphere where an accurate model of the radiation field near the terminator region and in the nightside is necessary. The procedure involves: the reduction of the three-dimensional equation to a one-dimensional equation system; the resolution of this system by the discrete ordinate method, and reconstruction of the three-dimensional radiation field. This method considers variations in atmospheric parameters and reflectance at the bottom of the atmosphere relative to spatial and frequency parameters.
Ben Jaffel Lotfi
Vidal-Madjar Alfred
No associations
LandOfFree
A new method for the resolution of the radiative transfer equation in three-dimensional geometry. I - Theory 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 A new method for the resolution of the radiative transfer equation in three-dimensional geometry. I - Theory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A new method for the resolution of the radiative transfer equation in three-dimensional geometry. I - Theory will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1841521