Intercomparison of the spectral characteristics of 200 hPa kinetic energy in some AMIP simulations. PCMDI report No. 23

Technical Report · Sat Jul 01 04:00:00 EDT 1995

DOI:https://doi.org/10.2172/110770· OSTI ID:110770

Boyle, J S

The 200 hPa kinetic energy budget terms are represented by means of their spherical harmonic components for a number of AMIP simulations. The data used are the monthly mean wind fields for 1979 to 1988 decadal simulations. The budget terms are decomposed into the divergent and rotational components. The comparison is limited to the lower wavenumbers so as to be within the nominal limits imposed by the models with the coarsest spatial resolution. The results show considerable differences among the models. The comparison is best for the rotational wind and decades for the divergent components, especially the conversion term. There is some ambiguity among the models as to the sign of some terms at certain wavenumbers. The models tend to overestimate the Walker type (east-west) divergent circulations compared to the Hadley type (north-south) compared to recent NMC and ECMWF operational analyses. The inter-model differences are substantial when viewed in light of the differences in the observational analyses and ensemble differences for the ECMWF model. However, the median values of all the models taken together are usually in fair agreement with observational values.

• Research Organization: Lawrence Livermore National Lab., CA (United States)
• Sponsoring Organization: USDOE, Washington, DC (United States)
• DOE Contract Number: W-7405-ENG-48
• OSTI ID: 110770
• Report Number(s): UCRL-ID--121413; ON: DE96001010
• Country of Publication: United States
• Language: English

Related Subjects

54 ENVIRONMENTAL SCIENCES
99 GENERAL AND MISCELLANEOUS
ATMOSPHERIC CIRCULATION
CLIMATE MODELS
EARTH ATMOSPHERE
KINETIC ENERGY
METEOROLOGY
TESTING