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  Kinetic energy spectrum of horizontal motions in middle-atmosphere models

Koshyk, J., Boville, B., Hamilton, K., Manzini, E., & Shibata, K. (1999). Kinetic energy spectrum of horizontal motions in middle-atmosphere models. Journal of Geophysical Research-Atmospheres, 104, 27177-27190. doi:10.1029/1999JD900814.

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Koshyk_et_al-1999-JGR.pdf (Publisher version), 2MB
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 Creators:
Koshyk, J.N.1, Author
Boville, B.A.1, Author
Hamilton, K.1, Author
Manzini, Elisa2, Author                 
Shibata, K1, Author
Affiliations:
1external, ou_persistent22              
2MPI for Meteorology, Max Planck Society, Bundesstraße 53, 20146 Hamburg, DE, ou_913545              

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Free keywords: GENERAL-CIRCULATION MODEL; GRAVITY-WAVES; PARAMETERIZATION; STRATOSPHERE; TURBULENCE; TROPOSPHERE; CONVECTION; SIMULATION; REPRESENTATION; CLIMATOLOGY
 Abstract: Data from several middle-atmosphere general circulation models are used to calculate kinetic energy spectra as a function of total horizontal wavenumber n. The horizontal and vertical resolution between models varies but all have upper. boundaries at heights greater than or similar to 80 km. Tropospheric spectra show power-law behavior with slopes slightly shallower than -3 for wavenumbers n greater than or similar to 10 (horizontal wavelengths less than or similar to 4000 km) and are dominated by the rotational part of the flow. These spectra agree well with those calculated using data obtained from a global assimilation model and with the results of previous observational studies. Stratospheric spectra have larger amplitudes than tropospheric ones at planetary scales and smaller amplitudes at smaller scales. Mesospheric spectra are characterized by enhanced spectral amplitudes at all wavenumbers compared to the stratosphere and spectral slopes in the wavenumber range n greater than or similar to 10 are generally shallower. Stratospheric and mesospheric spectra include approximately equal contributions from the rotational and divergent parts of the flow for n greater than or similar to 20 in all models. These features appear to be independent of model resolution. The divergent part of the flow, presumably associated with explicitly resolved inertiogravity waves in the models, increases more rapidly with height above the lower stratosphere than the rotational part. The divergent part is fairly insensitive to season, whereas the rotational part changes considerably between January and July in the middle-atmosphere region. Spectral amplitudes and vertical growth rates of both parts vary widely between models for a given season. The horizontal diffusion schemes used by the models are compared in an attempt to explain some of these differences.

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Language(s): eng - English
 Dates: 1999
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: ISI: 000083874700001
DOI: 10.1029/1999JD900814
 Degree: -

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Title: Journal of Geophysical Research-Atmospheres
Source Genre: Journal
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Publ. Info: Washington, D.C. : American Geophysical Union
Pages: - Volume / Issue: 104 Sequence Number: - Start / End Page: 27177 - 27190 Identifier: ISSN: 0148-0227
CoNE: https://pure.mpg.de/cone/journals/resource/991042728714264_1