On the mix-down times of dynamically active potential vorticity filaments

A simple model is used to study the evolution of potential vorticity filaments, viewed in cross-section, subject to steady shear and deformation flows representative of the large-scale atmospheric circulation. It is found that the balanced, ageostrophic circulation induced by the anomalous potential...

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Main Authors: Polvani, Lorenzo M., Esler Jr, Kenneth P, Plumb, R. Alan
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:en_US
Published: American Geophysical Union (AGU) 2017
Online Access:http://hdl.handle.net/1721.1/108606
https://orcid.org/0000-0002-6716-1576
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author Polvani, Lorenzo M.
Esler Jr, Kenneth P
Plumb, R. Alan
author2 Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
author_facet Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Polvani, Lorenzo M.
Esler Jr, Kenneth P
Plumb, R. Alan
author_sort Polvani, Lorenzo M.
collection MIT
description A simple model is used to study the evolution of potential vorticity filaments, viewed in cross-section, subject to steady shear and deformation flows representative of the large-scale atmospheric circulation. It is found that the balanced, ageostrophic circulation induced by the anomalous potential vorticity can cause the evolution of a dynamically active filament to differ substantially from that of a dynamically passive filament in a similar background flow. It is suggested that estimates of the mix-down time of material contained in atmospheric filaments need to be corrected to allow for this effect.
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spelling mit-1721.1/1086062024-05-15T03:19:32Z On the mix-down times of dynamically active potential vorticity filaments Polvani, Lorenzo M. Esler Jr, Kenneth P Plumb, R. Alan Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Massachusetts Institute of Technology. Program in Atmospheres, Oceans, and Climate Esler Jr, Kenneth P Plumb, Raymond Alan A simple model is used to study the evolution of potential vorticity filaments, viewed in cross-section, subject to steady shear and deformation flows representative of the large-scale atmospheric circulation. It is found that the balanced, ageostrophic circulation induced by the anomalous potential vorticity can cause the evolution of a dynamically active filament to differ substantially from that of a dynamically passive filament in a similar background flow. It is suggested that estimates of the mix-down time of material contained in atmospheric filaments need to be corrected to allow for this effect. 2017-05-02T18:24:14Z 2017-05-02T18:24:14Z 1999-10 1999-06 Article http://purl.org/eprint/type/JournalArticle 0094-8276 http://hdl.handle.net/1721.1/108606 Esler, J. Gavin, Lorenzo M. Polvani, and R. Alan Plumb. “On the Mix-down Times of Dynamically Active Potential Vorticity Filaments.” Geophysical Research Letters 26, no. 19 (October 1, 1999): 2953–2956. https://orcid.org/0000-0002-6716-1576 en_US http://dx.doi.org/10.1029/1999GL010875 Geophysical Research Letters Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Geophysical Union (AGU) Other univ. web domain
spellingShingle Polvani, Lorenzo M.
Esler Jr, Kenneth P
Plumb, R. Alan
On the mix-down times of dynamically active potential vorticity filaments
title On the mix-down times of dynamically active potential vorticity filaments
title_full On the mix-down times of dynamically active potential vorticity filaments
title_fullStr On the mix-down times of dynamically active potential vorticity filaments
title_full_unstemmed On the mix-down times of dynamically active potential vorticity filaments
title_short On the mix-down times of dynamically active potential vorticity filaments
title_sort on the mix down times of dynamically active potential vorticity filaments
url http://hdl.handle.net/1721.1/108606
https://orcid.org/0000-0002-6716-1576
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