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1 \section{Introduction}
2 \label{sec:intro}
3
4 In recent years, oceanographic state estimation has matured to the
5 extent that estimates of the evolving circulation of the ocean constrained by
6 in-situ and remotely sensed global observations are now routinely available
7 and being applied to myriad scientific problems \citep{wun07}. Ocean state
8 estimation is the process of fitting an ocean General Circulation Model (GCM)
9 to a multitude of observations. As formulated by the consortium for Estimating
10 the Circulation and Climate of the Ocean (ECCO), an automatic differentiation
11 tool is used to calculate the so-called adjoint code of a GCM. The method of
12 Lagrange multipliers is then used to render the problem one of unconstrained
13 least-squares minimization. Although much has been achieved, the existing
14 ECCO estimates lack interactive sea ice. This limits the ability to
15 utilize satellite data constraints over sea-ice covered regions. This also
16 limits the usefulness of the derived ocean state estimates for describing and
17 studying polar-subpolar interactions. This paper is a first step towards
18 adding sea-ice capability to the ECCO estimates. That is, we describe a
19 dynamic and thermodynamic sea ice model that has been coupled to the
20 Massachusetts Institute of Technology general circulation model
21 \citep[MITgcm][]{mar97a} and that has been modified to permit efficient and
22 accurate automatic differentiation.
23
24 The availability of an adjoint model as a powerful research tool
25 complementary to an ocean model was a major design requirement early
26 on in the development of the MITgcm \citep{marotzke99}. It
27 was recognized that the adjoint model permitted computing the
28 gradients of various scalar-valued model diagnostics, norms or,
29 generally, objective functions with respect to external or independent
30 parameters very efficiently. The information associtated with these
31 gradients is useful in at least two major contexts. First, for state
32 estimation problems, the objective function is the sum of squared
33 differences between observations and model results weighted by the
34 inverse error covariances. The gradient of such an objective function
35 can be used to reduce this measure of model-data misfit to find the
36 optimal model solution in a least-squares sense. Second, the
37 objective function can be a key oceanographic quantity such as
38 meridional heat or volume transport, ocean heat content or mean
39 surface temperature index. In this case the gradient provides a
40 complete set of sensitivities of this quantity to all independent
41 variables simultaneously. These sensitivities can be used to address
42 the cause of, say, changing net transports accurately.
43
44 References to existing sea-ice adjoint models, explaining that they are either
45 for simplified configurations, for ice-only studies, or for short-duration
46 studies to motivate the present work.
47
48 Traditionally, probably for historical reasons and the ease of
49 treating the Coriolis term, most standard sea-ice models are
50 discretized on Arakawa-B-grids \citep[e.g.,][]{hibler79, harder99,
51 kreyscher00, zhang98, hunke97}, although there are sea ice models
52 diretized on a C-grid \citep[e.g.,][]{ip91, tremblay97,
53 lemieux09}. %
54 \ml{[there is also MI-IM, but I only found this as a reference:
55 \url{http://retro.met.no/english/r_and_d_activities/method/num_mod/MI-IM-Documentation.pdf}]}
56 From the perspective of coupling a sea ice-model to a C-grid ocean
57 model, the exchange of fluxes of heat and fresh-water pose no
58 difficulty for a B-grid sea-ice model \citep[e.g.,][]{timmermann02a}.
59 However, surface stress is defined at velocities points and thus needs
60 to be interpolated between a B-grid sea-ice model and a C-grid ocean
61 model. Smoothing implicitly associated with this interpolation may
62 mask grid scale noise and may contribute to stabilizing the solution.
63 On the other hand, by smoothing the stress signals are damped which
64 could lead to reduced variability of the system. By choosing a C-grid
65 for the sea-ice model, we circumvent this difficulty altogether and
66 render the stress coupling as consistent as the buoyancy coupling.
67
68 A further advantage of the C-grid formulation is apparent in narrow
69 straits. In the limit of only one grid cell between coasts there is no
70 flux allowed for a B-grid (with no-slip lateral boundary counditions),
71 and models have used topographies with artificially widened straits to
72 avoid this problem \citep{holloway07}. The C-grid formulation on the
73 other hand allows a flux of sea-ice through narrow passages if
74 free-slip along the boundaries is allowed. We demonstrate this effect
75 in the Candian archipelago.
76
77 Talk about problems that make the sea-ice-ocean code very sensitive and
78 changes in the code that reduce these sensitivities.
79
80 This paper describes the MITgcm sea ice model; it presents example
81 Arctic and Antarctic results from a realistic, eddy-permitting, global
82 ocean and sea-ice configuration; it compares B-grid and C-grid dynamic
83 solvers and investigates further aspects of sea ice modeling in a
84 regional Arctic configuration; and it presents example results from
85 coupled ocean and sea-ice adjoint-model integrations.
86
87 %%% Local Variables:
88 %%% mode: latex
89 %%% TeX-master: "ceaice"
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