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Liou, Kuo-Nan; Freeman, Kenneth P.; Sasamori, Takashi (2011)
Publisher: Co-Action Publishing
Journal: Tellus A
Languages: English
Types: Article

Classified by OpenAIRE into

arxiv: Physics::Atmospheric and Oceanic Physics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Solar and Stellar Astrophysics
Band-by-band calculations are carried out to investigate the solar heating rate and radiative property of the atmosphere containing various combinations of absorbing gases, aerosols and the cloud. The solar spectrum is divided into nine bands according to the location of the absorbing gases which include water vapor, ozone, oxygen and carbon dioxide. The radiation transfer program takes into consideration the inhomogeneity of the cloudy and aerosol atmospheres, the wavelength dependence of solar radiation and the gaseous absorption within scattering layers. A cumulus in the lower troposphere procreates a heating rate as large as 12° C day-1 when the sun is overhead and generates additional heating rates due to ozone in the lower stratosphere. Aerosols are shown to have a pronounced influence on the heating rate of the lower clear atmosphere, but not for coudy conditions. When the sun is close to horizon, the effect of the cloud on the heating rate is shown to be unimportant. We further illustrate that significant under- and overestimation of the atmospheric absorption and reflection, respectively, would be anticipated if the absorption caused by ozone and oxygen is ignored, particularly in cloudy atmospheres.DOI: 10.1111/j.2153-3490.1978.tb00818.x
  • The results below are discovered through our pilot algorithms. Let us know how we are doing!

    • Battan, L. J. & Reitan, C. H. 1957. Droplet size measurement in convective clouds. In Arrzfiial stimulation of rain. London: Pergamon Press.
    • Chandrasekhar, S. 1953. Radiative transfer. New York: Dover Publ.
    • Hale, G. M.& Querry, M.R. 1973. Optical constants of water in the 200 nm to 200 pm wavelength region. Appl. Opt. 12,555-563.
    • Handbook of geophysics 1960. Chapter 16. New York: The Macmillan Company.
    • Howard, J. M.,Burch, D. L. Br Williams, D. 1956. Near infrared transmission through synthetic atmospheres.J. Opt. SOCA.m. 46,186-190.
    • Inn, E. C. & Tanaka, Y. 1953. Absorption coefficient of ozone in the ultraviolet and visible regions. J. Opt. SOCA.m. 43,870-873.
    • Lacis, A. A. & Hansen, J. E. 1974. Parameterization for the absorption of solar radiation in the Earth's atmosphere.J.Afmos.Sci. 31, 118-133.
    • Liou, K. N. 1973. A numerical experiment on Chandrasekhar's discrete-ordinate method for radiative transfer: Applications to cloudy and hazy atmospheres. J.Amos. Sci. 30, 1303-1326.
    • Liou, K. N. 1975. Applications of the discrete-ordinate method for radiative transfer to inhomogeneous aerosol atmosphere. J. Geophys. Res. 80,3434-3440.
    • Liou, K. N. 1976. On the absorption, reflection and transmission ofsolar radiation in cloudy atmosphms. J.Atmos. Sci. 33,798-805.
    • Liou, K. N. & Sasamori, T. 1975. On the transfer of solar radiation in aerosol atmospheres. J. Atmos. Sci. 32,2166-2177.
    • McClatchey, R. A. et al. 1971. Optical properties of the atmosphere.Environmental Res. Pap., 354, AFCRL.
    • Shettle, E. P. 1975. Atmospheric aerosol estimates for atmospheric optical models. Workshop of Remote Sensing of the Marine Boundary Layer, Vail, Colorado.
    • Thekaekara, M.P. 1974. Extraterrestrial solar spectrum, 3000-6100 A at 1 A intervals. Appl. Opt. 13, 318-522.
    • Vigroux, E. 1953. Contributions a I'Etude experimentale de absorption de I'Ozone. Annales de Physique 8, 709-762.
    • Welch, R. & Zdunkowski, W. 1976. A radiation model of the polluted atmospheric boundary layer. J.Amos. Sci. 33,2170-2184.
    • Yamamoto, G. 1962. Direct absorption of solar radiation by atmospheric water vapor, carbon dioxide and molecularoxygen. J.Atmos. Sci. 19, 182-188.
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