Finite-time instabilities of lower-stratospheric flow
The linear structures that produce the most in situ energy growth in the lower stratosphere for realistic wintertime flows are investigated using T21 and T42 calculations with the ECMWF 19-level forecast model. Significant growth is found for relatively large scale structures that grow by propagatin...
| Main Authors: | , , |
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| Format: | Journal article |
| Language: | English |
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1996
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| _version_ | 1797072783053684736 |
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| author | Hartmann, D Palmer, T Buizza, R |
| author_facet | Hartmann, D Palmer, T Buizza, R |
| author_sort | Hartmann, D |
| collection | OXFORD |
| description | The linear structures that produce the most in situ energy growth in the lower stratosphere for realistic wintertime flows are investigated using T21 and T42 calculations with the ECMWF 19-level forecast model. Significant growth is found for relatively large scale structures that grow by propagating from the outer edges of the vortex into the strong jet features of the lower-stratospheric flow. The growth is greater when the polar vortex is more asymmetric and contains localized jet structures. If the linear structures are properly phased, they can induce strong nonlinear interactions with the polar vortex, both for Northern Hemisphere and Southern Hemisphere flow conditions, even when the initial amplitudes are small. Large extensions from the main polar vortex that are peeled off during wave-breaking events give rise to a separate class of rapidly growing disturbances that may hasten the mixing of these vortex extensions. |
| first_indexed | 2024-03-06T23:12:41Z |
| format | Journal article |
| id | oxford-uuid:6608e31e-3ecc-4a43-a317-207facbade96 |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-06T23:12:41Z |
| publishDate | 1996 |
| record_format | dspace |
| spelling | oxford-uuid:6608e31e-3ecc-4a43-a317-207facbade962022-03-26T18:29:19ZFinite-time instabilities of lower-stratospheric flowJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:6608e31e-3ecc-4a43-a317-207facbade96EnglishSymplectic Elements at Oxford1996Hartmann, DPalmer, TBuizza, RThe linear structures that produce the most in situ energy growth in the lower stratosphere for realistic wintertime flows are investigated using T21 and T42 calculations with the ECMWF 19-level forecast model. Significant growth is found for relatively large scale structures that grow by propagating from the outer edges of the vortex into the strong jet features of the lower-stratospheric flow. The growth is greater when the polar vortex is more asymmetric and contains localized jet structures. If the linear structures are properly phased, they can induce strong nonlinear interactions with the polar vortex, both for Northern Hemisphere and Southern Hemisphere flow conditions, even when the initial amplitudes are small. Large extensions from the main polar vortex that are peeled off during wave-breaking events give rise to a separate class of rapidly growing disturbances that may hasten the mixing of these vortex extensions. |
| spellingShingle | Hartmann, D Palmer, T Buizza, R Finite-time instabilities of lower-stratospheric flow |
| title | Finite-time instabilities of lower-stratospheric flow |
| title_full | Finite-time instabilities of lower-stratospheric flow |
| title_fullStr | Finite-time instabilities of lower-stratospheric flow |
| title_full_unstemmed | Finite-time instabilities of lower-stratospheric flow |
| title_short | Finite-time instabilities of lower-stratospheric flow |
| title_sort | finite time instabilities of lower stratospheric flow |
| work_keys_str_mv | AT hartmannd finitetimeinstabilitiesoflowerstratosphericflow AT palmert finitetimeinstabilitiesoflowerstratosphericflow AT buizzar finitetimeinstabilitiesoflowerstratosphericflow |