Etudes et évaluation de processus océaniques par des hiérarchies ...
Etudes et évaluation de processus océaniques par des hiérarchies ... Etudes et évaluation de processus océaniques par des hiérarchies ...
60 CHAPITRE 4. ETUDES DE PROCESSUS OCÉANOGRAPHIQUES Journal of Marine Research, 58, 571–583, 2000 The parameterization of baroclinic instability in a simple model by A. Wirth 1 tel-00545911, version 1 - 13 Dec 2010 ABSTRACT Baroclinic instability of zonally forced ow in a two mode quasi-geostrophic numerical model with periodic boundary conditions is considered. Only the largest scale of the baroclinic mode is forced and the scale dependence of a diffusive parameterization of baroclinic layer thickness is determined. It is shown that the effect of baroclinic instability is a decreasing function of scale with an exponent of about half of that corresponding to the commonly used Laplace operator. We furthermore show that there is no linear relation between the time averaged amplitude of the large scale streamfunction(or quasi-geostrophicpotential vorticity) and the bolus velocity. 1. Introduction One of the major challenges in ocean modeling is the parameterization of small-scale processes not explicitly resolved in the models themselves. Many attempts have been made in this direction. The difficulty arises from the nonlinear interaction of processes on a wide range of length and time scales. Recently, interest has focused on the parameterization of a specic process, that is baroclinic instability. This process, of paramount importance in atmosphere and ocean dynamics, dominantly occurs at a small range of length and time scales. The typical length scale for the ocean is of a few times the baroclinic Rossby radius of deformation (
4.2. THE PARAMETRIZATION OF BAROCLINIC INSTABILITY IN A SIMPLE MODEL61 572 Journal of Marine Research [58, 4 tel-00545911, version 1 - 13 Dec 2010 (ii) that the dimension of the chaotic attractor of the full problem is smaller than the number of degrees of freedom of our numerical model. Both conditions are unlikely to be satised. The parameterization should, however, approach the effects of the parameterized scales in a statistical sense. A new way of parameterizing baroclinic instability was proposed by Gent and McWilliams (1990), based on diffusion of isopycnal thickness. Another, but not new, feature of the same parameterization is the down-gradient diffusion along isopycnals (see e.g. Redi, 1982). An interesting feature of this parameterization is that it can be interpreted as a quasi-adiabatic advection as explained in Gent et al. (1995). We like to refer the reader to this paper for a detailed discussion on the parameterization proposed by Gent and McWilliams. There are different ways of analyzing such parameterization.A pragmatic approach is to implement such parameterization in a large-scale ocean model (Danabasoglu and McWilliams, 1995) and evaluate its performance. Another way is to verify the foundations of the theory in numerical experiments (Treguier, 1999). The approach adapted here as in a variety of other experiments (see e.g. Killworth, 2000 and references therein) is to estimate the inuence of the small scales on the larger ones in a ne resolution model, that is, a model resolving the Rossby radius of deformation. We like to emphasize here that for resolving a length scale l 0 it is not enough to have the grid-size d 0 of the order or slightly smaller than l 0 . It is rather necessary that the length scale l 0 is in the inertial range of the nonlineardynamics (see e.g. Frisch, 1996). This usually means that the grid size d 0 has to be chosen at least an order of magnitude smaller than the length scale l 0 . It is indeed true that the dynamics on scales only a few times greater than the grid scale is dominated by linear dissipation being very different to the dynamics in the inertial range, which is dominated by nonlinear advection. The recent awareness of this problem in the ocean modeling community is apparent by the fact that models previously referred to as ‘‘eddy resolving’’ are now referred to as ‘‘eddy permitting.’’ The second point we like to dwell on is statistical signicance. Our numerical results (see Section 4) show that even for the estimation of mean values and variances, that is the lowest order moments, averaging times of about a hundred years are necessary. When such long times are necessary for a parameterized quantity to relax to their mean value the results using such parameterization have to be handled with care. An immediate consequence is that parameterized models can only be interpreted in an ensemble sense. The points mentioned in the previous two paragraphs put severe constraints on the feasibility of analyzing such parameterization. The experiment has thus to be set up very carefully, containing only the absolutely necessary ingredients. We thus consider the problem of ‘‘parameterizing baroclinic instability’’ in its numerically most feasible way. That is, we used a quasi-geostrophic two-mode model, which is periodic, both in the latitudinal and longitudinal direction. This is a simple model to test a parameterization of baroclinic instability. Another important choice is the implementation of periodic boundary conditions. In
- Page 15 and 16: 2.3. HIÉRARCHIE DE TYPES DE MODÈL
- Page 17 and 18: 2.5. MA RECHERCHE DANS LE CONTEXTE
- Page 19 and 20: 2.5. MA RECHERCHE DANS LE CONTEXTE
- Page 21 and 22: Chapitre 3 Dynamique océanique et
- Page 23 and 24: 3.1. LA CIRCULATION OCÉANIQUE À G
- Page 25 and 26: 3.1. LA CIRCULATION OCÉANIQUE À G
- Page 27 and 28: 3.2. PROCESSUS SUBMÉSO ECHELLES ET
- Page 29 and 30: 3.4. RETOUR À LA GRANDE ECHELLE PA
- Page 31 and 32: 3.5. MA RECHERCHE DANS LE CONTEXTE
- Page 33 and 34: 3.5. MA RECHERCHE DANS LE CONTEXTE
- Page 35 and 36: Bibliographie tel-00545911, version
- Page 37 and 38: Deuxième partie tel-00545911, vers
- Page 39 and 40: 33 Curriculum Vitae du Dr. Achim WI
- Page 41 and 42: 35 tel-00545911, version 1 - 13 Dec
- Page 43 and 44: Colloque bilan LEFE, Plouzané, Mai
- Page 45 and 46: Troisième partie tel-00545911, ver
- Page 47 and 48: Chapitre 4 Etudes de Processus Océ
- Page 49 and 50: 4.1. VARIABILITY OF THE GREAT WHIRL
- Page 51 and 52: 4.1. VARIABILITY OF THE GREAT WHIRL
- Page 53 and 54: 4.1. VARIABILITY OF THE GREAT WHIRL
- Page 55 and 56: 4.1. VARIABILITY OF THE GREAT WHIRL
- Page 57 and 58: 4.1. VARIABILITY OF THE GREAT WHIRL
- Page 59 and 60: 4.1. VARIABILITY OF THE GREAT WHIRL
- Page 61 and 62: 4.1. VARIABILITY OF THE GREAT WHIRL
- Page 63 and 64: 4.1. VARIABILITY OF THE GREAT WHIRL
- Page 65: 4.2. THE PARAMETRIZATION OF BAROCLI
- Page 69 and 70: 4.2. THE PARAMETRIZATION OF BAROCLI
- Page 71 and 72: 4.2. THE PARAMETRIZATION OF BAROCLI
- Page 73 and 74: 4.2. THE PARAMETRIZATION OF BAROCLI
- Page 75 and 76: 4.2. THE PARAMETRIZATION OF BAROCLI
- Page 77 and 78: 4.2. THE PARAMETRIZATION OF BAROCLI
- Page 79 and 80: 4.3. A NON-HYDROSTATIC FLAT-BOTTOM
- Page 81 and 82: 4.3. A NON-HYDROSTATIC FLAT-BOTTOM
- Page 83 and 84: 4.3. A NON-HYDROSTATIC FLAT-BOTTOM
- Page 85 and 86: 4.3. A NON-HYDROSTATIC FLAT-BOTTOM
- Page 87 and 88: 4.3. A NON-HYDROSTATIC FLAT-BOTTOM
- Page 89 and 90: 4.3. A NON-HYDROSTATIC FLAT-BOTTOM
- Page 91 and 92: 4.3. A NON-HYDROSTATIC FLAT-BOTTOM
- Page 93 and 94: 4.3. A NON-HYDROSTATIC FLAT-BOTTOM
- Page 95 and 96: 4.3. A NON-HYDROSTATIC FLAT-BOTTOM
- Page 97 and 98: 4.4. TILTED CONVECTIVE PLUMES IN NU
- Page 99 and 100: 4.4. TILTED CONVECTIVE PLUMES IN NU
- Page 101 and 102: 4.4. TILTED CONVECTIVE PLUMES IN NU
- Page 103 and 104: 4.4. TILTED CONVECTIVE PLUMES IN NU
- Page 105 and 106: 4.4. TILTED CONVECTIVE PLUMES IN NU
- Page 107 and 108: 4.4. TILTED CONVECTIVE PLUMES IN NU
- Page 109 and 110: 4.5. MEAN CIRCULATION AND STRUCTURE
- Page 111 and 112: 4.5. MEAN CIRCULATION AND STRUCTURE
- Page 113 and 114: 4.5. MEAN CIRCULATION AND STRUCTURE
- Page 115 and 116: 4.5. MEAN CIRCULATION AND STRUCTURE
4.2. THE PARAMETRIZATION OF BAROCLINIC INSTABILITY IN A SIMPLE MODEL61<br />
572 Journal of Marine Research [58, 4<br />
tel-00545911, version 1 - 13 Dec 2010<br />
(ii) that the dimension of the chaotic attractor of the full problem is smaller than the number<br />
of <strong>de</strong>grees of freedom of our numerical mo<strong>de</strong>l. Both conditions are unlikely to be satised.<br />
The <strong>par</strong>am<strong>et</strong>erization should, however, approach the effects of the <strong>par</strong>am<strong>et</strong>erized scales in<br />
a statistical sense.<br />
A new way of <strong>par</strong>am<strong>et</strong>erizing baroclinic instability was proposed by Gent and McWilliams<br />
(1990), based on diffusion of isopycnal thickness. Another, but not new, feature of<br />
the same <strong>par</strong>am<strong>et</strong>erization is the down-gradient diffusion along isopycnals (see e.g. Redi,<br />
1982). An interesting feature of this <strong>par</strong>am<strong>et</strong>erization is that it can be interpr<strong>et</strong>ed as a<br />
quasi-adiabatic advection as explained in Gent <strong>et</strong> al. (1995). We like to refer the rea<strong>de</strong>r to<br />
this paper for a d<strong>et</strong>ailed discussion on the <strong>par</strong>am<strong>et</strong>erization proposed by Gent and<br />
McWilliams.<br />
There are different ways of analyzing such <strong>par</strong>am<strong>et</strong>erization.A pragmatic approach is to<br />
implement such <strong>par</strong>am<strong>et</strong>erization in a large-scale ocean mo<strong>de</strong>l (Danabasoglu and McWilliams,<br />
1995) and evaluate its performance. Another way is to verify the foundations of the<br />
theory in numerical experiments (Treguier, 1999).<br />
The approach adapted here as in a vari<strong>et</strong>y of other experiments (see e.g. Killworth, 2000<br />
and references therein) is to estimate the inuence of the small scales on the larger ones in a<br />
ne resolution mo<strong>de</strong>l, that is, a mo<strong>de</strong>l resolving the Rossby radius of <strong>de</strong>formation. We like<br />
to emphasize here that for resolving a length scale l 0 it is not enough to have the grid-size d 0<br />
of the or<strong>de</strong>r or slightly smaller than l 0 . It is rather necessary that the length scale l 0 is in the<br />
inertial range of the nonlineardynamics (see e.g. Frisch, 1996). This usually means that the<br />
grid size d 0 has to be chosen at least an or<strong>de</strong>r of magnitu<strong>de</strong> smaller than the length scale l 0 .<br />
It is in<strong>de</strong>ed true that the dynamics on scales only a few times greater than the grid scale is<br />
dominated by linear dissipation being very different to the dynamics in the inertial range,<br />
which is dominated by nonlinear advection. The recent awareness of this problem in the<br />
ocean mo<strong>de</strong>ling community is ap<strong>par</strong>ent by the fact that mo<strong>de</strong>ls previously referred to as<br />
‘‘eddy resolving’’ are now referred to as ‘‘eddy permitting.’’<br />
The second point we like to dwell on is statistical signicance. Our numerical results<br />
(see Section 4) show that even for the estimation of mean values and variances, that is the<br />
lowest or<strong>de</strong>r moments, averaging times of about a hundred years are necessary. When such<br />
long times are necessary for a <strong>par</strong>am<strong>et</strong>erized quantity to relax to their mean value the<br />
results using such <strong>par</strong>am<strong>et</strong>erization have to be handled with care. An immediate consequence<br />
is that <strong>par</strong>am<strong>et</strong>erized mo<strong>de</strong>ls can only be interpr<strong>et</strong>ed in an ensemble sense.<br />
The points mentioned in the previous two <strong>par</strong>agraphs put severe constraints on the<br />
feasibility of analyzing such <strong>par</strong>am<strong>et</strong>erization. The experiment has thus to be s<strong>et</strong> up very<br />
carefully, containing only the absolutely necessary ingredients. We thus consi<strong>de</strong>r the<br />
problem of ‘‘<strong>par</strong>am<strong>et</strong>erizing baroclinic instability’’ in its numerically most feasible way.<br />
That is, we used a quasi-geostrophic two-mo<strong>de</strong> mo<strong>de</strong>l, which is periodic, both in the<br />
latitudinal and longitudinal direction. This is a simple mo<strong>de</strong>l to test a <strong>par</strong>am<strong>et</strong>erization of<br />
baroclinic instability.<br />
Another important choice is the implementation of periodic boundary conditions. In