NUMERICAL SIMULATIONS OF THE MADDEN AND JULIAN OSCILLATION
The structure of the disturbances resembles a Kelvin wave, although the speed of propagation is slower than anticipated from theory as applied to a dry atmosphere. However, a simple model of the tropical atmosphere demonstrates that the wave speed is sensitive to moisture effects. This notion is con...
| Main Authors: | , , |
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| Format: | Journal article |
| Language: | English |
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1988
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| _version_ | 1797073508579147776 |
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| author | Swinbank, R Palmer, T Davey, M |
| author_facet | Swinbank, R Palmer, T Davey, M |
| author_sort | Swinbank, R |
| collection | OXFORD |
| description | The structure of the disturbances resembles a Kelvin wave, although the speed of propagation is slower than anticipated from theory as applied to a dry atmosphere. However, a simple model of the tropical atmosphere demonstrates that the wave speed is sensitive to moisture effects. This notion is confirmed by two further general circulation model experiments in which the latent heat release is increased; in both cases the intrinsic speed of the wave is reduced in inverse proportion to the vertical gradient of equivalent potential temperature. The time-mean circulation of the basic aqua-planet integration exhibits some unusual features; for example a double Hadley cell, with ascending branches displaced some 15° either side of the equator. Dynamical reasons for the maintenance of the aqua-planet circulations are discussed, since these shed some light on the general circulation of the earth's atmosphere. -from Authors |
| first_indexed | 2024-03-06T23:23:12Z |
| format | Journal article |
| id | oxford-uuid:697bca46-c0ec-4ad4-b028-2bd6ac6489c2 |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-06T23:23:12Z |
| publishDate | 1988 |
| record_format | dspace |
| spelling | oxford-uuid:697bca46-c0ec-4ad4-b028-2bd6ac6489c22022-03-26T18:51:19ZNUMERICAL SIMULATIONS OF THE MADDEN AND JULIAN OSCILLATIONJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:697bca46-c0ec-4ad4-b028-2bd6ac6489c2EnglishSymplectic Elements at Oxford1988Swinbank, RPalmer, TDavey, MThe structure of the disturbances resembles a Kelvin wave, although the speed of propagation is slower than anticipated from theory as applied to a dry atmosphere. However, a simple model of the tropical atmosphere demonstrates that the wave speed is sensitive to moisture effects. This notion is confirmed by two further general circulation model experiments in which the latent heat release is increased; in both cases the intrinsic speed of the wave is reduced in inverse proportion to the vertical gradient of equivalent potential temperature. The time-mean circulation of the basic aqua-planet integration exhibits some unusual features; for example a double Hadley cell, with ascending branches displaced some 15° either side of the equator. Dynamical reasons for the maintenance of the aqua-planet circulations are discussed, since these shed some light on the general circulation of the earth's atmosphere. -from Authors |
| spellingShingle | Swinbank, R Palmer, T Davey, M NUMERICAL SIMULATIONS OF THE MADDEN AND JULIAN OSCILLATION |
| title | NUMERICAL SIMULATIONS OF THE MADDEN AND JULIAN OSCILLATION |
| title_full | NUMERICAL SIMULATIONS OF THE MADDEN AND JULIAN OSCILLATION |
| title_fullStr | NUMERICAL SIMULATIONS OF THE MADDEN AND JULIAN OSCILLATION |
| title_full_unstemmed | NUMERICAL SIMULATIONS OF THE MADDEN AND JULIAN OSCILLATION |
| title_short | NUMERICAL SIMULATIONS OF THE MADDEN AND JULIAN OSCILLATION |
| title_sort | numerical simulations of the madden and julian oscillation |
| work_keys_str_mv | AT swinbankr numericalsimulationsofthemaddenandjulianoscillation AT palmert numericalsimulationsofthemaddenandjulianoscillation AT daveym numericalsimulationsofthemaddenandjulianoscillation |