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dimitri |
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\section{Introduction} |
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\label{sec:intro} |
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The availability of an adjoint model as a powerful research tool |
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complementary to an ocean model was a major design requirement early |
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on in the development of the MIT general circulation model (MITgcm) |
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[Marshall et al. 1997a, Marotzke et al. 1999, Adcroft et al. 2002]. It |
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was recognized that the adjoint model permitted computing the |
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gradients of various scalar-valued model diagnostics, norms or, |
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generally, objective functions with respect to external or independent |
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parameters very efficiently. The information associtated with these |
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gradients is useful in at least two major contexts. First, for state |
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estimation problems, the objective function is the sum of squared |
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differences between observations and model results weighted by the |
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inverse error covariances. The gradient of such an objective function |
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can be used to reduce this measure of model-data misfit to find the |
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optimal model solution in a least-squares sense. Second, the |
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objective function can be a key oceanographic quantity such as |
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meridional heat or volume transport, ocean heat content or mean |
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surface temperature index. In this case the gradient provides a |
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complete set of sensitivities of this quantity to all independent |
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variables simultaneously. These sensitivities can be used to address |
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the cause of, say, changing net transports accurately. |
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References to existing sea-ice adjoint models, explaining that they are either |
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for simplified configurations, for ice-only studies, or for short-duration |
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studies to motivate the present work. |
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Traditionally, probably for historical reasons and the ease of |
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treating the Coriolis term, most standard sea-ice models are |
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discretized on Arakawa-B-grids \citep[e.g.,][]{hibler79, harder99, |
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kreyscher00, zhang98, hunke97}. From the perspective of coupling a |
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sea ice-model to a C-grid ocean model, the exchange of fluxes of heat |
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and fresh-water pose no difficulty for a B-grid sea-ice model |
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\citep[e.g.,][]{timmermann02a}. However, surface stress is defined at |
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velocities points and thus needs to be interpolated between a B-grid |
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sea-ice model and a C-grid ocean model. Smoothing implicitly |
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associated with this interpolation may mask grid scale noise and may |
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contribute to stabilizing the solution. On the other hand, by |
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smoothing the stress signals are damped which could lead to reduced |
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variability of the system. By choosing a C-grid for the sea-ice model, |
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we circumvent this difficulty altogether and render the stress |
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coupling as consistent as the buoyancy coupling. |
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A further advantage of the C-grid formulation is apparent in narrow |
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straits. In the limit of only one grid cell between coasts there is no |
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flux allowed for a B-grid (with no-slip lateral boundary counditions), |
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and models have used topographies artificially widened straits to |
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avoid this problem \citep{holloway07}. The C-grid formulation on the |
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other hand allows a flux of sea-ice through narrow passages if |
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free-slip along the boundaries is allowed. We demonstrate this effect |
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in the Candian archipelago. |
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Talk about problems that make the sea-ice-ocean code very sensitive and |
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changes in the code that reduce these sensitivities. |
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This paper describes the MITgcm sea ice |
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model; it presents example Arctic and Antarctic results from a realistic, |
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eddy-permitting, global ocean and sea-ice configuration; it compares B-grid |
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and C-grid dynamic solvers in a regional Arctic configuration; and it presents |
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example results from coupled ocean and sea-ice adjoint-model integrations. |