Changeset 11693
- Timestamp:
- 2019-10-14T14:53:52+02:00 (4 years ago)
- Location:
- NEMO/trunk/doc/latex
- Files:
-
- 27 edited
Legend:
- Unmodified
- Added
- Removed
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NEMO/trunk/doc/latex/NEMO/subfiles/apdx_DOMAINcfg.tex
r11690 r11693 530 530 This option is described in the Report by Levier \textit{et al.} (2007), available on the \NEMO\ web site. 531 531 532 \ onlyinsubfile{\input{../../global/epilogue}}532 \subinc{\input{../../global/epilogue}} 533 533 534 534 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/apdx_algos.tex
r11690 r11693 311 311 \begin{figure}[!ht] 312 312 \centering 313 \includegraphics[width=0.66\textwidth]{ALGOS_ISO_triad}313 %\includegraphics[width=0.66\textwidth]{ALGOS_ISO_triad} 314 314 \caption[Triads used in the Griffies's like iso-neutral diffision scheme for 315 315 $u$- and $w$-components)]{ … … 461 461 where $A_{e}$ is the eddy induced velocity coefficient, 462 462 and $r_i$ and $r_j$ the slopes between the iso-neutral and the geopotential surfaces. 463 %%gm wrong: to be modified with 2 2D streamfunctions 463 \cmtgm{Wrong: to be modified with 2 2D streamfunctions} 464 464 In other words, the eddy induced velocity can be derived from a vector streamfuntion, $\phi$, 465 465 which is given by $\phi = A_e\,\textbf{r}$ as $\textbf{U}^* = \textbf{k} \times \nabla \phi$. 466 %%end gm467 466 468 467 A traditional way to implement this additional advection is to add it to the eulerian velocity prior to … … 822 821 \ie\ the variance of the tracer is preserved by the discretisation of the skew fluxes. 823 822 824 \ onlyinsubfile{\input{../../global/epilogue}}823 \subinc{\input{../../global/epilogue}} 825 824 826 825 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/apdx_diff_opers.tex
r11598 r11693 421 421 that is a Laplacian diffusion is applied on momentum along the coordinate directions. 422 422 423 \ onlyinsubfile{\input{../../global/epilogue}}423 \subinc{\input{../../global/epilogue}} 424 424 425 425 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/apdx_invariants.tex
r11599 r11693 25 25 \clearpage 26 26 27 %%% Appendix put in gmcommentas it has not been updated for \zstar and s coordinate27 %%% Appendix put in cmtgm as it has not been updated for \zstar and s coordinate 28 28 %I'm writting this appendix. It will be available in a forthcoming release of the documentation 29 29 30 %\ gmcomment{30 %\cmtgm{ 31 31 32 32 %% ================================================================================================= … … 270 270 271 271 %gm comment 272 \ gmcomment{272 \cmtgm{ 273 273 The last equality comes from the following equation, 274 274 \begin{flalign*} … … 583 583 \label{subsec:INVARIANTS_2.6} 584 584 585 \ gmcomment{585 \cmtgm{ 586 586 A pressure gradient has no contribution to the evolution of the vorticity as the curl of a gradient is zero. 587 587 In the $z$-coordinate, this property is satisfied locally on a C-grid with 2nd order finite differences … … 694 694 695 695 %gm comment 696 \ gmcomment{696 \cmtgm{ 697 697 \begin{flalign*} 698 698 \sum\limits_{i,j,k} \biggl\{ p_t\;\partial_t b_t \biggr\} &&&\\ … … 1479 1479 %} 1480 1480 1481 \ onlyinsubfile{\input{../../global/epilogue}}1481 \subinc{\input{../../global/epilogue}} 1482 1482 1483 1483 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/apdx_s_coord.tex
r11599 r11693 584 584 the expression of the 3D divergence in the $s-$coordinates established above. 585 585 586 \ onlyinsubfile{\input{../../global/epilogue}}586 \subinc{\input{../../global/epilogue}} 587 587 588 588 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/apdx_triads.tex
r11690 r11693 1177 1177 \] 1178 1178 1179 \ onlyinsubfile{\input{../../global/epilogue}}1179 \subinc{\input{../../global/epilogue}} 1180 1180 1181 1181 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_ASM.tex
r11599 r11693 194 194 \end{clines} 195 195 196 \ onlyinsubfile{\input{../../global/epilogue}}196 \subinc{\input{../../global/epilogue}} 197 197 198 198 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_DIA.tex
r11690 r11693 55 55 A complete description of the use of this I/O server is presented in the next section. 56 56 57 %\ gmcomment{ % start of gmcomment57 %\cmtgm{ % start of gmcomment 58 58 59 59 %% ================================================================================================= … … 2061 2061 The maximum values from the run are also copied to the ocean.output file. 2062 2062 2063 \ onlyinsubfile{\input{../../global/epilogue}}2063 \subinc{\input{../../global/epilogue}} 2064 2064 2065 2065 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_DIU.tex
r11599 r11693 160 160 \] 161 161 162 \ onlyinsubfile{\input{../../global/epilogue}}162 \subinc{\input{../../global/epilogue}} 163 163 164 164 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_DOM.tex
r11690 r11693 695 695 \end{description} 696 696 697 \ onlyinsubfile{\input{../../global/epilogue}}697 \subinc{\input{../../global/epilogue}} 698 698 699 699 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_DYN.tex
r11690 r11693 67 67 Furthermore, the tendency terms associated with the 2D barotropic vorticity balance (when \texttt{trdvor?} is defined) 68 68 can be derived from the 3D terms. 69 \ gmcomment{STEVEN: not quite sure I've got the sense of the last sentence. does70 MISC correspond to "extracting tendency terms" or "vorticity balance"?}69 \cmtgm{STEVEN: not quite sure I've got the sense of the last sentence. 70 Does MISC correspond to "extracting tendency terms" or "vorticity balance"?} 71 71 72 72 %% ================================================================================================= … … 153 153 as changes in the divergence of the barotropic transport are absorbed into the change of the level thicknesses, 154 154 re-orientated downward. 155 \ gmcomment{not sure of this... to be modified with the change in emp setting}155 \cmtgm{not sure of this... to be modified with the change in emp setting} 156 156 In the case of a linear free surface, the time derivative in \autoref{eq:DYN_wzv} disappears. 157 157 The upper boundary condition applies at a fixed level $z=0$. … … 287 287 $u$ and $v$ are located at different grid points, 288 288 a price worth paying to avoid a double averaging in the pressure gradient term as in the $B$-grid. 289 \ gmcomment{ To circumvent this, Adcroft (ADD REF HERE)289 \cmtgm{ To circumvent this, Adcroft (ADD REF HERE) 290 290 Nevertheless, this technique strongly distort the phase and group velocity of Rossby waves....} 291 291 … … 516 516 In the vertical, the centred $2^{nd}$ order evaluation of the advection is preferred, \ie\ $u_{uw}^{ubs}$ and 517 517 $u_{vw}^{ubs}$ in \autoref{eq:DYN_adv_cen2} are used. 518 UBS is diffusive and is associated with vertical mixing of momentum. \ gmcomment{ gm pursue the518 UBS is diffusive and is associated with vertical mixing of momentum. \cmtgm{ gm pursue the 519 519 sentence:Since vertical mixing of momentum is a source term of the TKE equation... } 520 520 … … 534 534 there is also the possibility of using a $4^{th}$ order evaluation of the advective velocity as in ROMS. 535 535 This is an error and should be suppressed soon. 536 \ gmcomment{action : this have to be done}536 \cmtgm{action : this have to be done} 537 537 538 538 %% ================================================================================================= … … 915 915 it is still significant as shown by \citet{levier.treguier.ea_rpt07} in the case of an analytical barotropic Kelvin wave. 916 916 917 \ gmcomment{ %%% copy from griffies Book917 \cmtgm{ %%% copy from griffies Book 918 918 919 919 \textbf{title: Time stepping the barotropic system } … … 1043 1043 1044 1044 %% gm %%======>>>> given here the discrete eqs provided to the solver 1045 \ gmcomment{ %%% copy from chap-model basics1045 \cmtgm{ %%% copy from chap-model basics 1046 1046 \[ 1047 1047 % \label{eq:DYN_spg_flt} … … 1054 1054 and $\mathrm {\mathbf M}$ represents the collected contributions of the Coriolis, hydrostatic pressure gradient, 1055 1055 non-linear and viscous terms in \autoref{eq:MB_dyn}. 1056 } %end gmcomment1056 } %end cmtgm 1057 1057 1058 1058 Note that in the linear free surface formulation (\texttt{vvl?} not defined), … … 1082 1082 no slip or partial slip boundary conditions are applied according to the user's choice (see \autoref{chap:LBC}). 1083 1083 1084 \ gmcomment{1084 \cmtgm{ 1085 1085 Hyperviscous operators are frequently used in the simulation of turbulent flows to 1086 1086 control the dissipation of unresolved small scale features. … … 1183 1183 the first derivative term normal to the coast depends on the free or no-slip lateral boundary conditions chosen, 1184 1184 while the third derivative terms normal to the coast are set to zero (see \autoref{chap:LBC}). 1185 \ gmcomment{add a remark on the the change in the position of the coefficient}1185 \cmtgm{add a remark on the the change in the position of the coefficient} 1186 1186 1187 1187 %% ================================================================================================= … … 1252 1252 the snow-ice mass is taken into account when computing the surface pressure gradient. 1253 1253 1254 \ gmcomment{ missing : the lateral boundary condition !!! another external forcing1254 \cmtgm{ missing : the lateral boundary condition !!! another external forcing 1255 1255 } 1256 1256 … … 1596 1596 and only array swapping and Asselin filtering is done in \mdl{dynnxt}. 1597 1597 1598 \ onlyinsubfile{\input{../../global/epilogue}}1598 \subinc{\input{../../global/epilogue}} 1599 1599 1600 1600 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_LBC.tex
r11690 r11693 25 25 \clearpage 26 26 27 %gm% add here introduction to this chapter 27 \cmtgm{Add here introduction to this chapter} 28 28 29 29 %% ================================================================================================= … … 708 708 direction of rotation). %, e.g. anticlockwise or clockwise. 709 709 710 \ onlyinsubfile{\input{../../global/epilogue}}710 \subinc{\input{../../global/epilogue}} 711 711 712 712 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_LDF.tex
r11690 r11693 68 68 \label{sec:LDF_slp} 69 69 70 \ gmcomment{70 \cmtgm{ 71 71 we should emphasize here that the implementation is a rather old one. 72 72 Better work can be achieved by using \citet{griffies.gnanadesikan.ea_JPO98, griffies_bk04} iso-neutral scheme. … … 84 84 $r_{1f}$, $r_{1vw}$, $r_{2t}$, $r_{2vw}$ for $v$. 85 85 86 %gm% add here afigure of the slope in i-direction 86 \cmtgm{Add here afigure of the slope in i-direction} 87 87 88 88 %% ================================================================================================= … … 94 94 the diffusive fluxes in the three directions are set to zero and $T$ is assumed to be horizontally uniform, 95 95 \ie\ a linear function of $z_T$, the depth of a $T$-point. 96 %gm { Steven : My version is obviously wrong since I'm left with an arbitrary constant which is the local vertical temperature gradient} 96 \cmtgm{Steven : My version is obviously wrong since 97 I'm left with an arbitrary constant which is the local vertical temperature gradient} 97 98 98 99 \begin{equation} … … 112 113 \end{equation} 113 114 114 %gm% caution I'm not sure the simplification was a good idea! 115 \cmtgm{Caution I'm not sure the simplification was a good idea!} 115 116 116 117 These slopes are computed once in \rou{ldf\_slp\_init} when \np[=.true.]{ln_sco}{ln\_sco}, … … 144 145 \end{equation} 145 146 146 %gm% rewrite this as the explanation is not very clear !!! 147 \cmtgm{rewrite this as the explanation is not very clear !!!} 147 148 %In practice, \autoref{eq:LDF_slp_iso} is of little help in evaluating the neutral surface slopes. Indeed, for an unsimplified equation of state, the density has a strong dependancy on pressure (here approximated as the depth), therefore applying \autoref{eq:LDF_slp_iso} using the $in situ$ density, $\rho$, computed at T-points leads to a flattening of slopes as the depth increases. This is due to the strong increase of the $in situ$ density with depth. 148 149 … … 173 174 will include a pressure dependent part, leading to the wrong evaluation of the neutral slopes. 174 175 175 %gm%176 176 Note: The solution for $s$-coordinate passes trough the use of different (and better) expression for 177 177 the constraint on iso-neutral fluxes. … … 182 182 \alpha \ \textbf{F}(T) = \beta \ \textbf{F}(S) 183 183 \] 184 % gm{where vector F is ....}184 \cmtgm{where vector F is ....} 185 185 186 186 This constraint leads to the following definition for the slopes: … … 229 229 This allows an iso-neutral diffusion scheme without additional background horizontal mixing. 230 230 This technique can be viewed as a diffusion operator that acts along large-scale 231 (2~$\Delta$x) \ gmcomment{2deltax doesnt seem very large scale} iso-neutral surfaces.231 (2~$\Delta$x) \cmtgm{2deltax doesnt seem very large scale} iso-neutral surfaces. 232 232 The diapycnal diffusion required for numerical stability is thus minimized and its net effect on the flow is quite small when compared to the effect of an horizontal background mixing. 233 233 … … 478 478 479 479 %%gm from Triad appendix : to be incorporated.... 480 \ gmcomment{480 \cmtgm{ 481 481 Values of iso-neutral diffusivity and GM coefficient are set as described in \autoref{sec:LDF_coef}. 482 482 If none of the keys \key{traldf\_cNd}, N=1,2,3 is set (the default), spatially constant iso-neutral $A_l$ and … … 544 544 \colorbox{yellow}{TBC} 545 545 546 \ onlyinsubfile{\input{../../global/epilogue}}546 \subinc{\input{../../global/epilogue}} 547 547 548 548 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_OBS.tex
r11690 r11693 1180 1180 \end{figure} 1181 1181 1182 \ onlyinsubfile{\input{../../global/epilogue}}1182 \subinc{\input{../../global/epilogue}} 1183 1183 1184 1184 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_SBC.tex
r11690 r11693 880 880 %ENDIF 881 881 882 %\gmcomment{ word doc of runoffs: 883 %In the current \NEMO\ setup river runoff is added to emp fluxes, these are then applied at just the sea surface as a volume change (in the variable volume case this is a literal volume change, and in the linear free surface case the free surface is moved) and a salt flux due to the concentration/dilution effect. There is also an option to increase vertical mixing near river mouths; this gives the effect of having a 3d river. All river runoff and emp fluxes are assumed to be fresh water (zero salinity) and at the same temperature as the sea surface. 884 %Our aim was to code the option to specify the temperature and salinity of river runoff, (as well as the amount), along with the depth that the river water will affect. This would make it possible to model low salinity outflow, such as the Baltic, and would allow the ocean temperature to be affected by river runoff. 885 886 %The depth option makes it possible to have the river water affecting just the surface layer, throughout depth, or some specified point in between. 887 888 %To do this we need to treat evaporation/precipitation fluxes and river runoff differently in the tra_sbc module. We decided to separate them throughout the code, so that the variable emp represented solely evaporation minus precipitation fluxes, and a new 2d variable rnf was added which represents the volume flux of river runoff (in kg/m2s to remain consistent with emp). This meant many uses of emp and emps needed to be changed, a list of all modules which use emp or emps and the changes made are below: 882 \cmtgm{ word doc of runoffs: 883 In the current \NEMO\ setup river runoff is added to emp fluxes, 884 these are then applied at just the sea surface as a volume change (in the variable volume case 885 this is a literal volume change, and in the linear free surface case the free surface is moved) 886 and a salt flux due to the concentration/dilution effect. 887 There is also an option to increase vertical mixing near river mouths; 888 this gives the effect of having a 3d river. 889 All river runoff and emp fluxes are assumed to be fresh water (zero salinity) and 890 at the same temperature as the sea surface. 891 Our aim was to code the option to specify the temperature and salinity of river runoff, 892 (as well as the amount), along with the depth that the river water will affect. 893 This would make it possible to model low salinity outflow, such as the Baltic, 894 and would allow the ocean temperature to be affected by river runoff. 895 896 The depth option makes it possible to have the river water affecting just the surface layer, 897 throughout depth, or some specified point in between. 898 899 To do this we need to treat evaporation/precipitation fluxes and river runoff differently in 900 the \mdl{tra_sbc} module. 901 We decided to separate them throughout the code, 902 so that the variable emp represented solely evaporation minus precipitation fluxes, 903 and a new 2d variable rnf was added which represents the volume flux of river runoff 904 (in $kg/m^2s$ to remain consistent with $emp$). 905 This meant many uses of emp and emps needed to be changed, 906 a list of all modules which use $emp$ or $emps$ and the changes made are below:} 889 907 890 908 %% ================================================================================================= … … 908 926 Two different bulk formulae are available: 909 927 910 911 912 913 914 915 916 917 918 919 920 921 922 923 924 925 926 927 928 929 930 928 \begin{description} 929 \item [{\np[=1]{nn_isfblk}{nn\_isfblk}}]: The melt rate is based on a balance between the upward ocean heat flux and 930 the latent heat flux at the ice shelf base. A complete description is available in \citet{hunter_rpt06}. 931 \item [{\np[=2]{nn_isfblk}{nn\_isfblk}}]: The melt rate and the heat flux are based on a 3 equations formulation 932 (a heat flux budget at the ice base, a salt flux budget at the ice base and a linearised freezing point temperature equation). 933 A complete description is available in \citet{jenkins_JGR91}. 934 \end{description} 935 936 Temperature and salinity used to compute the melt are the average temperature in the top boundary layer \citet{losch_JGR08}. 937 Its thickness is defined by \np{rn_hisf_tbl}{rn\_hisf\_tbl}. 938 The fluxes and friction velocity are computed using the mean temperature, salinity and velocity in the the first \np{rn_hisf_tbl}{rn\_hisf\_tbl} m. 939 Then, the fluxes are spread over the same thickness (ie over one or several cells). 940 If \np{rn_hisf_tbl}{rn\_hisf\_tbl} larger than top $e_{3}t$, there is no more feedback between the freezing point at the interface and the the top cell temperature. 941 This can lead to super-cool temperature in the top cell under melting condition. 942 If \np{rn_hisf_tbl}{rn\_hisf\_tbl} smaller than top $e_{3}t$, the top boundary layer thickness is set to the top cell thickness.\\ 943 944 Each melt bulk formula depends on a exchange coeficient ($\Gamma^{T,S}$) between the ocean and the ice. 945 There are 3 different ways to compute the exchange coeficient: 946 \begin{description} 947 \item [{\np[=0]{nn_gammablk}{nn\_gammablk}}]: The salt and heat exchange coefficients are constant and defined by \np{rn_gammas0}{rn\_gammas0} and \np{rn_gammat0}{rn\_gammat0}. 948 \begin{gather*} 931 949 % \label{eq:SBC_isf_gamma_iso} 932 933 934 935 936 937 938 939 940 941 942 943 944 \[945 \gamma^{T,S} = \frac{u_{*}}{\Gamma_{Turb} + \Gamma^{T,S}_{Mole}}946 \]947 948 949 950 951 952 953 954 955 956 957 958 959 960 961 962 963 964 965 966 967 As in \np[=1]{nn_isf}{nn\_isf}, the fluxes are spread over the top boundary layer thickness (\np{rn_hisf_tbl}{rn\_hisf\_tbl})\\950 \gamma^{T} = rn\_gammat0 \\ 951 \gamma^{S} = rn\_gammas0 952 \end{gather*} 953 This is the recommended formulation for ISOMIP. 954 \item [{\np[=1]{nn_gammablk}{nn\_gammablk}}]: The salt and heat exchange coefficients are velocity dependent and defined as 955 \begin{gather*} 956 \gamma^{T} = rn\_gammat0 \times u_{*} \\ 957 \gamma^{S} = rn\_gammas0 \times u_{*} 958 \end{gather*} 959 where $u_{*}$ is the friction velocity in the top boundary layer (ie first \np{rn_hisf_tbl}{rn\_hisf\_tbl} meters). 960 See \citet{jenkins.nicholls.ea_JPO10} for all the details on this formulation. It is the recommended formulation for realistic application. 961 \item [{\np[=2]{nn_gammablk}{nn\_gammablk}}]: The salt and heat exchange coefficients are velocity and stability dependent and defined as: 962 \[ 963 \gamma^{T,S} = \frac{u_{*}}{\Gamma_{Turb} + \Gamma^{T,S}_{Mole}} 964 \] 965 where $u_{*}$ is the friction velocity in the top boundary layer (ie first \np{rn_hisf_tbl}{rn\_hisf\_tbl} meters), 966 $\Gamma_{Turb}$ the contribution of the ocean stability and 967 $\Gamma^{T,S}_{Mole}$ the contribution of the molecular diffusion. 968 See \citet{holland.jenkins_JPO99} for all the details on this formulation. 969 This formulation has not been extensively tested in \NEMO\ (not recommended). 970 \end{description} 971 \item [{\np[=2]{nn_isf}{nn\_isf}}]: The ice shelf cavity is not represented. 972 The fwf and heat flux are computed using the \citet{beckmann.goosse_OM03} parameterisation of isf melting. 973 The fluxes are distributed along the ice shelf edge between the depth of the average grounding line (GL) 974 (\np{sn_depmax_isf}{sn\_depmax\_isf}) and the base of the ice shelf along the calving front 975 (\np{sn_depmin_isf}{sn\_depmin\_isf}) as in (\np[=3]{nn_isf}{nn\_isf}). 976 The effective melting length (\np{sn_Leff_isf}{sn\_Leff\_isf}) is read from a file. 977 \item [{\np[=3]{nn_isf}{nn\_isf}}]: The ice shelf cavity is not represented. 978 The fwf (\np{sn_rnfisf}{sn\_rnfisf}) is prescribed and distributed along the ice shelf edge between 979 the depth of the average grounding line (GL) (\np{sn_depmax_isf}{sn\_depmax\_isf}) and 980 the base of the ice shelf along the calving front (\np{sn_depmin_isf}{sn\_depmin\_isf}). 981 The heat flux ($Q_h$) is computed as $Q_h = fwf \times L_f$. 982 \item [{\np[=4]{nn_isf}{nn\_isf}}]: The ice shelf cavity is opened (\np[=.true.]{ln_isfcav}{ln\_isfcav} needed). 983 However, the fwf is not computed but specified from file \np{sn_fwfisf}{sn\_fwfisf}). 984 The heat flux ($Q_h$) is computed as $Q_h = fwf \times L_f$. 985 As in \np[=1]{nn_isf}{nn\_isf}, the fluxes are spread over the top boundary layer thickness (\np{rn_hisf_tbl}{rn\_hisf\_tbl}) 968 986 \end{description} 969 987 … … 1521 1539 % in ocean-ice models. 1522 1540 1523 \ onlyinsubfile{\input{../../global/epilogue}}1541 \subinc{\input{../../global/epilogue}} 1524 1542 1525 1543 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_STO.tex
r11598 r11693 205 205 The first four parameters define the stochastic part of equation of state. 206 206 207 \ onlyinsubfile{\input{../../global/epilogue}}207 \subinc{\input{../../global/epilogue}} 208 208 209 209 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_TRA.tex
r11690 r11693 452 452 restore this property. 453 453 454 %%%gmcomment : Cross term are missing in the current implementation.... 454 \cmtgm{Cross term are missing in the current implementation....} 455 455 456 456 %% ================================================================================================= … … 1037 1037 %!! i.e. transport proportional to the along-slope density gradient 1038 1038 1039 %%%gmcomment : this section has to be really written 1039 \cmtgm{This section has to be really written} 1040 1040 1041 1041 When applying an advective BBL (\np[=1..2]{nn_bbl_adv}{nn\_bbl\_adv}), … … 1374 1374 \label{sec:TRA_zpshde} 1375 1375 1376 \ gmcomment{STEVEN: to be consistent with earlier discussion of differencing and averaging operators,1376 \cmtgm{STEVEN: to be consistent with earlier discussion of differencing and averaging operators, 1377 1377 I've changed "derivative" to "difference" and "mean" to "average"} 1378 1378 … … 1464 1464 Sensitivity of the advection schemes to the way horizontal averages are performed in 1465 1465 the vicinity of partial cells should be further investigated in the near future. 1466 \ gmcomment{gm : this last remark has to be done}1467 1468 \ onlyinsubfile{\input{../../global/epilogue}}1466 \cmtgm{gm : this last remark has to be done} 1467 1468 \subinc{\input{../../global/epilogue}} 1469 1469 1470 1470 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_ZDF.tex
r11690 r11693 28 28 \clearpage 29 29 30 %gm% Add here a small introduction to ZDF and naming of the different physics (similar to what have been written for TRA and DYN. 30 \cmtgm{ Add here a small introduction to ZDF and naming of the different physics 31 (similar to what have been written for TRA and DYN).} 31 32 32 33 %% ================================================================================================= … … 1642 1643 \end{figure} 1643 1644 1644 \ onlyinsubfile{\input{../../global/epilogue}}1645 \subinc{\input{../../global/epilogue}} 1645 1646 1646 1647 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_cfgs.tex
r11690 r11693 292 292 Unlike ordinary river points the Baltic inputs also include salinity and temperature data. 293 293 294 \ onlyinsubfile{\input{../../global/epilogue}}294 \subinc{\input{../../global/epilogue}} 295 295 296 296 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_conservation.tex
r11598 r11693 334 334 It has not been implemented. 335 335 336 \ onlyinsubfile{\input{../../global/epilogue}}336 \subinc{\input{../../global/epilogue}} 337 337 338 338 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_misc.tex
r11690 r11693 415 415 increment also applies to the time.step file which is otherwise updated every timestep. 416 416 417 \ onlyinsubfile{\input{../../global/epilogue}}417 \subinc{\input{../../global/epilogue}} 418 418 419 419 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_model_basics.tex
r11690 r11693 579 579 an explicit computation of vertical advection relative to the moving s-surfaces. 580 580 581 %\gmcomment{ 582 %A key point here is that the $s$-coordinate depends on $(i,j)$ ==> horizontal pressure gradient... 581 \cmtgm{A key point here is that the $s$-coordinate depends on $(i,j)$ 582 ==> horizontal pressure gradient...} 583 583 The generalized vertical coordinates used in ocean modelling are not orthogonal, 584 584 which contrasts with many other applications in mathematical physics. … … 680 680 and similar expressions are used for mixing and forcing terms. 681 681 682 \ gmcomment{682 \cmtgm{ 683 683 \colorbox{yellow}{ to be updated $= = >$} 684 684 Add a few works on z and zps and s and underlies the differences between all of them … … 1150 1150 Nevertheless it is currently not available in the iso-neutral case. 1151 1151 1152 \ onlyinsubfile{\input{../../global/epilogue}}1152 \subinc{\input{../../global/epilogue}} 1153 1153 1154 1154 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_model_basics_zstar.tex
r11690 r11693 147 147 \begin{figure}[!t] 148 148 \centering 149 \includegraphics[width=0.66\textwidth]{MBZ_DYN_dynspg_ts}149 %\includegraphics[width=0.66\textwidth]{MBZ_DYN_dynspg_ts} 150 150 \caption[Schematic of the split-explicit time stepping scheme for 151 151 the barotropic and baroclinic modes, after \citet{Griffies2004?}]{ … … 311 311 In particular, this means that in filtered case, the matrix to be inverted has to be recomputed at each time-step. 312 312 313 \ onlyinsubfile{\input{../../global/epilogue}}313 \subinc{\input{../../global/epilogue}} 314 314 315 315 \end{document} -
NEMO/trunk/doc/latex/NEMO/subfiles/chap_time_domain.tex
r11690 r11693 31 31 % - daymod: definition of the time domain (nit000, nitend and the calendar) 32 32 33 \ gmcomment{STEVEN :maybe a picture of the directory structure in the introduction which33 \cmtgm{STEVEN :maybe a picture of the directory structure in the introduction which 34 34 could be referred to here, would help ==> to be added} 35 35 … … 158 158 \end{equation} 159 159 160 %%gm 161 %%gm UPDATE the next paragraphs with time varying thickness ... 162 %%gm 160 \cmtgm{UPDATE the next paragraphs with time varying thickness ...} 163 161 164 162 This scheme is rather time consuming since it requires a matrix inversion. … … 213 211 Fast barotropic motions (such as tides) are also simulated with a better accuracy. 214 212 215 %\ gmcomment{213 %\cmtgm{ 216 214 \begin{figure} 217 215 \centering … … 328 326 the \nam{run}{run} namelist variables. 329 327 330 \ gmcomment{328 \cmtgm{ 331 329 add here how to force the restart to contain only one time step for operational purposes 332 330 … … 338 336 } 339 337 340 \ gmcomment{ % add a subsection here338 \cmtgm{ % add a subsection here 341 339 342 340 %% ================================================================================================= … … 353 351 } %% end add 354 352 355 \ gmcomment{ % add implicit in vvl case and Crant-Nicholson scheme353 \cmtgm{ % add implicit in vvl case and Crant-Nicholson scheme 356 354 357 355 Implicit time stepping in case of variable volume thickness. … … 404 402 } 405 403 406 \ onlyinsubfile{\input{../../global/epilogue}}404 \subinc{\input{../../global/epilogue}} 407 405 408 406 \end{document} -
NEMO/trunk/doc/latex/global/document.tex
r11591 r11693 18 18 %% End of common preamble between main and sub-files 19 19 %% Override custom cmds for full manual compilation 20 \newcommand{\ onlyinsubfile}[1]{#1}21 \newcommand{\ notinsubfile}[1]{}20 \newcommand{\subinc}[1]{#1} 21 \newcommand{\subexc}[1]{} 22 22 23 23 \begin{document} 24 24 25 \renewcommand{\ onlyinsubfile}[1]{}26 \renewcommand{\ notinsubfile}[1]{#1}25 \renewcommand{\subinc}[1]{} 26 \renewcommand{\subexc}[1]{#1} 27 27 28 28 -
NEMO/trunk/doc/latex/global/new_cmds.tex
r11584 r11693 34 34 35 35 %% Gurvan's comments 36 \newcommand{\ gmcomment}[1]{}36 \newcommand{\cmtgm}[1]{} 37 37 38 38 %% Maths -
NEMO/trunk/doc/latex/global/packages.tex
r11688 r11693 18 18 %% Issue with fontawesome pkg: path to FontAwesome.otf has to be hard-coded 19 19 \defaultfontfeatures{ 20 Path = / usr/local/texlive/2019/texmf-dist/fonts/opentype/public/fontawesome/20 Path = /home/ntmlod/.local/texlive2019/texmf-dist/fonts/opentype/public/fontawesome/ 21 21 } 22 22 \usepackage{academicons, fontawesome, newtxtext}
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