Modelling of the twilight sky brightness using a numerical solution of the radiation transfer equation
- 31 December 1996
- journal article
- Published by Elsevier BV in Journal of Atmospheric and Terrestrial Physics
- Vol. 58 (16), 1843-1848
- https://doi.org/10.1016/0021-9169(95)00175-1
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
- Numerical technique for solving the radiative transfer equation for a spherical shell atmosphereApplied Optics, 1994
- A new spherical model for computing the radiation field available for photolysis and heating at twilightPlanetary and Space Science, 1991
- Polar twilight UV‐visible radiation field: Perturbations due to multiple scattering, ozone depletion, stratospheric clouds, and surface albedoPublished by American Geophysical Union (AGU) ,1990
- The troposphere-stratosphere radiation field at twilight: A spherical modelPlanetary and Space Science, 1983
- Multidimensional radiative transfer: Applications to planetary coronaePlanetary and Space Science, 1977
- A mid-latitude ozone model for the 1976 U.S. Standard AtmosphereJournal of Geophysical Research, 1976
- A Global Average Model of Atmospheric Aerosols for Radiative Transfer CalculationsJournal of Applied Meteorology, 1976
- Monte Carlo Studies of the Sky Radiation at TwilightApplied Optics, 1974