|
| 1 | +## SPEC complition instructions |
| 2 | + |
| 3 | +Guide for installing SPEC including the python wrappers, relies on usign cmake |
| 4 | + |
| 5 | +### Compilation |
| 6 | + |
| 7 | +Get the repository and install the necessary compilers and libraries |
| 8 | +``` |
| 9 | +git clone [email protected]:PrincetonUniversity/SPEC.git |
| 10 | +conda create -n "spec_wrapper" python=3.11 |
| 11 | +conda activate spec_wrapper |
| 12 | +conda install gcc_linux-64 gxx_linux-64 gfortran_linux-64 |
| 13 | +conda install hdf5 openblas libopenblas fftw scalapack openmpi cmake ninja |
| 14 | +conda install h5py matplotlib f90nml scipy scikit-build mpi4py ipython |
| 15 | +pip install f90wrap |
| 16 | +``` |
| 17 | + |
| 18 | +Link to the correct `f2py` |
| 19 | +``` |
| 20 | +ln -s ~/anaconda3/envs/spec_wrapper/bin/f2py ~/anaconda3/envs/spec_wrapper/bin/f2py3 |
| 21 | +``` |
| 22 | + |
| 23 | +If necessary, unset HDF5 and FFTW environmental variables |
| 24 | +``` |
| 25 | +unset HDF5, HDF5_ROOT, HDF5_HOME, FFTW, FFTW_DIR |
| 26 | +``` |
| 27 | + |
| 28 | +Finally, install SPEC and the wrapper (logs will be in `compile.log`) |
| 29 | +``` |
| 30 | +pip install -v . 2>&1 | tee compile.log |
| 31 | +``` |
| 32 | + |
| 33 | +Install the `py_spec` python library |
| 34 | +``` |
| 35 | +cd Utilities/pythontools/ |
| 36 | +pip install -e . |
| 37 | +``` |
| 38 | + |
| 39 | + |
| 40 | +### Testing your SPEC installation |
| 41 | + |
| 42 | +First, verify that the stand-alone executable is usable. |
| 43 | +A few test cases are provided in `InputFiles/TestCases`. |
| 44 | + |
| 45 | +Create a new directory for SPEC runs and change into it |
| 46 | + |
| 47 | +```bash |
| 48 | +mkdir ~/SPEC_runs |
| 49 | +cd ~/SPEC_runs |
| 50 | +``` |
| 51 | + |
| 52 | +Copy a demo input file into the current working directory: |
| 53 | + |
| 54 | +```bash |
| 55 | +cp ~/SPEC/InputFiles/TestCases/G3V01L0Fi.001.sp . |
| 56 | +``` |
| 57 | + |
| 58 | +Call SPEC with an input file (`*.sp`) as argument on the command line: |
| 59 | + |
| 60 | +```bash |
| 61 | +xspec G3V01L0Fi.001.sp |
| 62 | +``` |
| 63 | + |
| 64 | +You should see the screen output of the SPEC run. |
| 65 | +Among the last lines should be something similar to this: |
| 66 | + |
| 67 | +``` |
| 68 | +ending : 0.88 : myid= 0 ; completion ; time= 0.88s = 0.01m = 0.00h = 0.00d ; date= 2022/02/17 ; time= 17:35:33 ; ext = G1V02L0Fi.001 |
| 69 | +ending : : |
| 70 | +xspech : : |
| 71 | +xspech : 0.88 : myid= 0 : time= 0.01m = 0.00h = 0.00d ; |
| 72 | +``` |
| 73 | + |
| 74 | +This indicates that the stand-alone executable is usable. |
| 75 | + |
| 76 | +Next, the python wrapper is tested. |
| 77 | + |
| 78 | +1. Check that the SPEC version can be found: |
| 79 | + |
| 80 | + ```bash |
| 81 | + python -c "from spec import spec_f90wrapped as spec; print('SPEC version: {:}'.format(spec.constants.version))" |
| 82 | + ``` |
| 83 | + |
| 84 | + This should print a message like "SPEC version: 3.1" on the screen. |
| 85 | + |
| 86 | +2. Check that the Python wrapper can be used as a stand-alone code: |
| 87 | + |
| 88 | + ```bash |
| 89 | + OMP_NUM_THREADS=1 python ~/SPEC/Utilities/python_wrapper/spec/core.py G3V01L0Fi.001.sp |
| 90 | + ``` |
| 91 | + |
| 92 | + This should conclude with the message `SPEC called from python finished!`. |
| 93 | + |
| 94 | +3. Run the optimization example code: |
| 95 | + |
| 96 | + ```bash |
| 97 | + OMP_NUM_THREADS=1 python ~/SPEC/Utilities/python_wrapper/examples/example.py |
| 98 | + ``` |
| 99 | + |
| 100 | + This should run a basic optimization problem, |
| 101 | + where the SPEC inputs are controlled via `scipy.optimize`. |
| 102 | + |
| 103 | +4. Run the interactive re-convergence example code: |
| 104 | + |
| 105 | + ```bash |
| 106 | + OMP_NUM_THREADS=1 python ~/SPEC/Utilities/python_wrapper/examples/example_2.py |
| 107 | + ``` |
| 108 | + |
| 109 | + This should compute a SPEC equilibrium, then change the central pressure, |
| 110 | + re-converge SPEC, etc. for a set of five values of the central pressure |
| 111 | + in a two-volume classical Stellarator case. |
| 112 | + After the pressure scan with re-convergence, |
| 113 | + a plot of the MHD energy vs. the central pressure is shown. |
0 commit comments