A simple tutorial method, based on a photon tracking procedure, is described to determine the spherical albedo for a thin atmosphere overlying a reflecting surface. This procedure is used to provide a physical structure with which to interpret the more detailed but highly mathematical analyses presented. The final equations are shown to be in good numerical agreement with more exact solutions for thin atmospheres
Accurate values for the intensity and polarization of light reflected and transmitted by optically t...
A new model for computing radiative transfer in a spherically symmetric atmosphere has been develope...
Accurate values for the intensity and polarization of light reflected and transmitted by optically t...
Doubling principle providing rapid and accurate results for problem of diffuse reflection from plane...
We use Ambartsumian's method of addition of layers to show that various problems, including the stan...
We use Ambartsumian's method of addition of layers to show that various problems, including the stan...
A solution is presented to the radiative transfer of the solar irradiation through a turbid atmosphe...
Normalized probability distribution of photon optical paths for radiative transfer equatons to deter...
The fundamental physical and mathematical principles governing the transmission of radiation through...
The research accomplished during this period is briefly summarized. The interior radiances within an...
The direct method for the solution of the spherical harmonics approximation to the equation of trans...
Dissertation (Ph.D.) University of Alaska Fairbanks, 1992The equation for radiation transport in ver...
Two stream methods provide rapid approximate calculations of radiative transfer in scattering and ab...
The complete radiation field is calculated for scattering layers of various optical thicknesses. Res...
Ground specular reflection modification of light scattering from planetary atmosphere to
Accurate values for the intensity and polarization of light reflected and transmitted by optically t...
A new model for computing radiative transfer in a spherically symmetric atmosphere has been develope...
Accurate values for the intensity and polarization of light reflected and transmitted by optically t...
Doubling principle providing rapid and accurate results for problem of diffuse reflection from plane...
We use Ambartsumian's method of addition of layers to show that various problems, including the stan...
We use Ambartsumian's method of addition of layers to show that various problems, including the stan...
A solution is presented to the radiative transfer of the solar irradiation through a turbid atmosphe...
Normalized probability distribution of photon optical paths for radiative transfer equatons to deter...
The fundamental physical and mathematical principles governing the transmission of radiation through...
The research accomplished during this period is briefly summarized. The interior radiances within an...
The direct method for the solution of the spherical harmonics approximation to the equation of trans...
Dissertation (Ph.D.) University of Alaska Fairbanks, 1992The equation for radiation transport in ver...
Two stream methods provide rapid approximate calculations of radiative transfer in scattering and ab...
The complete radiation field is calculated for scattering layers of various optical thicknesses. Res...
Ground specular reflection modification of light scattering from planetary atmosphere to
Accurate values for the intensity and polarization of light reflected and transmitted by optically t...
A new model for computing radiative transfer in a spherically symmetric atmosphere has been develope...
Accurate values for the intensity and polarization of light reflected and transmitted by optically t...