1 | \chapter{Physical parameterizations of the generic model: some references} |
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2 | |
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3 | \label{sc:phystd} |
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4 | |
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5 | \section{General} |
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6 | |
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7 | The Generic Climate Model uses a large number of physical parameterizations based on various scientific theories. Some also use specific numerical methods. A list of these parameterizations is given below, along with the most appropriate references for each one. Most of these documents can be found at\\ |
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8 | \verb+http://www.lmd.jussieu.fr/mars.html+. |
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9 | |
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10 | \paragraph{General references:} |
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11 | No documents attempt to give a complete scientific description of the current |
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12 | version of the GCM. Here's a reference to a Mars GCM description: |
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13 | \begin{itemize} |
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14 | \item {\it Forget et al.} [1999] (article |
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15 | published in the JGR) |
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16 | \item ``Updated Detailed Design Document for the Model'' |
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17 | (ESA contract, Work Package 6, 1999, available on the web) |
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18 | which is simply a compilation of the preceding article with |
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19 | a few additions that were published separately. |
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20 | \end{itemize} |
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21 | |
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22 | \nocite{Forg:99} |
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23 | |
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24 | \section{Radiative transfer} |
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25 | |
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26 | The radiative transfer parameterizations are used to calculate the heating |
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27 | and cooling ratios in the atmosphere and the radiative flux at the surface. |
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28 | |
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29 | [TO WRITE: IMPORTANT SECTION - REFERENCES HERE ARE FOR MARS ONLY] |
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30 | |
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31 | %\end{itemize} |
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32 | |
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33 | |
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34 | \subsection{\bf Absorption/emission and diffusion by dust:} |
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35 | |
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36 | \subsubsection*{Dust spatial distribution} |
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37 | (\verb+ dustopacity+) |
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38 | |
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39 | \begin{itemize} |
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40 | \item Vertical distribution and description of ``MGS'' and ``Viking'' scenarios |
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41 | in the ESA report {\it Mars Climate Database V3.0 Detailed Design Document} |
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42 | by Lewis et al. (2001), available on the web. |
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43 | \item For the ``MY24'' scenario, dust distribution obtained from assimilation |
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44 | of TES data is used (and read via the \verb+readtesassim+ routine). |
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45 | \end{itemize} |
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46 | \nocite{Forg:99,Lewi:99} |
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47 | |
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48 | \subsubsection*{Thermal IR radiation} |
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49 | (\verb+ lwmain+) |
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50 | \begin{itemize} |
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51 | \item Numerical method: {\it Toon et al.} [1989] |
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52 | \item Optical properties of dust: {\it Forget} [1998] |
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53 | \nocite{Toon:89,Forg:98grl} |
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54 | \end{itemize} |
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55 | |
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56 | \subsubsection*{Solar radiation} |
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57 | (\verb+ swmain+) |
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58 | \begin{itemize} |
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59 | \item Numerical method: {\it Fouquart and Bonel} [1980] |
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60 | \nocite{Fouq:80} |
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61 | |
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62 | \item Optical properties of dust: |
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63 | see the discussion in {\it Forget et al. } [1999], which quotes |
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64 | {\it Ockert-Bell et al.} [1997] and {\it Clancy and Lee} [1991]. |
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65 | \nocite{Ocke:97,Clan:91} |
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66 | \end{itemize} |
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67 | |
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68 | \section{Subgrid atmospheric dynamical processes} |
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69 | |
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70 | \subsection{Turbulent diffusion in the upper layer} |
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71 | (\verb+ vdifc+) |
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72 | |
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73 | \begin{itemize} |
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74 | \item Implicit numerical scheme in the vertical: |
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75 | see the thesis of Laurent Li (LMD, Universit\'e Paris 7, 1990), Appendix C2. |
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76 | |
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77 | \item Calculation of the turbulent diffusion coefficients: |
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78 | {\it Forget et al. } [1999]. |
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79 | \end{itemize} |
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80 | |
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81 | \subsection{Convection} |
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82 | (\verb+ convadj+) |
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83 | |
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84 | See {\it Hourdin et al.} [1993] |
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85 | \nocite{Hour:93} |
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86 | |
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87 | \section{Surface thermal conduction} |
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88 | (\verb+soil+) |
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89 | |
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90 | Thesis of Fr\'ed\'eric Hourdin (LMD, Universit\'e Paris 7, 1992) : |
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91 | section 3.3 (equations) and Appendix A (Numerical scheme). |
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92 | |
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93 | \section{CO$_2$ Condensation} |
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94 | |
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95 | In {\it Forget et al.} [1998] (article published in Icarus): \\ |
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96 | - Numerical method for calculating the condensation and sublimation levels |
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97 | at the surface and in the atmosphere (\verb+ newcondens+) |
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98 | explained in the appendix. |
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99 | \\ |
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100 | - Description of the numerical scheme for calculating the evolution of CO$_2$ |
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101 | snow emissivity (\verb+co2snow+) explained in section 4.1 |
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102 | \nocite{Forg:98} |
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103 | |
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104 | \section{Tracer transport and sources} |
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105 | \begin{itemize} |
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106 | \item ``Van-Leer'' transport scheme used in the dynamical part |
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107 | (\verb+ tracvl+ and \verb+ vlsplt+ in the dynamical part): |
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108 | {\it Hourdin and Armengaud} [1999] \nocite{Hour:99} |
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109 | |
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110 | \item Transport by turbulent diffusion (in \verb+ vdifc+), convection |
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111 | (in \verb+ convadj+), sedimentation (\verb+ sedim+), |
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112 | dust lifting by winds (\verb+ dustlift+) : |
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113 | see note ``Preliminary design of dust lifting and transport in the Model'' |
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114 | (ESA contract, Work Package 4, 1998, available on the web). |
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115 | |
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116 | |
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117 | %\item Simplified water cycle (source in {\tt vdifc}, {\tt |
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118 | %watercloud}) : and also see the Maitrise study by Delphine Nobileau, LMD, 2000. |
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119 | \item {\bf Watercycle}, see {\it Montmessin et al.} [2004] |
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120 | \nocite{Mont:04jgr} |
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121 | |
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122 | \end{itemize} |
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123 | |
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124 | |
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