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POT3D is a Fortran code that computes potential field solutions to approximate the solar coronal magnetic field using observed photospheric magnetic fields as a boundary condition. It can be used to generate potential field source surface (PFSS), potential field current sheet (PFCS), and open field (OF) models. It has been (and continues to be) used for numerous studies of coronal structure and dynamics. The code is highly parallelized using MPI and is GPU-accelerated using Fortran standard parallelism (do concurrent) and OpenACC, along with an option to use the NVIDIA cuSparse library. The HDF5 file format is used for input/output.
Presentation
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Downloading and compiling POT3D
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# MPI=openmpi-4.1.2-intel2021.4.0
MPI=intelmpi-2021.7.0
if [[ "$MPI" =~ ^intel ]]; then
module load hdf5/1.10.7-impi-intel
export I_MPI_F90=ifort
else
module load hdf5/1.10.7-ompi-intel
export OMPI_MPIF90=ifort
fi
#################################################################
# Location of local hdf5 installed with same compiler being used for POT3D:
HDF5_INCLUDE_DIR="$HDF5_ROOT/include"
HDF5_LIB_DIR="$HDF5_ROOT/lib"
# Fortran HDF5 library flags (these can be version dependent):
HDF5_LIB_FLAGS="-lhdf5_fortran -lhdf5_hl_fortran -lhdf5 -lhdf5_hl""
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Sample build script for PSC:
Download HPC-X from ISC23 SCC Getting Started with Bridges-2 Cluster.
Download and install HDF5 before building POT3D.
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source /jet/packages/intel/oneapi/compiler/2022.1.0/env/vars.sh source /jet/packages/intel/oneapi/mkl/2022.1.0/env/vars.sh # MPI=intelmpi MPI=hpcx if [[ "$MPI" =~ ^hpcx ]]; then module use $HOME/hpcx-2.13.1/modulefiles module load hpcx export OMPI_MPICC=icc export OMPI_MPICXX=icpc export OMPI_MPIFC=ifort export OMPI_MPIF90=ifort export FC=mpif90 else source /jet/packages/intel/oneapi/mpi/2021.6.0/env/vars.sh export FC=mpiifort fi ################################################################# # Location of local hdf5 installed with same compiler being used for POT3D: HDF5_INCLUDE_DIR="$HDF5_ROOT/include" HDF5_LIB_DIR="$HDF5_ROOT/lib" # Fortran HDF5 library flags (these can be version dependent): HDF5_LIB_FLAGS="-lhdf5_fortran -lhdf5_hl_fortran -lhdf5 -lhdf5_hl"" ... |
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Task and Submission
Use the run input in the POT3D package’s under
testsuite/isc2023
folder.Run POT3D with
isc2023
input on both PSC bridges-2 and FAU Fritz CPU clusters using 4 nodes.
Experiment with number of ranks per socket/numa domains to get the best results.
Your job should converge at 25112 steps and print outputs like below:Code Block ### The CG solver has converged. Iteration: 25112 Residual: 9.972489313728662E-13
Profile a run.
Use any of the remote clusters to run an MPI profile (such as IPM profile or any other profiler) for a run using 4 nodes with full PPN.
Submit the profile as a PDF to the team's folder.
In your presentation, also indicate the 3 main MPI calls that are being used and their run times, as well as the total MPI time for the test.
Bonus task: Run POT3D on the FAU Alex PSC cluster using the A100 V100 GPU partition.
Use only 4 GPUs for the run. It is recommended to use one rank per GPU.
Submit the results to the team's folder.
NOTE: To compile and run POT3D with the
nvfortran
compiler, you must load and/or build the HDF5 library compiled withnvfortran
. The code is known to work with HDF5 1.8.21 (http://portal.hdfgroup.org/display/support/HDF5+1.8.21 )An example build script for POT3D with the NVIDIA compiler can be found in
build_examples/build_gpu_nv22.3_ubuntu20.04.sh
Note that you do NOT need to enable the
cusparse
option because the test case is not set up to use the algorithm that requirescusparse
. Therefore, if linkingcusparse
is causing difficulties, you can change the build script linePOT3D_CUSPARSE=1
toPOT3D_CUSPARSE=0
.
Submission and Presentation:
- Submit all your build scripts, run scripts, inputs, and output text files (pot3d.dat, pot3d.out, timing.out, etc.)
- Do not submit the output HDF5 data or the source code.
- Prepare slides for the team’s interview based on your work for this application.
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