Hyperbolic lines and the stratospheric polar vortex
The necessary and sufficient conditions for Lagrangian hyperbolicity recently derived in the literature are reviewed in the light of older concepts of effective local rotation in strain coordinates. In particular, we introduce the simple interpretation of the necessary condition as a constraint on t...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.1082.1377 2023-05-15T14:01:06+02:00 Hyperbolic lines and the stratospheric polar vortex Tieh-Yong Koh Bernard Legras The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1082.1377 http://www.lmd.ens.fr/legras/publis/chaos2002.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1082.1377 http://www.lmd.ens.fr/legras/publis/chaos2002.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.lmd.ens.fr/legras/publis/chaos2002.pdf text ftciteseerx 2020-05-03T00:26:20Z The necessary and sufficient conditions for Lagrangian hyperbolicity recently derived in the literature are reviewed in the light of older concepts of effective local rotation in strain coordinates. In particular, we introduce the simple interpretation of the necessary condition as a constraint on the local angular displacement in strain coordinates. These mathematically rigorous conditions are applied to the winter stratospheric circulation of the southern hemisphere, using analyzed wind data from the European Center for Medium-Range Weather Forecasts. Our results demonstrate that the sufficient condition is too strong and the necessary condition is too weak, so that both conditions fail to identify hyperbolic lines in the stratosphere. However a phenomenological, nonrigorous, criterion based on the necessary condition reveals the hyperbolic structure of the flow. Another ͑still nonrigorous͒ alternative is the finite-size Lyapunov exponent ͑FSLE͒ which is shown to produce good candidates for hyperbolic lines. In addition, we also tested the sufficient condition for Lagrangian ellipticity and found that it is too weak to detect elliptic coherent structures ͑ECS͒ in the stratosphere, of which the polar vortex is an obvious candidate. Yet, the FSLE method reveals a clear ECS-like barrier to mixing along the polar vortex edge. Further theoretical advancement is needed to explain the apparent success of nonrigorous methods, such as the FSLE approach, so as to achieve a sound kinematic understanding of chaotic mixing in the winter stratosphere and other geophysical flows. © 2002 American Institute of Physics. ͓DOI:10.1063/1.1480442͔ Transport plays an important role in the distribution of chemicals in the stratosphere "the layer of atmosphere between 12 and 55 km in altitude…. This fact is clearly illustrated by, for instance, the formation of the Antarctic ozone hole every austral winter. In the extratropical stratosphere, chemical transport proceeds in quasihorizontal layers, where air parcels practically conserve ... Text Antarc* Antarctic Unknown Antarctic Austral The Antarctic |
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English |
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The necessary and sufficient conditions for Lagrangian hyperbolicity recently derived in the literature are reviewed in the light of older concepts of effective local rotation in strain coordinates. In particular, we introduce the simple interpretation of the necessary condition as a constraint on the local angular displacement in strain coordinates. These mathematically rigorous conditions are applied to the winter stratospheric circulation of the southern hemisphere, using analyzed wind data from the European Center for Medium-Range Weather Forecasts. Our results demonstrate that the sufficient condition is too strong and the necessary condition is too weak, so that both conditions fail to identify hyperbolic lines in the stratosphere. However a phenomenological, nonrigorous, criterion based on the necessary condition reveals the hyperbolic structure of the flow. Another ͑still nonrigorous͒ alternative is the finite-size Lyapunov exponent ͑FSLE͒ which is shown to produce good candidates for hyperbolic lines. In addition, we also tested the sufficient condition for Lagrangian ellipticity and found that it is too weak to detect elliptic coherent structures ͑ECS͒ in the stratosphere, of which the polar vortex is an obvious candidate. Yet, the FSLE method reveals a clear ECS-like barrier to mixing along the polar vortex edge. Further theoretical advancement is needed to explain the apparent success of nonrigorous methods, such as the FSLE approach, so as to achieve a sound kinematic understanding of chaotic mixing in the winter stratosphere and other geophysical flows. © 2002 American Institute of Physics. ͓DOI:10.1063/1.1480442͔ Transport plays an important role in the distribution of chemicals in the stratosphere "the layer of atmosphere between 12 and 55 km in altitude…. This fact is clearly illustrated by, for instance, the formation of the Antarctic ozone hole every austral winter. In the extratropical stratosphere, chemical transport proceeds in quasihorizontal layers, where air parcels practically conserve ... |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Tieh-Yong Koh Bernard Legras |
spellingShingle |
Tieh-Yong Koh Bernard Legras Hyperbolic lines and the stratospheric polar vortex |
author_facet |
Tieh-Yong Koh Bernard Legras |
author_sort |
Tieh-Yong Koh |
title |
Hyperbolic lines and the stratospheric polar vortex |
title_short |
Hyperbolic lines and the stratospheric polar vortex |
title_full |
Hyperbolic lines and the stratospheric polar vortex |
title_fullStr |
Hyperbolic lines and the stratospheric polar vortex |
title_full_unstemmed |
Hyperbolic lines and the stratospheric polar vortex |
title_sort |
hyperbolic lines and the stratospheric polar vortex |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1082.1377 http://www.lmd.ens.fr/legras/publis/chaos2002.pdf |
geographic |
Antarctic Austral The Antarctic |
geographic_facet |
Antarctic Austral The Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
http://www.lmd.ens.fr/legras/publis/chaos2002.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1082.1377 http://www.lmd.ens.fr/legras/publis/chaos2002.pdf |
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