\chapter{Physical parameterizations of the generic model: some references} \label{sc:phystd} \section{General} 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\\ \verb+http://www.lmd.jussieu.fr/mars.html+. \paragraph{General references:} No documents attempt to give a complete scientific description of the current version of the GCM. Here's a reference to a Mars GCM description: \begin{itemize} \item {\it Forget et al.} [1999] (article published in the JGR) \item ``Updated Detailed Design Document for the Model'' (ESA contract, Work Package 6, 1999, available on the web) which is simply a compilation of the preceding article with a few additions that were published separately. \end{itemize} \nocite{Forg:99} \section{Radiative transfer} The radiative transfer parameterizations are used to calculate the heating and cooling ratios in the atmosphere and the radiative flux at the surface. [TO WRITE: IMPORTANT SECTION - REFERENCES HERE ARE FOR MARS ONLY] %\end{itemize} \subsection{\bf Absorption/emission and diffusion by dust:} \subsubsection*{Dust spatial distribution} (\verb+ dustopacity+) \begin{itemize} \item Vertical distribution and description of ``MGS'' and ``Viking'' scenarios in the ESA report {\it Mars Climate Database V3.0 Detailed Design Document} by Lewis et al. (2001), available on the web. \item For the ``MY24'' scenario, dust distribution obtained from assimilation of TES data is used (and read via the \verb+readtesassim+ routine). \end{itemize} \nocite{Forg:99,Lewi:99} \subsubsection*{Thermal IR radiation} (\verb+ lwmain+) \begin{itemize} \item Numerical method: {\it Toon et al.} [1989] \item Optical properties of dust: {\it Forget} [1998] \nocite{Toon:89,Forg:98grl} \end{itemize} \subsubsection*{Solar radiation} (\verb+ swmain+) \begin{itemize} \item Numerical method: {\it Fouquart and Bonel} [1980] \nocite{Fouq:80} \item Optical properties of dust: see the discussion in {\it Forget et al. } [1999], which quotes {\it Ockert-Bell et al.} [1997] and {\it Clancy and Lee} [1991]. \nocite{Ocke:97,Clan:91} \end{itemize} \section{Subgrid atmospheric dynamical processes} \subsection{Turbulent diffusion in the upper layer} (\verb+ vdifc+) \begin{itemize} \item Implicit numerical scheme in the vertical: see the thesis of Laurent Li (LMD, Universit\'e Paris 7, 1990), Appendix C2. \item Calculation of the turbulent diffusion coefficients: {\it Forget et al. } [1999]. \end{itemize} \subsection{Convection} (\verb+ convadj+) See {\it Hourdin et al.} [1993] \nocite{Hour:93} \section{Surface thermal conduction} (\verb+soil+) Thesis of Fr\'ed\'eric Hourdin (LMD, Universit\'e Paris 7, 1992) : section 3.3 (equations) and Appendix A (Numerical scheme). \section{CO$_2$ Condensation} In {\it Forget et al.} [1998] (article published in Icarus): \\ - Numerical method for calculating the condensation and sublimation levels at the surface and in the atmosphere (\verb+ newcondens+) explained in the appendix. \\ - Description of the numerical scheme for calculating the evolution of CO$_2$ snow emissivity (\verb+co2snow+) explained in section 4.1 \nocite{Forg:98} \section{Tracer transport and sources} \begin{itemize} \item ``Van-Leer'' transport scheme used in the dynamical part (\verb+ tracvl+ and \verb+ vlsplt+ in the dynamical part): {\it Hourdin and Armengaud} [1999] \nocite{Hour:99} \item Transport by turbulent diffusion (in \verb+ vdifc+), convection (in \verb+ convadj+), sedimentation (\verb+ sedim+), dust lifting by winds (\verb+ dustlift+) : see note ``Preliminary design of dust lifting and transport in the Model'' (ESA contract, Work Package 4, 1998, available on the web). %\item Simplified water cycle (source in {\tt vdifc}, {\tt %watercloud}) : and also see the Maitrise study by Delphine Nobileau, LMD, 2000. \item {\bf Watercycle}, see {\it Montmessin et al.} [2004] \nocite{Mont:04jgr} \end{itemize}