| contributor author | Hayashi, Yoshikazu | |
| date accessioned | 2017-06-09T14:22:18Z | |
| date available | 2017-06-09T14:22:18Z | |
| date copyright | 1981/06/01 | |
| date issued | 1981 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-18142.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4154115 | |
| description abstract | In order to explain why the Aleutian high stands out in the winter stratosphere, a complex Fourier analysis is made of simulated and observed stationary waves. It is found that in the troposphere the envelope of the time mean geopotential height consisting of wavenumbers 1 ? 3 attains its major and minor maxima in the Pacific and Atlantic, respectively. The major maximum is dominated by wavenumbers 1 ? 2 and shifts eastward with height in the stratosphere in the approximate direction of the group velocity and strengthens the Aleutian high. The minor maximum is dominated by wavenumber 3 and is confined in the troposphere. | |
| publisher | American Meteorological Society | |
| title | Vertical-Zonal Propagation of a Stationary Planetary Wave Packet | |
| type | Journal Paper | |
| journal volume | 38 | |
| journal issue | 6 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/1520-0469(1981)038<1197:VZPOAS>2.0.CO;2 | |
| journal fristpage | 1197 | |
| journal lastpage | 1205 | |
| tree | Journal of the Atmospheric Sciences:;1981:;Volume( 038 ):;issue: 006 | |
| contenttype | Fulltext | |