A new spherical model for computing the radiation field available for photolysis and heating at twilight

Planetary and Space Science

Volumn 39, Issue 5, 1991, Pages 671-683

  Dahlback, Arne ^a   Stamnes, Knut ^b  

^a NORWEGIAN INSTITUTE FOR AIR RESEARCH   (Norway)

^b UNIVERSITY OF ALASKA FAIRBANKS   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 34250006925     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/0032-0633(91)90061-E     Document Type: Article

References (19)

1. The troposphere-stratosphere radiation field at twilight: a spherical model
2. Nonlocal perturbation techniques in radiative transfer
3. Photodissociation in the atmosphere 1 Actinic flux and the effects of ground reflections and clouds
4. The theory of multiple scattering of radiation in plane parallel atmospheres
5. Uncertainties in total ozone amounts inferred from zenith sky observations: implications for ozone trend analyses
6. Uncertainties in total ozone amounts inferred from zenith sky observations: implications for ozone trend analyses
7. A new look at the discrete ordinate method for radiative transfer calculations in anisotropically scattering atmospheres
8. Optimum spectral resolution for computing atmospheric heating and photo-dissociation rates
9. Numerically stable algorithm for discrete-ordinate-method radiative transfer in multiple scattering and emitting layered media
10. Radiative energy budget in the cloudy and hazy Arctic
11. Extension of the doubling method to inhomogeneous sources