Compressibility effects in the Miami isopycnic coordinate ocean model

Potential density referenced to sea level pressure $(\sigma\sb0$) has shown its usefulness as vertical coordinate in ocean models in many ways, but there are problems with $\sigma\sb0$ (potential density referenced to sea level) coordinates in the deep ocean: $\sigma\sb0(z)$ can be multivalued, lead...

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Main Author: Sun, Shan
Other Authors: Rainer Bleck - Committee Chair
Format: Article in Journal/Newspaper
Language:unknown
Published: Scholarly Repository 1997
Subjects:
Online Access:https://scholarlyrepository.miami.edu/dissertations/3462
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spelling ftunivmiamiir:oai:scholarlyrepository.miami.edu:dissertations-4461 2023-05-15T13:36:29+02:00 Compressibility effects in the Miami isopycnic coordinate ocean model Sun, Shan Rainer Bleck - Committee Chair 1997-01-01T08:00:00Z https://scholarlyrepository.miami.edu/dissertations/3462 unknown Scholarly Repository Dissertations from ProQuest Geophysics; Physical Oceanography; Engineering Marine and Ocean article 1997 ftunivmiamiir 2019-08-09T22:54:59Z Potential density referenced to sea level pressure $(\sigma\sb0$) has shown its usefulness as vertical coordinate in ocean models in many ways, but there are problems with $\sigma\sb0$ (potential density referenced to sea level) coordinates in the deep ocean: $\sigma\sb0(z)$ can be multivalued, leading to coordinate folding, and $\sigma\sb0$ surfaces can deviate from the so-called neutral surfaces, which are the surfaces along which turbulent lateral mixing takes place in a stratified medium. The reason for both of these problems is that most isopycnal models regard seawater as uniformly compressible. However, the effect of water temperature on compressibility cannot be ignored.In this study a two-pronged approach is taken to improve the model accuracy. First, since the effects of compressibility variation are proportional to the difference between the local and the reference pressure, we replace the model's traditional $\sigma\sb0$ coordinate by $\sigma\sb2$ (potential density referenced to 2000 dbar). This step eliminates many of the coordinate folding problems associated with $\sigma\sb0$ and generally reduces the difference between coordinate and neutrally buoyant surfaces. Second, we split the compressibility coefficient into a pressure- and a temperature-dependent part and, recognizing that the former is dynamically passive, retain only the effect of the latter in the governing equations. This is accomplished by introducing a new variable called "active density"--the density with the pressure-related compressibility removed. Therefore, $\sigma\sb2$ is adopted as vertical coordinate, but active density is used to express the seawater density within the layers.The above changes are applied in a near-global, 16-layer, 2$\sp\circ$ x 2$\sp\circ$cos (lat.) Miami Isopycnic Coordinate Ocean Model (MICOM). The model is driven by observed atmospheric conditions. MICOM modified in this fashion produces realistic meridional mass and associated heat fluxes in the three major ocean basins. A realistic formation rate of a few major water masses, including the North Atlantic Deep Water and the Antarctic Bottom Water, is also obtained. To summarize the various circulation features obtained by the model, a three-dimensional mass transport diagram spanning four density classes is constructed. Many features in it compare well with those revealed by observed hydrographic data. Article in Journal/Newspaper Antarc* Antarctic North Atlantic Deep Water North Atlantic University of Miami: Scholarly Repository Antarctic The Antarctic
institution Open Polar
collection University of Miami: Scholarly Repository
op_collection_id ftunivmiamiir
language unknown
topic Geophysics; Physical Oceanography; Engineering
Marine and Ocean
spellingShingle Geophysics; Physical Oceanography; Engineering
Marine and Ocean
Sun, Shan
Compressibility effects in the Miami isopycnic coordinate ocean model
topic_facet Geophysics; Physical Oceanography; Engineering
Marine and Ocean
description Potential density referenced to sea level pressure $(\sigma\sb0$) has shown its usefulness as vertical coordinate in ocean models in many ways, but there are problems with $\sigma\sb0$ (potential density referenced to sea level) coordinates in the deep ocean: $\sigma\sb0(z)$ can be multivalued, leading to coordinate folding, and $\sigma\sb0$ surfaces can deviate from the so-called neutral surfaces, which are the surfaces along which turbulent lateral mixing takes place in a stratified medium. The reason for both of these problems is that most isopycnal models regard seawater as uniformly compressible. However, the effect of water temperature on compressibility cannot be ignored.In this study a two-pronged approach is taken to improve the model accuracy. First, since the effects of compressibility variation are proportional to the difference between the local and the reference pressure, we replace the model's traditional $\sigma\sb0$ coordinate by $\sigma\sb2$ (potential density referenced to 2000 dbar). This step eliminates many of the coordinate folding problems associated with $\sigma\sb0$ and generally reduces the difference between coordinate and neutrally buoyant surfaces. Second, we split the compressibility coefficient into a pressure- and a temperature-dependent part and, recognizing that the former is dynamically passive, retain only the effect of the latter in the governing equations. This is accomplished by introducing a new variable called "active density"--the density with the pressure-related compressibility removed. Therefore, $\sigma\sb2$ is adopted as vertical coordinate, but active density is used to express the seawater density within the layers.The above changes are applied in a near-global, 16-layer, 2$\sp\circ$ x 2$\sp\circ$cos (lat.) Miami Isopycnic Coordinate Ocean Model (MICOM). The model is driven by observed atmospheric conditions. MICOM modified in this fashion produces realistic meridional mass and associated heat fluxes in the three major ocean basins. A realistic formation rate of a few major water masses, including the North Atlantic Deep Water and the Antarctic Bottom Water, is also obtained. To summarize the various circulation features obtained by the model, a three-dimensional mass transport diagram spanning four density classes is constructed. Many features in it compare well with those revealed by observed hydrographic data.
author2 Rainer Bleck - Committee Chair
format Article in Journal/Newspaper
author Sun, Shan
author_facet Sun, Shan
author_sort Sun, Shan
title Compressibility effects in the Miami isopycnic coordinate ocean model
title_short Compressibility effects in the Miami isopycnic coordinate ocean model
title_full Compressibility effects in the Miami isopycnic coordinate ocean model
title_fullStr Compressibility effects in the Miami isopycnic coordinate ocean model
title_full_unstemmed Compressibility effects in the Miami isopycnic coordinate ocean model
title_sort compressibility effects in the miami isopycnic coordinate ocean model
publisher Scholarly Repository
publishDate 1997
url https://scholarlyrepository.miami.edu/dissertations/3462
geographic Antarctic
The Antarctic
geographic_facet Antarctic
The Antarctic
genre Antarc*
Antarctic
North Atlantic Deep Water
North Atlantic
genre_facet Antarc*
Antarctic
North Atlantic Deep Water
North Atlantic
op_source Dissertations from ProQuest
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