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January and July Simulations with a Spectral General Circulation Model

The authors describe the results of Jan. and July simulations conducted with a nine-level spectral model by using a rhomboidal truncation at wavenumber 15. Sea surface temperature, sea-ice distribution, and solar zenith angle are held constant in each simulation. The model includes interactive cloud...

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Bibliographic Details
Published in:Journal of the atmospheric sciences 1983-01, Vol.40 (3), p.580-604
Main Authors: Pitcher, Eric J., Malone, Robert C., Ramanathan, V., Blackmon, Maurice L., Puri, Kamal, Bourke, William
Format: Article
Language:English
Online Access:Get full text
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Summary:The authors describe the results of Jan. and July simulations conducted with a nine-level spectral model by using a rhomboidal truncation at wavenumber 15. Sea surface temperature, sea-ice distribution, and solar zenith angle are held constant in each simulation. The model includes interactive clouds and radiative processes after Ramanathan et al. (1983). Selected fields are shown which highlight the model's strengths and weaknesses. The latitude-height distribution of the zonal wind is successfully simulated. The model captures the separation between the wintertime westerly jets in the troposphere and stratosphere and, thus, simulates the sign reversal in the vertical wind shear across the jet axis in the upper troposphere. In addition to the zonal wind, the zonally averaged temperature, meridional wind, and vertical velocity are also shown. Regional distributions of sea level pressure, surface air temperature, precipitation, and a number of other fields defined at various pressure levels are compared with observations. For the most part, the large-scale features of the observed general circulation are successfully simulated, although the sea level pressure in the subtropics over continental regions in the wintertime is higher than observed, and the model atmosphere tends to be a few degrees colder than observed. A partial explanation for this last deficiency is given. There is good agreement between the model stratosphere and the actual stratosphere. Preliminary indications suggest that the variability present in the model is comparable to that found in the atmosphere.
ISSN:0022-4928
1520-0469
DOI:10.1175/1520-0469(1983)040<0580:JAJSWA>2.0.CO;2