TROPICAL GRAVITY-WAVES AND SUPERCLUSTERS SIMULATED BY HIGH-HORIZONTAL-RESOLUTION SKYHI GENERAL-CIRCULATION MODELS

Citation
Y. Hayashi et al., TROPICAL GRAVITY-WAVES AND SUPERCLUSTERS SIMULATED BY HIGH-HORIZONTAL-RESOLUTION SKYHI GENERAL-CIRCULATION MODELS, Journal of the Meteorological Society of Japan, 75(6), 1997, pp. 1125-1139
Citations number
50
ISSN journal
00261165
Volume
75
Issue
6
Year of publication
1997
Pages
1125 - 1139
Database
ISI
SICI code
0026-1165(1997)75:6<1125:TGASSB>2.0.ZU;2-Q
Abstract
Tropical gravity waves and superclusters simulated by 40-level GFDL SK YHI general circulation model experiments with higher horizontal resol utions (0.6 degrees longitude x 0.72 degrees latitude) and (1.0 degree s x 1.2 degrees) are compared with those simulated by a lower-resoluti on (3.0 degrees x 3.6 degrees) experiment. Results indicated that simu lated precipitational heating appears to excite tropical gravity waves . At higher resolutions, precipitation is more confined in space and t ime, resulting in a broader wavenumber-frequency spectral distribution . Grid-scale precipitation, which is thought to mimic the precipitatio n associated with cloud clusters, is organized into larger-scale super clusters. The westward propagation of cloud clusters and eastward prop agation of superclusters can be more clearly seen in the high-resoluti on experiments. The high-resolution (0.6 degrees x 0.72 degrees) model indicates that the lower-stratospheric gravity-wave momentum flux is dominated by high-frequency components having periods shorter than one day. This flux doubles as the resolution is increased from (3.0 degre es x 3.6 degrees) to (0.6 degrees x 0.72 degrees). It is speculated th at a further increase in both the horizontal and vertical resolutions could substantially enhance the gravity-wave momentum flux convergence , thus forcing a stronger quasi-biennial oscillation.