A new spherical model for computing the radiation field available for photolysis and heating at twilight
- 1 May 1991
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 39 (5) , 671-683
- https://doi.org/10.1016/0032-0633(91)90061-e
Abstract
No abstract availableKeywords
This publication has 9 references indexed in Scilit:
- Uncertainties in total ozone amounts inferred from zenith sky observations: Implications for ozone trend analysesJournal of Geophysical Research: Atmospheres, 1990
- Optimum spectral resolution for computing atmospheric heating and photodissociation ratesPlanetary and Space Science, 1990
- Radiative Energy Budget in the Cloudy and Hazy ArcticJournal of the Atmospheric Sciences, 1989
- Numerically stable algorithm for discrete-ordinate-method radiative transfer in multiple scattering and emitting layered mediaApplied Optics, 1988
- Photodissociation in the atmosphere: 1. Actinic flux and the effects of ground reflections and cloudsJournal of Geophysical Research: Atmospheres, 1987
- The theory of multiple scattering of radiation in plane parallel atmospheresReviews of Geophysics, 1986
- The troposphere-stratosphere radiation field at twilight: A spherical modelPlanetary and Space Science, 1983
- A New Look at the Discrete Ordinate Method for Radiative Transfer Calculations in Anisotropically Scattering AtmospheresJournal of the Atmospheric Sciences, 1981
- Extension of the doubling method to inhomogeneous sourcesJournal of Quantitative Spectroscopy and Radiative Transfer, 1976