An unified approach to meteorological modelling based on multiple-scales asymptotics

In 2003, the author suggested a mathematical framework for the derivation of reduced meteorological models at a Mathematics conference (5th ICIAM, Sydney, Australia), (Klein, 2004). The framework consists of (i) non-dimensionalization of the 3-D compressible flow equations on the rotating sphere, (i...

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Main Author: R. Klein
Format: Article
Language:English
Published: Copernicus Publications 2008-03-01
Series:Advances in Geosciences
Online Access:http://www.adv-geosci.net/15/23/2008/adgeo-15-23-2008.pdf
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spelling doaj-9c83abd1430544a0b43b44e7d8b7f6082020-11-25T00:09:30ZengCopernicus PublicationsAdvances in Geosciences1680-73401680-73592008-03-01152333An unified approach to meteorological modelling based on multiple-scales asymptoticsR. KleinIn 2003, the author suggested a mathematical framework for the derivation of reduced meteorological models at a Mathematics conference (5th ICIAM, Sydney, Australia), (Klein, 2004). The framework consists of (i) non-dimensionalization of the 3-D compressible flow equations on the rotating sphere, (ii) identification of universal non-dimensional parameters, (iii) distinguished limits between these and additional problem-specific parameters, and (iv) multiple scales expansions in the remaining small parameter ε. This parameter may be interpreted as the cubic root of the centripetal acceleration due to the Earth's rotation divided by the acceleration of gravity, see also Keller (1951), Eq. (10). For the mojority of reduced models of theoretical meteorology that we have come across, the approach allowed us to generate systematic derivations starting directly from the 3-D compressible flow equations on the rotating sphere. The framework's potential fully shows in multiscale interaction studies such as Klein (2006), in which we incorporated bulk microphysics closures for moist processes and derived scale interaction models for deep convection. Currently, we study the structure, evolution, and motion of Hurricane strength H1/H2 vortices (Mikusky, 2007), large-scale stratocumulus cloud decks, and planetary-synoptic scale interaction models which should be relevant for Earth System Models of Intermediate Complexity (EMICs). Here we summarize the general framework and use the example of quasi-geostrophic theory to demonstrate its application. http://www.adv-geosci.net/15/23/2008/adgeo-15-23-2008.pdf
collection DOAJ
language English
format Article
sources DOAJ
author R. Klein
spellingShingle R. Klein
An unified approach to meteorological modelling based on multiple-scales asymptotics
Advances in Geosciences
author_facet R. Klein
author_sort R. Klein
title An unified approach to meteorological modelling based on multiple-scales asymptotics
title_short An unified approach to meteorological modelling based on multiple-scales asymptotics
title_full An unified approach to meteorological modelling based on multiple-scales asymptotics
title_fullStr An unified approach to meteorological modelling based on multiple-scales asymptotics
title_full_unstemmed An unified approach to meteorological modelling based on multiple-scales asymptotics
title_sort unified approach to meteorological modelling based on multiple-scales asymptotics
publisher Copernicus Publications
series Advances in Geosciences
issn 1680-7340
1680-7359
publishDate 2008-03-01
description In 2003, the author suggested a mathematical framework for the derivation of reduced meteorological models at a Mathematics conference (5th ICIAM, Sydney, Australia), (Klein, 2004). The framework consists of (i) non-dimensionalization of the 3-D compressible flow equations on the rotating sphere, (ii) identification of universal non-dimensional parameters, (iii) distinguished limits between these and additional problem-specific parameters, and (iv) multiple scales expansions in the remaining small parameter ε. This parameter may be interpreted as the cubic root of the centripetal acceleration due to the Earth's rotation divided by the acceleration of gravity, see also Keller (1951), Eq. (10). For the mojority of reduced models of theoretical meteorology that we have come across, the approach allowed us to generate systematic derivations starting directly from the 3-D compressible flow equations on the rotating sphere. The framework's potential fully shows in multiscale interaction studies such as Klein (2006), in which we incorporated bulk microphysics closures for moist processes and derived scale interaction models for deep convection. Currently, we study the structure, evolution, and motion of Hurricane strength H1/H2 vortices (Mikusky, 2007), large-scale stratocumulus cloud decks, and planetary-synoptic scale interaction models which should be relevant for Earth System Models of Intermediate Complexity (EMICs). Here we summarize the general framework and use the example of quasi-geostrophic theory to demonstrate its application.
url http://www.adv-geosci.net/15/23/2008/adgeo-15-23-2008.pdf
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