Three-dimensional atmospheric angular momentum simulated by the Japan Meteorological Agency model for the period of 1955-1994

Citation
I. Naito et al., Three-dimensional atmospheric angular momentum simulated by the Japan Meteorological Agency model for the period of 1955-1994, J METEO JPN, 78(2), 2000, pp. 111-122
Citations number
47
Categorie Soggetti
Earth Sciences
Journal title
JOURNAL OF THE METEOROLOGICAL SOCIETY OF JAPAN
ISSN journal
00261165 → ACNP
Volume
78
Issue
2
Year of publication
2000
Pages
111 - 122
Database
ISI
SICI code
0026-1165(200004)78:2<111:TAAMSB>2.0.ZU;2-V
Abstract
Axial and equatorial atmospheric angular momentum (AAM) functions for the r otational dynamics of the Earth are calculated monthly from ensemble mean d ata of three independent 40-year simulations during 1955-1994 by the global model of the Japan Meteorological Agency (JMA) forced by observed near-glo bal sea surface temperature (SST) conditions. The model results are compare d with those from the reanalysis data of the National Centers for Environme ntal Prediction (NCEP) and the operational objective analysis data of JMA a nd with the functions inferred from the observed length of day (LOD) and po lar motion. The annual term of the simulated axial wind AAM function (dimen sionless relative angular momentum of atmosphere due to zonal wind) during 1984-1994 agrees well with those from the two analysis data sets and roughl y with the inferred function from LOD, while the semi-annual term is consid erably over-estimated, suggesting an incompleteness in the simulated subtro pical zonal winds. The annual term of the simulated equatorial pressure AAM function (dimensionless atmospheric inertia products due to atmospheric ma ss redistribution) is considerably over-estimated with respect to those fro m the two analysis data sets, presumably due to the large simulated redistr ibution of atmospheric mass between the Eurasian continent and the North Pa cific Ocean. For interannual Variations during 1955-1994, only the axial wi nd AAM function is reasonably simulated and shows good agreement with that from NCEP data as well as the Southern Oscillation Index. The above results lead to an understanding that the SST-forced AGCM simulates reasonably the atmospheric axial modes exciting LOD change but not the equatorial (non-ax ial) modes exciting the polar motion.