Overview

An energy loan sea ice model was developed to manage the energetics of water phase changes in a consistent yet simple manner. The model, which has much in common with the one developed by Semtner (1976, Appendix) focuses on two aspects of the influence of sea ice: (1) the stabilization of ocean temp...

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Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2000
Subjects:
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.689.4820
http://hycom.org/attachments/067_ice.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.689.4820 2023-05-15T18:18:17+02:00 Overview The Pennsylvania State University CiteSeerX Archives 2000 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.689.4820 http://hycom.org/attachments/067_ice.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.689.4820 http://hycom.org/attachments/067_ice.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://hycom.org/attachments/067_ice.pdf text 2000 ftciteseerx 2016-01-08T18:17:12Z An energy loan sea ice model was developed to manage the energetics of water phase changes in a consistent yet simple manner. The model, which has much in common with the one developed by Semtner (1976, Appendix) focuses on two aspects of the influence of sea ice: (1) the stabilization of ocean temperature near the freezing point through ice formation and melting, and (2) the impact of the ice surface on ocean-atmosphere energy fluxes. Concerning the stabilization of ocean temperature, the energy loan concept of the ice model ensures that the oceanic mixed layer temperature does not drop below the freezing point (-1.8 o C) when the surface heat flux removes heat from the ocean. At each model grid point, the ocean borrows energy from an “energy bank ” to stabilize temperature at the freezing point. The energy required to maintain this temperature comes from freezing an appropriate amount of seawater. Conversely, if the surface heat flux adds heat to the ocean, the energy loan must be repaid before the ocean temperature in a grid box is permitted to rise above freezing. The influence of ice on surface fluxes is large, both by virtue of its high albedo compared to water and because an ice surface can be much colder than open water. In the present ice model, surface temperature is calculated based on the assumption that the system is energetically in a steady state; i.e., the heat flux through the ice matches the atmospheric heat flux. Specifics To illustrate this approach, the atmospheric heat flux is written as ()air i aF a T T =-, and the heat flux through the ice as ()ice w iF a T T =-, where iT, aT, and wT represents ice, air, and water temperature while a and b are proportionality factors. Given aT, wT, and a first guess of iT (the unknown in this problem), iT is modified by an amount iTD to minimize the difference between airF and iceF: ( ) (),i i a w i ia T T T b T T T+ D- =-- D which yields.a wi i aT bT Text Sea ice Unknown
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description An energy loan sea ice model was developed to manage the energetics of water phase changes in a consistent yet simple manner. The model, which has much in common with the one developed by Semtner (1976, Appendix) focuses on two aspects of the influence of sea ice: (1) the stabilization of ocean temperature near the freezing point through ice formation and melting, and (2) the impact of the ice surface on ocean-atmosphere energy fluxes. Concerning the stabilization of ocean temperature, the energy loan concept of the ice model ensures that the oceanic mixed layer temperature does not drop below the freezing point (-1.8 o C) when the surface heat flux removes heat from the ocean. At each model grid point, the ocean borrows energy from an “energy bank ” to stabilize temperature at the freezing point. The energy required to maintain this temperature comes from freezing an appropriate amount of seawater. Conversely, if the surface heat flux adds heat to the ocean, the energy loan must be repaid before the ocean temperature in a grid box is permitted to rise above freezing. The influence of ice on surface fluxes is large, both by virtue of its high albedo compared to water and because an ice surface can be much colder than open water. In the present ice model, surface temperature is calculated based on the assumption that the system is energetically in a steady state; i.e., the heat flux through the ice matches the atmospheric heat flux. Specifics To illustrate this approach, the atmospheric heat flux is written as ()air i aF a T T =-, and the heat flux through the ice as ()ice w iF a T T =-, where iT, aT, and wT represents ice, air, and water temperature while a and b are proportionality factors. Given aT, wT, and a first guess of iT (the unknown in this problem), iT is modified by an amount iTD to minimize the difference between airF and iceF: ( ) (),i i a w i ia T T T b T T T+ D- =-- D which yields.a wi i aT bT
author2 The Pennsylvania State University CiteSeerX Archives
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title Overview
spellingShingle Overview
title_short Overview
title_full Overview
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title_full_unstemmed Overview
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publishDate 2000
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.689.4820
http://hycom.org/attachments/067_ice.pdf
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