source: trunk/DOC/documentation/parallel.tex @ 3552

Last change on this file since 3552 was 892, checked in by slebonnois, 12 years ago

SL: Important commit ! Adaptation of Venus physics to parallel computation / template for arch on the LMD servers using ifort / documentation for 1D column physics and for parallel computations

File size: 2.6 KB
Line 
1\documentclass[a4paper,10pt]{article}
2%\usepackage{graphicx}
3\usepackage{natbib}  % si appel à bibtex
4%\usepackage[francais]{babel}
5%\usepackage[latin1]{inputenc}  % accents directs (é...), avec babel
6%\usepackage{rotating}
7
8\setlength{\hoffset}{-1.in}
9\setlength{\oddsidemargin}{3.cm}
10\setlength{\textwidth}{15.cm}
11\setlength{\marginparsep}{0.mm}
12\setlength{\marginparwidth}{0.mm}
13
14\setlength{\voffset}{-1.in}
15\setlength{\topmargin}{0.mm}
16\setlength{\headheight}{0.mm}
17\setlength{\headsep}{30.mm}
18\setlength{\textheight}{24.cm}
19\setlength{\footskip}{1.cm}
20
21\setlength{\parindent}{0.mm}
22\setlength{\parskip}{1 em}
23\newcommand{\ten}[1]{$\times 10^{#1}$~} 
24\renewcommand{\baselinestretch}{1.}
25
26\begin{document}
27\pagestyle{plain}
28
29\begin{center}
30{\bf \LARGE 
31Documentation for LMDZ, Planets version
32
33\vspace{1cm}
34\Large
35Running the GCM in parallel using MPI
36-- Venus
37}
38
39\vspace{1cm}
40S\'ebastien Lebonnois
41
42\vspace{1cm}
43Latest version: \today
44\end{center}
45
46
47\section{Compilation}
48
49To compile the GCM for parallel runs using MPI, you need to find the MPI compilor (\textsf{mpif90}) you want to use on your machine. With that knowledge, you can build you own \textsf{arch-$<$your\_architecture$>$.fcm} file in the \textsf{LMDZ.COMMON/arch/} directory.
50You can find inspiration, for example, on the \textsf{arch-GNOMEp.fcm} (for the {\em gnome} computation server of UPMC), which uses \textsf{ifort}.
51For the LMD local computation machines (e.g. {\em levan}), you can use \textsf{arch-linux-64bit-para.fcm}.
52
53You also need to have \textsf{netcdf} and \textsf{ioipsl} compiled using the same compilor and main options. The paths to these libraries (and includes) must be written in the \textsf{arch-$<$your\_architecture$>$.path} file.
54
55An example of command line to compile the Venus GCM using \textsf{makelmdz} is then:
56
57\textsf{makelmdz -arch $<$your\_architecture$>$ -parallel mpi -d $<$nlon$>$x$<$nlat$>$x$<$nlev$>$ -p venus gcm}
58
59\section{Run}
60 
61To run the simulation, you have to use the \textsf{mpirun} launcher corresponding to your \textsf{mpif90} compilor.
62
63The command line is:
64
65\textsf{mpirun -n $<$number\_of\_procs$>$ gcm.e}
66
67\section{Outputs}
68
69Each of the processors used during the run will write its own portion of the \textsf{hist$<$mth/day/ins$>$.nc} files. To gather these portions back into one single file, there is a tool located in the ioipsl directory that you built from the SVN instructions.
70
71This tool is called \textsf{rebuild} and is found in the \textsf{ioipsl/modipsl/bin/} directory.
72
73To use it, the command line is:
74
75\textsf{rebuild -f -o $<$name\_of\_final\_file$>$.nc hist$<$mth/day/ins$>$\_*.nc}
76
77\end{document}
Note: See TracBrowser for help on using the repository browser.