Isentropic zonal average formalism and the near-surface circulation

Hoskins (1991) proposed dividing the atmosphere into 3 regions: Overworld, Middleworld and Underworld, using potential temperature θ and potential vorticity (PV) as reference (Fig. 1). In the Underworld (θ < 300 K), isentropes intercept the Earth’s surface and a direct isentropic zonal aver...

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Main Authors: Koh, Tieh Yong, Plumb, Alan R.
Other Authors: Proceedings of the Conference on Atmospheric and Oceanic Fluid Dynamics, American Meteorological Society (14th : 2003)
Format: Conference Paper
Language:English
Published: 2014
Subjects:
Online Access:https://hdl.handle.net/10356/79719
http://hdl.handle.net/10220/20355
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author Koh, Tieh Yong
Plumb, Alan R.
author2 Proceedings of the Conference on Atmospheric and Oceanic Fluid Dynamics, American Meteorological Society (14th : 2003)
author_facet Proceedings of the Conference on Atmospheric and Oceanic Fluid Dynamics, American Meteorological Society (14th : 2003)
Koh, Tieh Yong
Plumb, Alan R.
author_sort Koh, Tieh Yong
collection NTU
description Hoskins (1991) proposed dividing the atmosphere into 3 regions: Overworld, Middleworld and Underworld, using potential temperature θ and potential vorticity (PV) as reference (Fig. 1). In the Underworld (θ < 300 K), isentropes intercept the Earth’s surface and a direct isentropic zonal average circulation exists in the mid-latitudes. Held and Schneider (1999) suggested that this circulation may be understood as follows: the equator-pole temperature gradient determines the near-surface eddy heat flux via an eddydiffusion mechanism. The poleward eddy heat flux in turn drives an equatorward mean flow next to the surface whose horizontal convergence in the subtropics forces the mean quasi-isentropic ascent of air into the troposphere. Radiative cooling causes air to sink back to the surface, thus closing the circulation.
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spelling ntu-10356/797192020-09-26T21:24:19Z Isentropic zonal average formalism and the near-surface circulation Koh, Tieh Yong Plumb, Alan R. Proceedings of the Conference on Atmospheric and Oceanic Fluid Dynamics, American Meteorological Society (14th : 2003) DRNTU::Science::Astronomy Hoskins (1991) proposed dividing the atmosphere into 3 regions: Overworld, Middleworld and Underworld, using potential temperature θ and potential vorticity (PV) as reference (Fig. 1). In the Underworld (θ < 300 K), isentropes intercept the Earth’s surface and a direct isentropic zonal average circulation exists in the mid-latitudes. Held and Schneider (1999) suggested that this circulation may be understood as follows: the equator-pole temperature gradient determines the near-surface eddy heat flux via an eddydiffusion mechanism. The poleward eddy heat flux in turn drives an equatorward mean flow next to the surface whose horizontal convergence in the subtropics forces the mean quasi-isentropic ascent of air into the troposphere. Radiative cooling causes air to sink back to the surface, thus closing the circulation. Accepted version 2014-08-21T01:36:26Z 2019-12-06T13:32:42Z 2014-08-21T01:36:26Z 2019-12-06T13:32:42Z 2003 2003 Conference Paper Koh, T. Y. & Plumb, R. A. (2003). Isentropic zonal average formalism and the near-surface circulation. Proceedings of the 14th Conference on Atmospheric and Oceanic Fluid Dynamics, American Meteorological Society, 9-13 June 2003. https://hdl.handle.net/10356/79719 http://hdl.handle.net/10220/20355 en © 2003 The Author(s). This is the author created version of a work that has been peer reviewed and accepted for publication by Proceedings of the 14th Conference on Atmospheric and Oceanic Fluid Dynamics, American Meteorological Society, 9-13 June 2003. It incorporates referee’s comments but changes resulting from the publishing process, such as copyediting, structural formatting, may not be reflected in this document. application/pdf
spellingShingle DRNTU::Science::Astronomy
Koh, Tieh Yong
Plumb, Alan R.
Isentropic zonal average formalism and the near-surface circulation
title Isentropic zonal average formalism and the near-surface circulation
title_full Isentropic zonal average formalism and the near-surface circulation
title_fullStr Isentropic zonal average formalism and the near-surface circulation
title_full_unstemmed Isentropic zonal average formalism and the near-surface circulation
title_short Isentropic zonal average formalism and the near-surface circulation
title_sort isentropic zonal average formalism and the near surface circulation
topic DRNTU::Science::Astronomy
url https://hdl.handle.net/10356/79719
http://hdl.handle.net/10220/20355
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