Compile, run & validate ARPEGE with physics on NVIDIA accelerators.
This repository contains :
- a frozen version of gmkpack (in the gmkpack directory)
- configuration files for gmkpack (in the support directory)
- source code for various ancillary libraries
- scripts to compile ancillary libraries (hdf, netcdf, eccodes, lapack, eigen3, dummies for other unused libraries)
- scripts to prepare & compile packs with different compilers
- test cases at various resolutions for ARPEGE (
cy49
directory), with references - sample scripts to run the test cases (
scripts/sbatch-meteo.sh
&scripts/sbatch-ecmwf.sh
)
Compilers :
- NVHPC 23.11, 24.1, 24.3, 24.5
- Intel 18.05
- Any other C/C++/FORTRAN with MPI support
Python 3
At least 100Gb of free disk space.
Install gpupack in your HOME directory :
$ cd $HOME
$ git clone https://github.com/pmarguinaud/gpupack.git
It is possible to clone gpupack somewhere else, but in this case, you need to create a symbolic link in your HOME to point to the right location of gpupack :
cd $SCRATCH
$ git clone https://github.com/pmarguinaud/gpupack.git
$ cd $HOME
$ ln -s $SCRATCH/gpupack
gpupack accepts the following options (some of them similar to those used by gmkpack) :
- -r; $RELEASE
- -b; $BRANCH
- -l; $ARCH, architecture/compiler name
- -o; $OPT, architecture/compiler flavor
- -R; git $REPOSITORY
- -G; use ectrans GPU library
- -N; create the pack, but do not compile
- -S; do everything in a screen session
- -H; display help message and exit
gpupack will fetch a branch named ${RELEASE}_${BRANCH}
in the git $REPOSITORY given by the -R option, and create
a pack named ${RELEASE}_${BRANCH}.01.${ARCH}.${OPT}
.
cd to $HOME/gpupack
, and inspect the content of the scripts gpupack
and scripts/gpupack
:
export GPUPACK_PREFIX=$HOME/gpupack
# Cycle & a branch
export CYCLE=49t2
export BRANCH=openacc
export REPO=https://github.com/pmarguinaud/IAL.git
export ECTRANS_GPU=OFF
# Architecture flavor
export OPT=1d
# Compiler
export ARCH=NVHPC2403
...
# Load gpupack shell functions
source $GPUPACK_PREFIX/scripts/gpupack
# Create gpupack profile
create_gpupack_sh
# Load gpupack profile
source ./gpupack.sh
# Install common libraries (architecture independent)
if [ ! -d "$GPUPACK_PREFIX/install/common" ]
then
common_install
fi
# Check versions of Perl & cmake
common_check_versions
# Install architecture dependent libraries
if [ ! -d "$GPUPACK_PREFIX/install/$ARCH" ]
then
libraries_install
fi
# Create a pack
pack_create
# Compile the pack
if [ "$COMPILE" == "ON" ]
then
pack_compile
fi
Each step is detailed in the following sections. When you have understood these different steps, you will be able to combine them to automate building and testing in your own script, taking into account the constraints of your environment.
The shell function create_gpupack_sh
(from scripts/gpupack
) will create gpupack.sh. You will have to manually source this file
before working with gpupack.
These are architecture independant libraries.
-
Perl version 5.26 has a bug which affects strongly the performance of gmkpack; it is therefore required to install a more recent version. gpupack is shipped with the source code of Perl 5.38.
-
fypp (a Fortran pre-processor) is mandatory to compile ARPEGE source code. gpupack can fetch and install fypp.
-
A recent version of cmake is required to compile ARPEGE libraries. gpupack can install cmake 3.26.
-
The yaml Python module can also be installed by gpupack.
-
The utilities from the vimpack repository are required (gitpack & vimpack) and are installed by gpupack.
Please look at scripts/gpupack.common
and see how to adapt it to your environment.
Before doing that, you need to setup wrappers for your compiler suite. Please look in the support/wrap/ directory and
see if one existing architecture (let us call it ARCH) fits your needs. If so, please edit the scripts in
support/wrap/ARCH, so that these scripts can compile actual code (you will probably need to fix some paths which are
different on your system), with all library references resolved by the linker (that is, do not forget to add
-Wl,-rpath,/path/to/libraries
as needed, so that references to dynamic libraries be resolved using RPATH).
If your architecture does not exist, then try to pick something similar from what already exists, and make a copy, in a different directory. Then edit the compiler wrappers.
gpupack is shipped with the following libraries, and can install them :
- eccodes
- hdf5
- netcdf
- netcdf/fortran
- lapack
- eigen
- cutlass (only compiled when the nvhpc compiler suite is used)
It can also create dummies for these libraries (which are not required to make an ARPEGE forecast) :
- rgb
- bufr
- gribex
- fdbdummy
- wamdummy
- naglitedummy
- oasisdummy
- ibmdummy
- mpidummy
Look at scripts/gpupack.libraries
and see how to adapt it to fit your needs and your constraints.
Please look at the content of the support/arch directory. Each architecture (ARCH) might exist with different flavors (mostly compilation options or floating point precision); for example, INTEL1805 exists with two suffixes :
- 2d : -O2, double precision
- 2s : -O2, single precision
Look at the contents of INTEL1805.2d for instance. If your architecture does not exist, you need to copy INTEL1805.2d into ARCH.OPT, and adapt the contents of ARCH.OPT.
Please note that the NVIDIA target architecture has to be selected in NVHPC2401.1d and NVHPC2401.1s (GPU = cc70 or GPU = cc80).
The pack_create
function (defined in scripts/gpupack.pack
) creates a pack; this involves the following
steps :
- invoking
gmkpack
with the appropriate options - download source code, for ARPEGE and other differents components (ecbuild, eckit, oops, fiat, ectrans, field_api)
The pack will be created in pack. Its name is ${CYCLE}_${BRANCH}.01.${ARCH}.${OPT}
. It should contain the following scripts :
ics_packages
; for compiling libraries inhub/local
ics_masterodb
; for compiling ARPEGE source codeld_masterodb
; does not compile ARPEGE source code, only create ARPEGE executable
The pack_compile
function (defined in scripts/gpupack.pack
) compiles the pack. This involves :
- compiling the packages (ecbuild, eckit, ...) with
ics_packages
- compiling the ARPEGE source code with
ics_masterodb
If the compilation is successful, then unnecessary files may be removed (directory hub/local/build
), but also
with lockpack
in src/local
.
It is possible to invoke ics_packages
and ics_masterodb
manually from
within the pack. Please note that by default ics_packages
and ics_masterodb
will run with 16 threads, but it is possible to change the value by editing
GMK_THREADS in those files.
If the compilation is successful, then the bin/MASTERODB
file will exist and be executable.
Please note that compiling the code on ECMWF cluster is not possible on login nodes, because of cgroups limitations; it
is necessary to turn ics_masterodb
into a batch job and submit it in the par
queue.
A script and different initial condition files are provided in the cy49
directory; we provide different resolutions : t0031l15, t0107l70, t0538l60, t0798l90.
The t0031l15 runs in about 20s on an dual socket AMD Rome node. The t0798l90 requires at least three dual socket AMD nodes; it has also been tested on three dual socket AMD nodes, each equipped with 4 NVIDIA V100 cards.
Please look at the script cy49/arp/arp.sh
and see how you can adapt it to your environment. The following scripts :
scripts/sbatch-ecmwf.sh
scripts/sbatch-meteo.sh
provides examples of how cy49/arp/arp.sh
is submitted to ECMWF & Meteo-France batch systems.
These matrix multiplications occur in the following routines :
verint.F90
verints.F90
verder.F90
We normally use DGEMM (from the MKL library) in these routines, but we cannot use DGEMM on accelerators, we coded some simple multiplications that we enable with the LLSIMPLE_DGEMM library.
The script cy49/arp/arp.sh
run the code in four different modes :
- nominal : ARPEGE physics is managed by a very large OpenMP section; this is the optimal mode on traditionnal CPUs.
- openmp : ARPEGE physics is managed by a succession of small OpenMP sections
- openmpsinglecolumn : ARPEGE physics is managed by a succession of small OpenMP sections, without vectorisation with column processed independently. This is meant for validation.
- openaccsinglecolumn : ARPEGE physics is managed by a succession of small OpenACC sections (with possibly a few OpenMP section in between). This is supposed to be the optimal mode on GPUs.
Some comparison are made when references are available (in cy49/arp/*/ref
directories). We also make the following
comparisons :
- nominal - openmp
- nominal - openmpsinglecolumn
- nominal - openaccsinglecolumn
- openmpsinglecolumn - openaccsinglecolumn
We consider that these comparison should lead to identical results in the following cases :
- INTEL with vectorisation :
+---------------------+----------+---------+---------------------+-----------------------+
| | nominal | openmp | openmpsinglecolumn | openaccsinglecolumn |
+---------------------+----------+---------+---------------------+-----------------------+
| nominal | = | = | | |
+---------------------+----------+---------+---------------------+-----------------------+
| openmp | = | = | | |
+---------------------+----------+---------+---------------------+-----------------------+
| openmpsinglecolumn | | | = | = |
+---------------------+----------+---------+---------------------+-----------------------+
| openaccsinglecolumn | | | = | = |
+---------------------+----------+---------+---------------------+-----------------------+
- NVHPC without vectorisation :
+---------------------+----------+---------+---------------------+-----------------------+
| | nominal | openmp | openmpsinglecolumn | openaccsinglecolumn |
+---------------------+----------+---------+---------------------+-----------------------+
| nominal | = | = | = | |
+---------------------+----------+---------+---------------------+-----------------------+
| openmp | = | = | = | |
+---------------------+----------+---------+---------------------+-----------------------+
| openmpsinglecolumn | = | = | = | |
+---------------------+----------+---------+---------------------+-----------------------+
| openaccsinglecolumn | | | | = |
+---------------------+----------+---------+---------------------+-----------------------+