A new numerical model to compute photolysis rates and solar heating with anisotropic scattering in spherical geometry

Annales Geophysicae

Volumn 14, Issue 1, 1996, Pages 80-97

  Balluch, M ^a  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 2842556987     PISSN: 09927689     EISSN: None     Source Type: Journal    
DOI: 10.1007/s00585-996-0080-0     Document Type: Article

References (7)

1. Anderson, D. E., The troposphere-stratosphere radiation field at twilight: a spherical model, Planet. Space Sci., 31, 1517, 1983.
2. Anderson, D. E., and S. A. Lloyd, Polar twilight UV-visible radiation field: perturbations due to multiple scattering, ozone depletion, stratospheric clouds, and surface albedo, JGR, 95, D6, 7429-7434, 1990.
3. Balhich, M., and D. J. Lary, Reply to the comments on 'solar heating rates: the importance of spherical geometry', J. Atmos. Sci., 52, 3, 1995.
4. Bohren, C. F., and D. R. Huffman, Absorption and scattering of light by small particles, New York, Chichester, J. Wiley and Sons, 1983.
5. Dahlback, A., and K. Stamnes, A new spherical model for computing the radiation field available for photolysis and heating at twilight, Planet. Space Sci., 39, 671-683, 1991.
6. Lary, D. J., and M. Balluch, Solar heating rates: the importance of spherical geometry, J. Atmos. Sci., 50, 3983-3993, 1993.
7. 2 absorption, Q. J. R. Meteorol. Soc., 120, 1683-1688, 1994.