Changeset 6440 for branches/UKMO/dev_r5518_GC3p0_package/DOC/TexFiles/Chapters/Chap_Model_Basics.tex
- Timestamp:
- 2016-04-07T16:32:24+02:00 (8 years ago)
- File:
-
- 1 edited
Legend:
- Unmodified
- Added
- Removed
-
branches/UKMO/dev_r5518_GC3p0_package/DOC/TexFiles/Chapters/Chap_Model_Basics.tex
r3294 r6440 247 247 sufficient to solve a linearized version of (\ref{Eq_PE_ssh}), which still allows 248 248 to take into account freshwater fluxes applied at the ocean surface \citep{Roullet_Madec_JGR00}. 249 Nevertheless, with the linearization, an exact conservation of heat and salt contents is lost. 249 250 250 251 The filtering of EGWs in models with a free surface is usually a matter of discretisation 251 of the temporal derivatives, using the time splitting method \citep{Killworth_al_JPO91, Zhang_Endoh_JGR92} 252 or the implicit scheme \citep{Dukowicz1994}. In \NEMO, we use a slightly different approach 253 developed by \citet{Roullet_Madec_JGR00}: the damping of EGWs is ensured by introducing an 254 additional force in the momentum equation. \eqref{Eq_PE_dyn} becomes: 255 \begin{equation} \label{Eq_PE_flt} 256 \frac{\partial {\rm {\bf U}}_h }{\partial t}= {\rm {\bf M}} 257 - g \nabla \left( \tilde{\rho} \ \eta \right) 258 - g \ T_c \nabla \left( \widetilde{\rho} \ \partial_t \eta \right) 259 \end{equation} 260 where $T_c$, is a parameter with dimensions of time which characterizes the force, 261 $\widetilde{\rho} = \rho / \rho_o$ is the dimensionless density, and $\rm {\bf M}$ 262 represents the collected contributions of the Coriolis, hydrostatic pressure gradient, 263 non-linear and viscous terms in \eqref{Eq_PE_dyn}. 264 265 The new force can be interpreted as a diffusion of vertically integrated volume flux divergence. 266 The time evolution of $D$ is thus governed by a balance of two terms, $-g$ \textbf{A} $\eta$ 267 and $g \, T_c \,$ \textbf{A} $D$, associated with a propagative regime and a diffusive regime 268 in the temporal spectrum, respectively. In the diffusive regime, the EGWs no longer propagate, 269 $i.e.$ they are stationary and damped. The diffusion regime applies to the modes shorter than 270 $T_c$. For longer ones, the diffusion term vanishes. Hence, the temporally unresolved EGWs 271 can be damped by choosing $T_c > \rdt$. \citet{Roullet_Madec_JGR00} demonstrate that 272 (\ref{Eq_PE_flt}) can be integrated with a leap frog scheme except the additional term which 273 has to be computed implicitly. This is not surprising since the use of a large time step has a 274 necessarily numerical cost. Two gains arise in comparison with the previous formulations. 275 Firstly, the damping of EGWs can be quantified through the magnitude of the additional term. 276 Secondly, the numerical scheme does not need any tuning. Numerical stability is ensured as 277 soon as $T_c > \rdt$. 278 279 When the variations of free surface elevation are small compared to the thickness of the first 280 model layer, the free surface equation (\ref{Eq_PE_ssh}) can be linearized. As emphasized 281 by \citet{Roullet_Madec_JGR00} the linearization of (\ref{Eq_PE_ssh}) has consequences on the 282 conservation of salt in the model. With the nonlinear free surface equation, the time evolution 283 of the total salt content is 284 \begin{equation} \label{Eq_PE_salt_content} 285 \frac{\partial }{\partial t}\int\limits_{D\eta } {S\;dv} 286 =\int\limits_S {S\;(-\frac{\partial \eta }{\partial t}-D+P-E)\;ds} 287 \end{equation} 288 where $S$ is the salinity, and the total salt is integrated over the whole ocean volume 289 $D_\eta$ bounded by the time-dependent free surface. The right hand side (which is an 290 integral over the free surface) vanishes when the nonlinear equation (\ref{Eq_PE_ssh}) 291 is satisfied, so that the salt is perfectly conserved. When the free surface equation is 292 linearized, \citet{Roullet_Madec_JGR00} show that the total salt content integrated in the fixed 293 volume $D$ (bounded by the surface $z=0$) is no longer conserved: 294 \begin{equation} \label{Eq_PE_salt_content_linear} 295 \frac{\partial }{\partial t}\int\limits_D {S\;dv} 296 = - \int\limits_S {S\;\frac{\partial \eta }{\partial t}ds} 297 \end{equation} 298 299 The right hand side of (\ref{Eq_PE_salt_content_linear}) is small in equilibrium solutions 300 \citep{Roullet_Madec_JGR00}. It can be significant when the freshwater forcing is not balanced and 301 the globally averaged free surface is drifting. An increase in sea surface height \textit{$\eta $} 302 results in a decrease of the salinity in the fixed volume $D$. Even in that case though, 303 the total salt integrated in the variable volume $D_{\eta}$ varies much less, since 304 (\ref{Eq_PE_salt_content_linear}) can be rewritten as 305 \begin{equation} \label{Eq_PE_salt_content_corrected} 306 \frac{\partial }{\partial t}\int\limits_{D\eta } {S\;dv} 307 =\frac{\partial}{\partial t} \left[ \;{\int\limits_D {S\;dv} +\int\limits_S {S\eta \;ds} } \right] 308 =\int\limits_S {\eta \;\frac{\partial S}{\partial t}ds} 309 \end{equation} 310 311 Although the total salt content is not exactly conserved with the linearized free surface, 312 its variations are driven by correlations of the time variation of surface salinity with the 313 sea surface height, which is a negligible term. This situation contrasts with the case of 314 the rigid lid approximation in which case freshwater forcing is represented by a virtual 315 salt flux, leading to a spurious source of salt at the ocean surface 316 \citep{Huang_JPO93, Roullet_Madec_JGR00}. 317 318 \newpage 319 $\ $\newline % force a new ligne 252 of the temporal derivatives, using a split-explicit method \citep{Killworth_al_JPO91, Zhang_Endoh_JGR92} 253 or the implicit scheme \citep{Dukowicz1994} or the addition of a filtering force in the momentum equation 254 \citep{Roullet_Madec_JGR00}. With the present release, \NEMO offers the choice between 255 an explicit free surface (see \S\ref{DYN_spg_exp}) or a split-explicit scheme strongly 256 inspired the one proposed by \citet{Shchepetkin_McWilliams_OM05} (see \S\ref{DYN_spg_ts}). 257 258 %\newpage 259 %$\ $\newline % force a new line 320 260 321 261 % ================================================================ … … 773 713 \end{equation} 774 714 775 The equations solved by the ocean model \eqref{Eq_PE} in $s-$coordinate can be written as follows :715 The equations solved by the ocean model \eqref{Eq_PE} in $s-$coordinate can be written as follows (see Appendix~\ref{Apdx_A_momentum}): 776 716 777 717 \vspace{0.5cm} 778 * momentum equation:718 $\bullet$ Vector invariant form of the momentum equation : 779 719 \begin{multline} \label{Eq_PE_sco_u} 780 \frac{ 1}{e_3} \frac{\partial \left( e_3\,u \right)}{\partial t}=720 \frac{\partial u }{\partial t}= 781 721 + \left( {\zeta +f} \right)\,v 782 722 - \frac{1}{2\,e_1} \frac{\partial}{\partial i} \left( u^2+v^2 \right) … … 787 727 \end{multline} 788 728 \begin{multline} \label{Eq_PE_sco_v} 789 \frac{ 1}{e_3} \frac{\partial \left( e_3\,v \right)}{\partial t}=729 \frac{\partial v }{\partial t}= 790 730 - \left( {\zeta +f} \right)\,u 791 731 - \frac{1}{2\,e_2 }\frac{\partial }{\partial j}\left( u^2+v^2 \right) … … 795 735 + D_v^{\vect{U}} + F_v^{\vect{U}} \quad 796 736 \end{multline} 737 738 \vspace{0.5cm} 739 $\bullet$ Vector invariant form of the momentum equation : 740 \begin{multline} \label{Eq_PE_sco_u} 741 \frac{1}{e_3} \frac{\partial \left( e_3\,u \right) }{\partial t}= 742 + \left( { f + \frac{1}{e_1 \; e_2 } 743 \left( v \frac{\partial e_2}{\partial i} 744 -u \frac{\partial e_1}{\partial j} \right)} \right) \, v \\ 745 - \frac{1}{e_1 \; e_2 \; e_3 } \left( 746 \frac{\partial \left( {e_2 \, e_3 \, u\,u} \right)}{\partial i} 747 + \frac{\partial \left( {e_1 \, e_3 \, v\,u} \right)}{\partial j} \right) 748 - \frac{1}{e_3 }\frac{\partial \left( { \omega\,u} \right)}{\partial k} \\ 749 - \frac{1}{e_1} \frac{\partial}{\partial i} \left( \frac{p_s + p_h}{\rho _o} \right) 750 + g\frac{\rho }{\rho _o}\sigma _1 751 + D_u^{\vect{U}} + F_u^{\vect{U}} \quad 752 \end{multline} 753 \begin{multline} \label{Eq_PE_sco_v} 754 \frac{1}{e_3} \frac{\partial \left( e_3\,v \right) }{\partial t}= 755 - \left( { f + \frac{1}{e_1 \; e_2} 756 \left( v \frac{\partial e_2}{\partial i} 757 -u \frac{\partial e_1}{\partial j} \right)} \right) \, u \\ 758 - \frac{1}{e_1 \; e_2 \; e_3 } \left( 759 \frac{\partial \left( {e_2 \; e_3 \,u\,v} \right)}{\partial i} 760 + \frac{\partial \left( {e_1 \; e_3 \,v\,v} \right)}{\partial j} \right) 761 - \frac{1}{e_3 } \frac{\partial \left( { \omega\,v} \right)}{\partial k} \\ 762 - \frac{1}{e_2 }\frac{\partial }{\partial j}\left( \frac{p_s+p_h }{\rho _o} \right) 763 + g\frac{\rho }{\rho _o }\sigma _2 764 + D_v^{\vect{U}} + F_v^{\vect{U}} \quad 765 \end{multline} 766 797 767 where the relative vorticity, \textit{$\zeta $}, the surface pressure gradient, and the hydrostatic 798 768 pressure have the same expressions as in $z$-coordinates although they do not represent 799 769 exactly the same quantities. $\omega$ is provided by the continuity equation 800 770 (see Appendix~\ref{Apdx_A}): 801 802 771 \begin{equation} \label{Eq_PE_sco_continuity} 803 772 \frac{\partial e_3}{\partial t} + e_3 \; \chi + \frac{\partial \omega }{\partial s} = 0 … … 809 778 810 779 \vspace{0.5cm} 811 *tracer equations:780 $\bullet$ tracer equations: 812 781 \begin{multline} \label{Eq_PE_sco_t} 813 782 \frac{1}{e_3} \frac{\partial \left( e_3\,T \right) }{\partial t}= … … 1023 992 \label{PE_zco_tilde} 1024 993 1025 The $\tilde{z}$-coordinate has been developed by \citet{Leclair_Madec_OM10s}. 1026 It is not available in the current version of \NEMO. 994 The $\tilde{z}$-coordinate has been developed by \citet{Leclair_Madec_OM11}. 995 It is available in \NEMO since the version 3.4. Nevertheless, it is currently not robust enough 996 to be used in all possible configurations. Its use is therefore not recommended. 997 1027 998 1028 999 \newpage … … 1157 1128 operator acting along $s-$surfaces (see \S\ref{LDF}). 1158 1129 1159 \subsubsection{Lateral second ordertracer diffusive operator}1160 1161 The lateral second ordertracer diffusive operator is defined by (see Appendix~\ref{Apdx_B}):1130 \subsubsection{Lateral Laplacian tracer diffusive operator} 1131 1132 The lateral Laplacian tracer diffusive operator is defined by (see Appendix~\ref{Apdx_B}): 1162 1133 \begin{equation} \label{Eq_PE_iso_tensor} 1163 1134 D^{lT}=\nabla {\rm {\bf .}}\left( {A^{lT}\;\Re \;\nabla T} \right) \qquad … … 1180 1151 ocean (see Appendix~\ref{Apdx_B}). 1181 1152 1153 For \textit{iso-level} diffusion, $r_1$ and $r_2 $ are zero. $\Re $ reduces to the identity 1154 in the horizontal direction, no rotation is applied. 1155 1182 1156 For \textit{geopotential} diffusion, $r_1$ and $r_2 $ are the slopes between the 1183 geopotential and computational surfaces: in $z$-coordinates they are zero 1184 ($r_1 = r_2 = 0$) while in $s$-coordinate (including $\textit{z*}$ case) they are 1185 equal to $\sigma _1$ and $\sigma _2$, respectively (see \eqref{Eq_PE_sco_slope} ). 1157 geopotential and computational surfaces: they are equal to $\sigma _1$ and $\sigma _2$, 1158 respectively (see \eqref{Eq_PE_sco_slope} ). 1186 1159 1187 1160 For \textit{isoneutral} diffusion $r_1$ and $r_2$ are the slopes between the isoneutral … … 1231 1204 to zero in the vicinity of the boundaries. The latter strategy is used in \NEMO (cf. Chap.~\ref{LDF}). 1232 1205 1233 \subsubsection{Lateral fourth ordertracer diffusive operator}1234 1235 The lateral fourth ordertracer diffusive operator is defined by:1206 \subsubsection{Lateral bilaplacian tracer diffusive operator} 1207 1208 The lateral bilaplacian tracer diffusive operator is defined by: 1236 1209 \begin{equation} \label{Eq_PE_bilapT} 1237 1210 D^{lT}=\Delta \left( {A^{lT}\;\Delta T} \right) 1238 1211 \qquad \text{where} \ D^{lT}=\Delta \left( {A^{lT}\;\Delta T} \right) 1239 1212 \end{equation} 1240 1241 1213 It is the second order operator given by \eqref{Eq_PE_iso_tensor} applied twice with 1242 1214 the eddy diffusion coefficient correctly placed. 1243 1215 1244 1245 \subsubsection{Lateral second order momentum diffusive operator} 1246 1247 The second order momentum diffusive operator along $z$- or $s$-surfaces is found by 1216 \subsubsection{Lateral Laplacian momentum diffusive operator} 1217 1218 The Laplacian momentum diffusive operator along $z$- or $s$-surfaces is found by 1248 1219 applying \eqref{Eq_PE_lap_vector} to the horizontal velocity vector (see Appendix~\ref{Apdx_B}): 1249 1220 \begin{equation} \label{Eq_PE_lapU} … … 1279 1250 of the Equator in a geographical coordinate system \citep{Lengaigne_al_JGR03}. 1280 1251 1281 \subsubsection{lateral fourth ordermomentum diffusive operator}1252 \subsubsection{lateral bilaplacian momentum diffusive operator} 1282 1253 1283 1254 As for tracers, the fourth order momentum diffusive operator along $z$ or $s$-surfaces
Note: See TracChangeset
for help on using the changeset viewer.