ESPEI¶
Installation¶
Anaconda (recommended)¶
ESPEI does not require any special compiler, but several dependencies do. Therefore it is suggested to install ESPEI from conda-forge.
conda install -c pycalphad -c msys2 -c conda-forge --yes espei
After installation, you must turn off dask’s work stealing.
Change the work stealing setting to distributed.scheduler.work-stealing: False
in ~/.config/dask/distributed.yaml
.
See configuration below for more details.
PyPI¶
Before you install ESPEI via PyPI, be aware that pycalphad and emcee must be compiled and pycalphad requires an external dependency of Ipopt.
pip install espei
After installation, you must turn off dask’s work stealing.
Change the work stealing setting to distributed.scheduler.work-stealing: False
in ~/.config/dask/distributed.yaml
.
See configuration below for more details.
Development versions¶
You may install ESPEI however you like, but here we suggest using Anaconda to download all of the required dependencies. This method installs ESPEI with Anaconda, removes specifically the ESPEI package, and replaces it with the package from GitHub.
git clone https://github.com/phasesresearchlab/espei.git
cd espei
conda install espei
conda remove --force espei
pip install -e .
Upgrading ESPEI later requires you to run git pull
in this directory.
After installation, you must turn off dask’s work stealing.
Change the work stealing setting to distributed.scheduler.work-stealing: False
in ~/.config/dask/distributed.yaml
.
See configuration below for more details.
Configuration¶
ESPEI uses dask-distributed to parallelize ESPEI.
After installation, you must turn off dask’s work stealing!
Change the file at ~/.config/dask/distributed.yaml
to look something like:
distributed:
version: 2
scheduler:
work-stealing: False
See the dask-distributed documentation for more.
Quickstart¶
ESPEI has two different fitting modes: single-phase and multi-phase fitting. You can run either of these modes or both of them sequentially.
To run either of the modes, you need to have a phase models file that describes the phases in the system using the standard CALPHAD approach within the compound energy formalism.
You also need to describe the data that ESPEI should fit to.
You will need single-phase and multi-phase data for a full run.
Fit settings and all datasets are stored as JSON files and described in detail at the Making ESPEI datasets page.
All of your input datasets should be validated by running espei --check-datasets my-input-datasets
, where my-input-datasets
is a folder of all your JSON files.
The main output result is going to be a database (defaults to out.tdb
), an array of the steps in the MCMC trace (defaults to trace.npy
), and the an array of the log-probabilities for each iteration and chain (defaults to lnprob.npy
).
Single-phase only¶
If you have only heat capacity, entropy and enthalpy data and mixing data (e.g. from first-principles), you may want to see the starting point for your MCMC calculation.
Create an input file called espei-in.yaml
.
system:
phase_models: my-phases.json
datasets: my-input-datasets
generate_parameters:
excess_model: linear
ref_state: SGTE91
Then ESPEI can be run by running
espei --input espei-in.yaml
Multi-phase only¶
If you have a database already and just want to do a multi-phase fitting, you can specify a starting TDB file (named my-tdb.tdb
) with
system:
phase_models: my-phases.json
datasets: my-input-data
mcmc:
iterations: 1000
input_db: my-tdb.tdb
The TDB file you input must have all of the degrees of freedom you want as FUNCTIONs with names beginning with VV
.
Restart from previous run-phase only¶
If you’ve run an MCMC fitting already in ESPEI and have a trace file called my-previous-trace.npy
, then you can resume the calculation with the following input file
system:
phase_models: my-phases.json
datasets: my-input-data
mcmc:
iterations: 1000
input_db: my-tdb.tdb
restart_trace: my-previous-trace.npy
Full run¶
A minimal full run of ESPEI with single phase fitting and MCMC fitting is done by the following
system:
phase_models: my-phases.json
datasets: my-input-data
generate_parameters:
excess_model: linear
ref_state: SGTE91
mcmc:
mcmc_steps: 1000
Input Customization¶
ESPEI lets you control many aspects of your calculations with the input files shown above. See ESPEI YAML input files for a full description of all possible inputs.
FAQ¶
Q: There is an error in my JSON files¶
A: Common mistakes are using single quotes instead of the double quotes required by JSON files. Another common source of errors is misaligned open/closing brackets.
Many mistakes are found with ESPEI’s check-datasets
utility.
Run espei check-datasets my-input-datasets
on your directory my-input-datasets
.
Q: How do I analyze my results?¶
A: By default, ESPEI will create trace.npy
and lnprob.npy
for the MCMC chain at the specified save interval and according to the save interval (defaults to ever iteration).
These are created from arrays via numpy.save()
and can thus be loaded with numpy.load()
.
Note that the arrays are preallocated with zeros.
These filenames and settings can be changed using in the input file.
You can then use these chains and corresponding log-probabilities to make corner plots, calculate autocorrelations, find optimal parameters for databases, etc..
Finally, you can use py:mod:espei.plot functions such as multiplot
to plot phase diagrams with your input equilibria data and plot_parameters
to compare single-phase data (e.g. formation and mixing data) with the properties calculated with your database.
Q: Can I run ESPEI on a supercomputer supporting MPI?¶
A: Yes! ESPEI has MPI support. See the Advanced Schedulers page for more details.
ESPEI, or Extensible Self-optimizing Phase Equilibria Infrastructure, is a tool for automated thermodynamic database development within the CALPHAD method. It uses pycalphad for calculating Gibbs free energies of thermodynamic models.

Cu-Mg phase diagram from a database created with and optimized by ESPEI. See the Cu-Mg Example.
Goals¶
- Offer a free and open-source tool for users to develop multicomponent databases with quantified uncertainty
- Enable development of CALPHAD-type models for Gibbs energy, thermodynamic or kinetic properties
- Provide a platform to build and apply novel model selection and optimization methods
The implementation for ESPEI involves first fitting single-phase data by calculating parameters in thermodynamic models that are linearly described by the single-phase input data. Then Markov Chain Monte Carlo (MCMC) is used to optimize the candidate models from the single-phase fitting to multi-phase zero-phase fraction data. The benefit of this approach is the automated, simultaneous fitting for many parameters that yields uncertainty quantification, as shown in Otis and Liu High-Throughput Thermodynamic Modeling and Uncertainty Quantification for ICME. Jom 69, (2017). Single-phase and multi-phase fitting methods are described in Chapter 3 of Richard Otis’s thesis.
History¶
The ESPEI package is based on a fork of pycalphad-fitting. The name and idea of ESPEI are originally based off of Shang, Wang, and Liu, ESPEI: Extensible, Self-optimizing Phase Equilibrium Infrastructure for Magnesium Alloys Magnes. Technol. 2010 617-622 (2010).
Change log¶
What’s New¶
0.6.2 (2018-11-27)¶
This backwards-compatible release includes several bug fixes and improvements.
- Updated branding to include the new ESPEI logo. See the logo in the
docs/_static
directory. - Add support for fitting excess heat capacity.
- Bug fix for broken potassium unary.
- Documentation improvements for recipes
- pycalphad 0.7.1 fixes for dask, sympy, and gmpy2 should mean that ESPEI should not require package upgrade or downgrades. Please report any installations issues in ESPEI’s Gitter Channel <https://gitter.im/PhasesResearchLab/ESPEI>.
- [Developers] ESPEI’s
eq_callables_dict
is nowpycalphad.codegen.callables.build_callables
. - [Developers] matplotlib plotting tests are removed because nose is no longer supported.
0.6.1 (2018-08-28)¶
This a major release with several important features and bug fixes.
- Enable use of ridge regression alpha for parameter selection via the
parameter_generation.ridge_alpha
input parameter. - Add ternary parameter selection. Works by default, just add data.
- Set memory limit to zero to avoid dask killing workers near the dask memory limits.
- Remove ideal mixing from plotting models so that
plot_parameters
gives the correct entropy values. - Add recipes documentation <https://github.com/PhasesResearchLab/ESPEI/blob/master/docs/recipes.rst> that contains some Python code for common utility operations.
- Add documentation for running custom distributed schedulers in ESPEI
0.6 (2018-07-02)¶
This is a update including breaking changes to the input files and several minor improvements.
- Update input file schema and Python API to be more consistent so that the
trace
always refers to the collection of chains andchain
refers to individual chains. Additionally removed some redundancy in the parameters nested under themcmc
heading, e.g.mcmc_steps
is nowiterations
andmcmc_save_interval
is nowsave_interval
in the input file and Python API. See Writing Input documentation for all of the updates. - The default save interval is now 1, which is more reasonable for most MCMC systems with significant numbers of phase equilibria.
- Bug fixes for plotting and some better plotting defaults for plotting input data
- Dataset parsing and cleaning improvements.
- Documentation improvements (see the PDF!)
0.5.2 (2018-04-28)¶
This is a major bugfix release for MCMC multi-phase fitting runs for single phase data.
- Fixed a major issue where single phase thermochemical data was always compared to Gibbs energy, giving incorrect errors in MCMC runs.
- Single phase errors in ESPEI incorrectly compared values with ideal mixing contributions to data, which is excess only.
- Fixed a bug where single phase thermochemical data with that are dependent on composition and pressure and/or temperature were not fit correctly.
- Added utilities for analyzing ESPEI results and add them to the Cu-Mg example docs.
0.5.1 (2018-04-17)¶
This is a minor bugfix release.
- Parameter generation for phases with vacancies would produce incorrect parameters because the vacancy site fractions were not being correctly removed from the contributions due to their treatement as
Species
objects inpycalphad >=0.7
.
0.5 (2018-04-03)¶
- Parameter selection now uses the corrected AIC, which further prevents overparameterization where there is sparse training data.
- Activity and single phase thermochemical data can now be included in MCMC fitting runs. Including single phase data can help anchor metastable phases to DFT data when they are not on the stable phase diagram. See the Gathering input data documentation for information on how to input activity data.
- Dataset checking has been improved. Now there are checks to make sure sublattice interactions are properly sorted and mole fractions sum to less than 1.0 in ZPF data.
- Support for fitting phases with arbitrary pycalphad Models in MCMC, including (charged and neutral) species and ionic liquids. There are several consequences of this:
- ESPEI requires support on
pycalphad >=0.7
- ESPEI now uses pycalphad
Model
objects directly. Using the JIT compiled Models has shown up to a 50% performance improvement in MCMC runs. - Using JIT compiled
Model
objects required the use ofcloudpickle
everywhere. Due to challenges in overridingpickle
for upstream packages, we now rely solely ondask
for scheduler tasks, includingmpi
viadask-mpi
. Note that users must turn offwork-stealing
in their~/.dask/config.yaml
file.
- ESPEI requires support on
- [Developers] Each method for calculating error in MCMC has been moved into a module for that method in an
error_functions
subpackage. One top level function from each module should be imported into themcmc.py
and used inlnprob
. Developers should then just customizelnprob
. - [Developers] Significant internal docs improvements: all non-trival functions have complete docstrings.
0.4.1 (2018-02-05)¶
- Enable plotting of isothermal sections with data using
dataplot
(andmultiplot
, etc.) - Tielines are now plotted in
dataplot
for isothermal sections and T-x phase diagrams - Add a useful
ravel_conditions
method to unpack conditions from datasets
0.4 (2017-12-29)¶
- MCMC is now deterministic by default (can be toggled off with the
mcmc.deterministic
setting). - Added support for having no scheduler (running with no parallelism) with the
mcmc.scheduler
option set toNone
. This may be useful for debugging. - Logging improvements
- Extraneous warnings that may be confusing for users and dirty the log are silenced.
- A warning is added for when there are no datasets found.
- Fixed a bug where logging was silenced with the dask scheduler
- Add
optimal_parameters
utility function as a helper to get optimal parameter sets for analysis - Several improvements to plotting
- Users can now plot phase diagram data alone with
dataplot
, useful for checking datasets visually. This changes the API fordataplot
to no longer infer the conditions from an equilibriumDataset
(from pycalphad). That functionality is preserved ineqdataplot
. - Experimental data points are now plotted with unique symbols depending on the reference key in the dataset. This is for both phase diagram and single phase parameter plots.
- Options to control plotting parameters (e.g. symbol size) and take user supplied Axes and Figures in the plotting functions. The symbol size is now smaller by default.
- Users can now plot phase diagram data alone with
- Documentation improvements for API and separation of theory from the Cu-Mg example
- Fixes a bug where elements with single character names would not find the correct reference state (which are typically named GHSERCC for the example of C).
- [Developer] All MCMC code is moved from the
paramselect
module to themcmc
module to separate these tasks - [Developer] Support for arbitrary user reference states (so long as the reference state is in the
refdata
module and follows the same format as SGTE91)
0.3.1.post2 (2017-10-31)¶
- Propogate the new entry point to setup.py
0.3.1.post1 (2017-10-31)¶
- Fix for module name/function conflict in entry point
0.3.1 (2017-10-31)¶
- ESPEI is much easier to run interactively in Python and in Jupyter Notebooks
- Reference data is now included in ESPEI instead of in pycalphad
- Several reference data fixes including support for single character elements (‘V’, ‘B’, ‘C’, …)
- Support for using multiprocessing to parallelize MCMC runs, used by default (@olivia-higgins)
- Improved documentation for installing and developing ESPEI
0.3.post2 (2017-09-20)¶
- Add input-schema.yaml file to installer
0.3.post1 (2017-09-20)¶
- Add LICENSE to manifest
0.3 (2017-09-20)¶
- ESPEI input is now described by a file. This change is breaking. Old command line arguments are not supported. See Writing input files for a full description of all the inputs.
- New input options are supported, including modifying the number of chains and standard deviation from the mean
- ESPEI is now available on conda-forge
- TinyDB 2 support is dropped in favor of TinyDB 3 for conda-forge deployment
- Allow for restarting previous mcmc calculations with a trace file
- Add Cu-Mg example to documentation
0.2.1 (2017-08-17)¶
Fixes to the 0.2 release plotting interface
multiplot
is renamed frommulti_plot
, as in docs.- Fixed an issue where phases in datasets, but not in equilibrium were not plotted by dataplot and raised an error.
0.2 (2017-08-15)¶
New
multiplot
interface for convienent plotting of phase diagrams + data.dataplot
function underlies key data plotting features and can be used witheqplot
. See their API docs for examples. Will break existing code using multiplot.MPI support for local/HPC runs. Only single node runs are explictly supported currently. Use
--scheduler='MPIPool'
command line option. Requiresmpi4py
.Default debug reporting of acceptance ratios
Option (and default) to output the log probability array matching the trace. Use
--probfile
option to control.Optimal parameters are now chosen based on lowest error in chain.
Bug fixes including
- py2/3 compatibiltiy
- unicode datasets
- handling of singular matrix errors from pycalphad’s
equilibrium
- reporting of failed conditions
0.1.5 (2017-08-02)¶
- Significant error checking of JSON inputs.
- Add new
--check-datasets
option to check the datasets at path. It should be run before you run ESPEI fittings. All errors must be resolved before you run. - Move the espei script module from
fit.py
torun_espei.py
. - Better docs building with mocking
- Google docstrings are now NumPy docstrings
0.1.4 (2017-07-24)¶
- Documentation improvements for usage and API docs
- Fail fast on JSON errors
0.1.3 (2017-06-23)¶
- Fix bad version pinning in setup.py
- Explicitly support Python 2.7
0.1.2 (2017-06-23)¶
- Fix dask incompatibilty due to new API usage
0.1.1 (2017-06-23)¶
- Fix a bug that caused logging to raise if bokeh isn’t installed
0.1 (2017-06-23)¶
ESPEI is now a package! New features include
- Fork https://github.com/richardotis/pycalphad-fitting
- Use emcee for MCMC fitting rather than pymc
- Support single-phase only fitting
- More control options for running ESPEI from the command line
- Better support for incremental saving of the chain
- Control over output with logging over printing
- Significant code cleanup
- Better usage documentation
See what’s new!
Cu-Mg Example¶
The Cu-Mg binary system is an interesting and simple binary subsystem for light metal alloys. It has been modeled in the literature by Coughanowr et al. [1], Zuo and Chang [2] and Zhou et al. [3] and was featured as a case study in Computational Thermodynamics The Calphad Method by Lukas, Fries, & Sundman [4].
Here we will combine density functional theory and experimental calculations of single-phase data to generate a first-principles phase diagram. Then that database will be used as a starting point for a Markov Chain Monte Carlo (MCMC) Bayesian optimization of the parameters to fit zero-phase fraction data.
Input data¶
All of the input data for ESPEI is stored in a public ESPEI-datasets repository on GitHub. The data in this repository is Creative Commons Attribution 4.0 (CC-BY-4.0) licensed and may be used, commercialized or reused freely.
In order to run ESPEI with the data in ESPEI-datasets, you should clone this repository to your computer. Files referred to throughout this tutorial are found in the CU-MG folder. The input files will be very breifly explained in this tutorial so that you are able to know their use. A more detailed description of the files is found on the Making ESPEI datasets page.
If you make changes or additions, you are encouraged to share these back to the ESPEI-datasets repository so that others may benefit from this data as you have. You may then add your name to the CONTRIBUTORS file as described in the README.
Phases and CALPHAD models¶
The Cu-Mg system contains five stable phases: Liquid, disordered fcc and hcp, the C15 Laves phase and the CuMg2 phase. All of these phases will be modeled as solution phases, except for CuMg2, which will be represented as a stoichiometric compound. The phase names and corresponding sublattice models are as follows:
LIQUID: (CU, MG)1
FCC_A1: (CU, MG)1 (VA)1
HCP_A3: (CU, MG)1 (VA)1
LAVES_C15: (CU, MG)2 (CU, MG)1
CUMG2: (CU)1 (MG)2
These phase names and sublattice models are described in the JSON file Cu-Mg-input.json file as seen below
{
"components": ["CU", "MG", "VA"],
"phases": {
"LIQUID" : {
"sublattice_model": [["CU", "MG"]],
"sublattice_site_ratios": [1]
},
"CUMG2": {
"sublattice_model": [["CU"], ["MG"]],
"sublattice_site_ratios": [1, 2]
},
"FCC_A1": {
"sublattice_model": [["CU", "MG"], ["VA"]],
"sublattice_site_ratios": [1, 1]
},
"HCP_A3": {
"sublattice_site_ratios": [1, 0.5],
"sublattice_model": [["CU", "MG"], ["VA"]]
},
"LAVES_C15": {
"sublattice_site_ratios": [2, 1],
"sublattice_model": [["CU", "MG"], ["CU", "MG"]]
}
}
}
ESPEI¶
ESPEI has two types of fitting – parameter generation and MCMC optimization. The parameter generation step uses experimental and first-principles data of the derivatives of the Gibbs free energy to parameterize the Gibbs energies of each individual phase. The MCMC optimization step fits the generated parameters to experimental phase equilibria data. These two fitting procedures can be used together to fully assess a given system. For clarity, we will preform these steps separately to fit Cu-Mg. The next two sections are devoted to describing ESPEI’s parameter generation and optimization.
Though it should be no problem for this case, since the data has already been
used, you should get in the habit of checking datasets before running ESPEI.
ESPEI has a tool to help find and report problems in your datasets. This is
automatically run when you load the datasets, but will fail on the first error.
Running the following commmand (assuming from here on that you are in the
CU-MG
folder from ESPEI-datasets):
espei --check-datasets input-data
The benefit of the this approach is that all of the datasets will be checked and
reported at once. If there are any failures, a list of them will be reported
with the two main types of errors being JSONError
, for which you should read
the JSON section of Making ESPEI datasets, or DatasetError
, which are related to
the validity of your datasets scientifically (maching conditions and values
shape, etc.). The DatasetError
messages are designed to be clear, so please
open an issue on GitHub
if there is any confusion.
First-principles phase diagram¶
By using the Cu-Mg-input.json
phase description for the fit settings and
passing all of the input data in the input-data
folder, we can first use
ESPEI to generate a phase diagram based on single-phase experimental and DFT
data. Currently all of the input datasets must be formation properties, and it
can be seen that the formation enthalpies are defined from DFT and experiments
for the Laves and CuMg2 phases. Mixing enthalpies are defined for the for the
fcc, hcp, and Laves phases from DFT and for liquid from experimental
measurements.
The following command will generate a database named cu-mg_dft.tdb
with
parameters selected and fit by ESPEI:
espei --input espei-in.yaml
where espei-in.yaml
is a ESPEI input file with
the following contents
system:
phase_models: Cu-Mg-input.json
datasets: input-data
generate_parameters:
excess_model: linear
ref_state: SGTE91
output:
output_db: cu-mg_dft.tdb
The calculation should be relatively quick, on the order of a minute of runtime.
With the above command, only mininmal output (warnings) will be reported. You
can increase the verbosity to report info messages by setting the
output.verbosity
key to 1
or debug messages with 2
.
With the following code, we can look at the generated phase diagram and compare it to our data.
# First-principles phase diagram
from pycalphad import Database, variables as v
from espei.datasets import load_datasets, recursive_glob
from espei.plot import multiplot
import matplotlib.pyplot as plt
# load the experimental and DFT datasets
datasets = load_datasets(recursive_glob('input-data', '*.json'))
# set up the pycalphad phase diagram calculation
dbf = Database('cu-mg_dft.tdb')
comps = ['CU', 'MG', 'VA']
phases = ['LIQUID', 'FCC_A1', 'HCP_A3', 'CUMG2', 'LAVES_C15']
conds = {v.P: 101325, v.T: (300, 1500, 10), v.X('MG'): (0, 1, 0.01)}
# plot the phase diagram and data
multiplot(dbf, comps, phases, conds, datasets)
plt.savefig('cu-mg_dft_phase_diagram.png')
Which should result in the following figure
We can see that the phase diagram is already very reasonable compared to the experimental points. The liquidus temperatures and the solubilities of the fcc and Laves phases are the key differences between the equilibrium data and our first-principles phase diagram. The next section will discuss using ESPEI to optimize the parameters selected and calculated based on the single-phase data to these multi-phase equilibria.
MCMC optimization¶
With the data in the CU-MG input data, ESPEI generated 18 parameters to fit. For systems with more components, solution phases, and input data, may more parameters could be required to describe the thermodynamics of the specific system well. Because they describe Gibbs free energies, parameters in CALPHAD models are highly correlated in both single-phase descriptions and for describing equilibria between phases. For large systems, global numerical optimization of many parameters simultaneously is computationally intractable.
To combat the problem of optimizing many paramters, ESPEI uses MCMC, a stochastic optimzation method. For more details on how MCMC is used in ESPEI, see the Theory page.
Now we will use our zero phase fraction equilibria data to optimize our
first-principles database with MCMC. The following command will take the
database we created in the single-phase parameter selection and perform a MCMC
optimization, creating a cu-mg_mcmc.tdb
:
espei --input espei-in.yaml
where espei-in.yaml
is an ESPEI input file with
the following structure
system:
phase_models: Cu-Mg-input.json
datasets: input-data
mcmc:
iterations: 1000
input_db: cu-mg_dft.tdb
output:
output_db: cu-mg_mcmc.tdb
ESPEI defaults to run 1000 iterations and depends on calculating equilibrium in pycalphad several times for each iteration and the optimization is compute-bound. Fortunately, MCMC optimzations are embarrasingly parallel and ESPEI allows for parallelization using dask or with MPI using mpi4py (single-node only at the time of writing - we are working on it).
Note that you may also see messages about convergence failures or about droppping conditions. These refer to failures to calculate the log-probability or in the pycalphad solver’s equilibrium calculation. They are not detrimental to the optimization accuracy, but overall optimization may be slower because those parameter proposals will never be accepted (they return a log-probability of \(-\infty\)).
Finally, we can use the newly optimized database to plot the phase diagram
# Optimized phase diagram from ESPEI's multi-phase fitting
from pycalphad import Database, variables as v
from espei.datasets import load_datasets, recursive_glob
from espei.plot import multiplot
import matplotlib.pyplot as plt
# load the experimental and DFT datasets
datasets = load_datasets(recursive_glob('input-data', '*.json'))
# set up the pycalphad phase diagram calculation
dbf = Database('cu-mg_mcmc.tdb')
comps = ['CU', 'MG', 'VA']
phases = ['LIQUID', 'FCC_A1', 'HCP_A3', 'CUMG2', 'LAVES_C15']
conds = {v.P: 101325, v.T: (300, 1500, 10), v.X('MG'): (0, 1, 0.01)}
# plot the phase diagram and data
multiplot(dbf, comps, phases, conds, datasets)
plt.savefig('cu-mg_mcmc_phase_diagram.png')
Analyzing ESPEI Results¶
After finishing a MCMC run, you will want to analyze your results.
All of the MCMC results will be maintained in two output files, which
are serialized NumPy arrays. The file names are set in your
espei-in.yaml
file. The filenames are set by output.tracefile
and output.probfile
(documentation)
and the defaults are trace.npy
and lnprob.npy
, respectively.
The tracefile
contains all of the parameters that were proposed over
all chains and iterations (the trace). The probfile
contains all of
calculated log probabilities for all chains and iterations (as negative
numbers, by convention).
There are several aspects of your data that you may wish to analyze. The next sections will explore some of the options.
Probability convergence¶
First we’ll plot how the probability changes for all of the chains as a function of iterations. This gives a qualitative view of convergence. There are several quantitative metrics that we won’t explore here, such as autocorrelation. Qualitatively, this run does not appear converged after 115 iterations.
# remove next line if not using iPython or Juypter Notebooks
%matplotlib inline
import matplotlib.pyplot as plt
import numpy as np
from espei.analysis import truncate_arrays
trace = np.load('trace.npy')
lnprob = np.load('lnprob.npy')
trace, lnprob = truncate_arrays(trace, lnprob)
ax = plt.gca()
ax.set_yscale('log')
ax.set_ylim(1e7, 1e10)
ax.set_xlabel('Iterations')
ax.set_ylabel('- lnprob')
num_chains = lnprob.shape[0]
for i in range(num_chains):
ax.plot(-lnprob[i,:])
plt.show()

Visualizing the trace of each parameter¶
We would like to see how each parameter changed during the iterations. For brevity in the number of plots we’ll plot all the chains for each parameter on the same plot. Here we are looking to see how the parameters explore the space and converge to a solution.
# remove next line if not using iPython or Juypter Notebooks
%matplotlib inline
import matplotlib.pyplot as plt
import numpy as np
from espei.analysis import truncate_arrays
trace = np.load('trace.npy')
lnprob = np.load('lnprob.npy')
trace, lnprob = truncate_arrays(trace, lnprob)
num_chains = trace.shape[0]
num_parameters = 3 # only plot the first three parameter, for all of them use `trace.shape[2]`
for parameter in range(num_parameters):
ax = plt.figure().gca()
ax.set_xlabel('Iterations')
ax.set_ylabel('Parameter value')
for chain in range(num_chains):
ax.plot(trace[chain, :, parameter])
plt.show()



Corner plots¶
Note: You must install the corner
package before using it
(conda install corner
or pip install corner
).
In a corner plot, the distributions for each parameter are plotted along the diagonal and covariances between them under the diagonal. A more circular covariance means that parameters are not correlated to each other, while elongated shapes indicate that the two parameters are correlated. Strongly correlated parameters are expected for some parameters in CALPHAD models within phases or for phases in equilibrium, because increasing one parameter while decreasing another would give a similar error.
# remove next line if not using iPython or Juypter Notebooks
%matplotlib inline
import matplotlib.pyplot as plt
import numpy as np
import corner
from espei.analysis import truncate_arrays
trace = np.load('trace.npy')
lnprob = np.load('lnprob.npy')
trace, lnprob = truncate_arrays(trace, lnprob)
# flatten the along the first dimension containing all the chains in parallel
fig = corner.corner(trace.reshape(-1, trace.shape[-1]))
plt.show()

Ultimately, there are many features to explore and we have only covered a few basics. Since all of the results are stored as arrays, you are free to analyze using whatever methods are relevant.
Summary¶
ESPEI allows thermodynamic databases to be easily reoptimized with little user interaction, so more data can be added later and the database reoptimized at the cost of only computer time. In fact, the existing database from estimates can be used as a starting point, rather than one directly from first-principles, and the database can simply be modified to match any new data.
References¶
[1] | Coughanowr, C. A., Ansara, I., Luoma, R., Hamalainen, M. & Lukas, H. L. Assessment of the Cu-Mg system. Zeitschrift f{ü}r Met. 82, 574–581 (1991). |
[2] | Zuo, Y. U. E. & Chang, Y. A. Thermodynamic calculation of the Mg-Cu phase diagram. Zeitschrift f{ü}r Met. 84, 662–667 (1993). |
[3] | Zhou, S. et al. Modeling of Thermodynamic Properties and Phase Equilibria for the Cu-Mg Binary System. J. Phase Equilibria Diffus. 28, 158–166 (2007). doi:10.1007/s11669-007-9022-0 |
[4] | Lukas, H., Fries, S. G. & Sundman, B. Computational Thermodynamics The Calphad Method. (Cambridge University Press, 2007). doi:10.1017/CBO9780511804137 |
Acknowledgements¶
Credit for initially preparing the datasets goes to Aleksei Egorov.
Making ESPEI datasets¶
JSON Format¶
ESPEI has a single input style in JSON format that is used for all data entry. Single-phase and multi-phase input files are almost identical, but detailed descriptions and key differences can be found in the following sections. For those unfamiliar with JSON, it is fairly similar to Python dictionaries with some rigid requirements
- All string quotes must be double quotes. Use
"key"
instead of'key'
.- Numbers should not have leading zeros.
00.123
should be0.123
and012.34
must be12.34
.- Lists and nested key-value pairs cannot have trailing commas.
{"nums": [1,2,3,],}
is invalid and should be{"nums": [1,2,3]}
.
These errors can be challenging to track down, particularly if you are only reading the JSON error messages in Python. A visual editor is encouraged for debugging JSON files such as JSONLint. A quick reference to the format can be found at Learn JSON in Y minutes.
ESPEI has support for checking all of your input datasets for errors, which you should always use before you attempt to run ESPEI.
This error checking will report all of the errors at once and all errors should be fixed.
Errors in the datasets will prevent fitting.
To check the datasets at path my-input-data/
you can run espei --check-datasets my-input-data
.
Phase Descriptions¶
The JSON file for describing CALPHAD phases is conceptually similar to a setup file in Thermo-Calc’s PARROT module.
At the top of the file there is the refdata
key that describes which reference state you would like to choose.
Currently the reference states are strings referring to dictionaries in pycalphad.refdata
only "SGTE91"
is implemented.
Each phase is described with the phase name as they key in the dictionary of phases.
The details of that phase is a dictionary of values for that key.
There are 4 possible entries to describe a phase: sublattice_model
, sublattice_site_ratios
, equivalent_sublattices
, and aliases
.
sublattice_model
is a list of lists, where each internal list contains all of the components in that sublattice.
The BCC_B2
sublattice model is [["AL", "NI", "VA"], ["AL", "NI", "VA"], ["VA"]]
, thus there are three sublattices where the first two have Al, Ni, and vacancies.
sublattice_site_ratios
should be of the same length as the sublattice model (e.g. 3 for BCC_B2
).
The sublattice site ratios can be fractional or integers and do not have to sum to unity.
The optional equivalent_sublattices
key is a list of lists that describe which sublattices are symmetrically equivalent.
Each sub-list in equivalent_sublattices
describes the indices (zero-indexed) of sublattices that are equivalent.
For BCC_B2
the equivalent sublattices are [[0, 1]]
, meaning that the sublattice at index 0 and index 1 are equivalent.
There can be multiple different sets (multiple sub-lists) of equivalent sublattices and there can be many equivalent sublattices within a sublattice (see FCC_L12
).
If no equivalent_sublattice
key exists, it is assumed that there are none.a
Finally, the aliases
key is used to refer to other phases that this sublattice model can describe when symmetry is accounted for.
Aliases are used here to describe the BCC_A2
and FCC_A1
, which are the disordered phases of BCC_B2
and FCC_L12
, respectively.
Notice that the aliased phases are not otherwise described in the input file.
Multiple phases can exist with aliases to the same phase, e.g. FCC_L12
and FCC_L10
can both have FCC_A1
as an alias.
{
"refdata": "SGTE91",
"components": ["AL", "NI", "VA"],
"phases": {
"LIQUID" : {
"sublattice_model": [["AL", "NI"]],
"sublattice_site_ratios": [1]
},
"BCC_B2": {
"aliases": ["BCC_A2"],
"sublattice_model": [["AL", "NI", "VA"], ["AL", "NI", "VA"], ["VA"]],
"sublattice_site_ratios": [0.5, 0.5, 1],
"equivalent_sublattices": [[0, 1]]
},
"FCC_L12": {
"aliases": ["FCC_A1"],
"sublattice_model": [["AL", "NI"], ["AL", "NI"], ["AL", "NI"], ["AL", "NI"], ["VA"]],
"sublattice_site_ratios": [0.25, 0.25, 0.25, 0.25, 1],
"equivalent_sublattices": [[0, 1, 2, 3]]
},
"AL3NI1": {
"sublattice_site_ratios": [0.75, 0.25],
"sublattice_model": [["AL"], ["NI"]]
},
"AL3NI2": {
"sublattice_site_ratios": [3, 2, 1],
"sublattice_model": [["AL"], ["AL", "NI"], ["NI", "VA"]]
},
"AL3NI5": {
"sublattice_site_ratios": [0.375, 0.625],
"sublattice_model": [["AL"], ["NI"]]
}
}
}
Units¶
- Energies are in
J/mol-atom
(and the derivatives follow) - All compositions are mole fractions
- Temperatures are in Kelvin
- Pressures in Pascal
Single-phase Data¶
Two example of ESPEI input file for single-phase data follow. The first dataset has some data for the formation heat capacity for BCC_B2.
The components
and phases
keys simply describe those found in this entry.
Use the reference
key for bookkeeping the source of the data.
In solver
the sublattice configuration and site ratios are described for the phase.
sublattice_configurations
is a list of different configurations, that should correspond to the sublattices for the phase descriptions.
Non-mixing sublattices are represented as a string, while mixing sublattices are represented as a lists.
Thus an endmember for BCC_B2
(as in this example) is ["AL", "NI", VA"]
and if there were mixing (as in the next example) it might be ["AL", ["AL", "NI"], "VA"]
.
Mixing also means that the sublattice_occupancies
key must be specified, but that is not the case in this example.
It is important to note that any mixing configurations must have any ideal mixing contributions removed.
Regardless of whether there is mixing or not, the length of this list should always equal the number of sublattices in the phase, though the sub-lists can have mixing up to the number of components in that sublattice.
Note that the sublattice_configurations
is a list of these lists.
That is, there can be multiple sublattice configurations in a single dataset.
See the second example in this section for such an example.
The conditions
describe temperatures (T
) and pressures (P
) as either scalars or one-dimensional lists.
Most important to describing data are the output
and values
keys.
The type of quantity is expressed using the output
key.
This can in principle be any thermodynamic quantity, but currently only CPM*
, SM*
, and HM*
(where *
is either nothing, _MIX
or _FORM
) are supported.
Support for changing reference states planned but not yet implemented, so all thermodynamic quantities must be formation quantities (e.g. HM_FORM
or HM_MIX
, etc.).
The values
key is the most complicated and care must be taken to avoid mistakes.
values
is a 3-dimensional array where each value is the output
for a specific condition of pressure, temperature, and sublattice configurations from outside to inside.
Alternatively, the size of the array must be (len(P), len(T), len(subl_config))
.
In the example below, the shape of the values
array is (1, 12, 1) as there is one pressure scalar, one sublattice configuration, and 12 temperatures.
{
"reference": "Yi Wang et al 2009",
"components": ["AL", "NI", "VA"],
"phases": ["BCC_B2"],
"solver": {
"sublattice_site_ratios": [0.5, 0.5, 1],
"sublattice_configurations": [["AL", "NI", "VA"]],
"comment": "NiAl sublattice configuration (2SL)"
},
"conditions": {
"P": 101325,
"T": [ 0, 10, 20, 30, 40, 50, 60, 70, 80, 90, 100, 110]
},
"output": "CPM_FORM",
"values": [[[ 0 ],
[-0.0173 ],
[-0.01205],
[ 0.12915],
[ 0.24355],
[ 0.13305],
[-0.1617 ],
[-0.51625],
[-0.841 ],
[-1.0975 ],
[-1.28045],
[-1.3997 ]]]
}
In the second example below, there is formation enthalpy data for multiple sublattice configurations.
All of the keys and values are conceptually similar.
Here, instead of describing how the output
quantity changes with temperature or pressure, we are instead only comparing HM_FORM
values for different sublattice configurations.
The key differences from the previous example are that there are 9 different sublattice configurations described by sublattice_configurations
and sublattice_occupancies
.
Note that the sublattice_configurations
and sublattice_occupancies
should have exactly the same shape.
Sublattices without mixing should have single strings and occupancies of one.
Sublattices that do have mixing should have a site ratio for each active component in that sublattice.
If the sublattice of a phase is ["AL", "NI", "VA"]
, it should only have two occupancies if only ["AL", "NI"]
are active in the sublattice configuration.
The last difference to note is the shape of the values
array.
Here there is one pressure, one temperature, and 9 sublattice configurations to give a shape of (1, 1, 9).
{
"reference": "C. Jiang 2009 (constrained SQS)",
"components": ["AL", "NI", "VA"],
"phases": ["BCC_B2"],
"solver": {
"sublattice_occupancies": [
[1, [0.5, 0.5], 1],
[1, [0.75, 0.25], 1],
[1, [0.75, 0.25], 1],
[1, [0.5, 0.5], 1],
[1, [0.5, 0.5], 1],
[1, [0.25, 0.75], 1],
[1, [0.75, 0.25], 1],
[1, [0.5, 0.5], 1],
[1, [0.5, 0.5], 1]
],
"sublattice_site_ratios": [0.5, 0.5, 1],
"sublattice_configurations": [
["AL", ["NI", "VA"], "VA"],
["AL", ["NI", "VA"], "VA"],
["NI", ["AL", "NI"], "VA"],
["NI", ["AL", "NI"], "VA"],
["AL", ["AL", "NI"], "VA"],
["AL", ["AL", "NI"], "VA"],
["NI", ["AL", "VA"], "VA"],
["NI", ["AL", "VA"], "VA"],
["VA", ["AL", "NI"], "VA"]
],
"comment": "BCC_B2 sublattice configuration (2SL)"
},
"conditions": {
"P": 101325,
"T": 300
},
"output": "HM_FORM",
"values": [[[-40316.61077, -56361.58554,
-49636.39281, -32471.25149, -10890.09929,
-35190.49282, -38147.99217, -2463.55684,
-15183.13371]]]
}
Multi-phase Data¶
The difference between single- and multi-phase is data is in the absence of the solver
key, since we are no longer concerned with individual site configurations, and the values
key where we need to represent phase equilibria rather than thermodynamic quantities.
Notice that the type of data we are entering in the output
key is ZPF
(zero-phase fraction) rather than CP_FORM
or H_MIX
.
Each entry in the ZPF list is a list of all phases in equilibrium, here [["AL3NI2", ["NI"], [0.4083]], ["BCC_B2", ["NI"], [0.4340]]]
where each phase entry has the name of the phase, the composition element, and the composition of the tie line point.
If there is no corresponding tie line point, such as on a liquidus line, then one of the compositions will be null
: [["LIQUID", ["NI"], [0.6992]], ["BCC_B2", ["NI"], [null]]]
.
Three- or n-phase equilibria are described as expected: [["LIQUID", ["NI"], [0.752]], ["BCC_B2", ["NI"], [0.71]], ["FCC_L12", ["NI"], [0.76]]]
.
Note that for higher-order systems the component names and compositions are lists and should be of length c-1
, where c
is the number of components.
{
"components": ["AL", "NI"],
"phases": ["AL3NI2", "BCC_B2"],
"conditions": {
"P": 101325,
"T": [1348, 1176, 977]
},
"output": "ZPF",
"values": [
[["AL3NI2", ["NI"], [0.4083]], ["BCC_B2", ["NI"], [0.4340]]],
[["AL3NI2", ["NI"], [0.4114]], ["BCC_B2", ["NI"], [0.4456]]],
[["AL3NI2", ["NI"], [0.4114]], ["BCC_B2", ["NI"], [0.4532]]]
],
"reference": "37ALE"
}
Activity Data¶
Activity data is very similar to thermochemical data, except we must enter a reference state. Another minor detail is that that non-endmember compositions must be represented by composition conditions rather than as sublattice occupancies because it’s the result of equilibrium calculations where we cannot know the sublattice occupancies. An example for Cu-Mg activties follows, with data digitized from S.P. Garg, Y.J. Bhatt, C. V. Sundaram, Thermodynamic study of liquid Cu-Mg alloys by vapor pressure measurements, Metall. Trans. 4 (1973) 283–289. doi:10.1007/BF02649628.
{
"components": ["CU", "MG", "VA"],
"phases": ["LIQUID"],
"solver": {
"mode": "manual",
"sublattice_site_ratios": [1],
"sublattice_configurations": [["CU", "MG"]]
},
"reference_state": {
"phases": ["LIQUID"],
"conditions": {
"P": 101325,
"T": 1200,
"X_CU": 0.0
}
},
"conditions": {
"P": 101325,
"T": 1200,
"X_CU": [0.9, 0.8, 0.7, 0.6, 0.5, 0.4, 0.3, 0.2, 0.1, 0.0]
},
"output": "ACR_MG",
"values": [[[0.0057,0.0264,0.0825,0.1812,0.2645,0.4374,0.5852,0.7296,0.882,1.0]]],
"reference": "garg1973thermodynamic",
"comment": "Digitized Figure 3 and converted from activity coefficients."
}
Common Mistakes¶
- A single element sublattice is different in a phase model (
[["A", "B"], ["A"]]]
) than a sublattice configuration ([["A", "B"], "A"]
). - Make sure you use the right units (
J/mole-atom
, mole fractions, Kelvin, Pascal) - Mixing configurations should not have ideal mixing contributions.
ESPEI YAML input files¶
This page aims to completely describe the ESPEI input file in the YAML format. Possibly useful links are the YAML refcard and the (possibly less useful) Full YAML specification. These are all key value pairs in the format
key: value
They are nested for purely organizational purposes.
top_level_key:
key: value
As long as keys are nested under the correct heading, they have no required order. All of the possible keys are
system:
phase_models
datasets
output:
verbosity
output_db
tracefile
probfile
generate_parameters:
excess_model
ref_state
ridge_alpha
mcmc:
iterations
save_interval
cores
scheduler
input_db
restart_trace
chains_per_parameter
chain_std_deviation
deterministic
The next sections describe each of the keys individually.
If a setting has a default of required
it must be set explicitly.
system¶
The system
key is intended to describe the specific system you are fitting, including the components, phases, and the data to fit to.
phase_models¶
type: | string |
---|---|
default: | required |
The JSON file describing the CALPHAD models for each phase. See Phase Descriptions for an example of how to write this file.
datasets¶
type: | string |
---|---|
default: | required |
The path to a directory containing JSON files of input datasets.
The file extension to each of the datasets must be named as .json
, but they can otherwise be named freely.
For an examples of writing these input JSON files, see Making ESPEI datasets.
output¶
output_db¶
type: | string |
---|---|
default: | out.tdb |
The database to write out. Can be any file format that can be written by a pycalphad Database.
tracefile¶
type: | string |
---|---|
default: | trace.npy |
Name of the file that the MCMC trace is written to.
The array has shape (number of chains, iterations, number of parameters)
.
The array is preallocated and padded with zeros, so if you selected to take 2000 MCMC iterations, but only got through 1500, the last 500 values would be all 0.
You must choose a unique file name.
An error will be raised if file specified by tracefile
already exists.
probfile¶
type: | string |
---|---|
default: | lnprob.npy |
Name of the file that the MCMC ln probabilities are written to.
The array has shape (number of chains, iterations)
.
The array is preallocated and padded with zeros, so if you selected to take 2000 MCMC iterations, but only got through 1500, the last 500 values would be all 0.
You must choose a unique file name.
An error will be raised if file specified by probfile
already exists.
generate_parameters¶
The options in generate_parameters
are used to control parameter selection and fitting to single phase data.
This should be used if you have input thermochemical data, such as heat capacities and mixing energies.
Generate parameters will use the Akaike information criterion to select model parameters and fit them, creating a database.
excess_model¶
type: | string |
---|---|
default: | required |
options: | linear |
Which type of model to use for excess mixing parameters. Currently only linear is supported.
The exponential model is planned, as well as support for custom models.
ref_state¶
type: | string |
---|---|
default: | required |
options: | SGTE91 | SR2016 |
The reference state to use for the pure elements and lattice stabilities. Currently only SGTE91 and SR2016 (for certain elements) is supported.
There are plans to extend to support custom reference states.
ridge_alpha¶
type: | float |
---|---|
default: | 1.0e-100 |
Controls the ridge regression hyperparameter, $ alpha $, as given in the following equation for the ridge regression problem
ridge_alpha
should be a positive floating point number which scales the relative contribution of parameter magnitudes to the residuals.
If an exponential form is used, the floating point value must have a decimal place before the e
,
that is 1e-4
is invalid while 1.e-4
is valid. More generally, the floating point must match the following
regular expression per the YAML 1.1 spec: [-+]?([0-9][0-9_]*)?\.[0-9.]*([eE][-+][0-9]+)?
.
mcmc¶
The options in mcmc
control how Markov Chain Monte Carlo is performed using the emcee package.
In order to run an MCMC fitting, you need to specify one and only one source of parameters somewhere in the input file.
The parameters can come from including a generate_parameters
step, or by specifying the mcmc.input_db
key with a file to load as pycalphad Database.
If you choose to use the parameters from a database, you can then further control settings based on whether it is the first MCMC run for a system (you are starting fresh) or whether you are continuing from a previous run (a ‘restart’).
iterations¶
type: | int |
---|---|
default: | required |
Number of iterations to perform in emcee. Each iteration consists of accepting one step for each chain in the ensemble.
save_interval¶
type: | int |
---|---|
default: | 1 |
Controls the interval (in number of iterations) for saving the MCMC chain and probability files. By default, new files will be written out every iteration. For large files (many mcmc iterations and chains per parameter), these might become expensive to write out to disk.
cores¶
type: | int |
---|---|
min: | 1 |
How many cores from available cores to use during parallelization with dask or emcee. If the chosen number of cores is larger than available, then this value is ignored and espei defaults to using the number available.
Cores does not take affect for MPIPool scheduler option. MPIPool requires the number of processors be set directly with MPI.
scheduler¶
type: | string |
---|---|
default: | dask |
options: | dask | None | JSON file |
Which scheduler to use for parallelization. You can choose from either dask, None, or pass the path to a JSON scheduler file created by dask-distributed.
Choosing dask allows for the choice of cores used through the cores key.
Choosing None will result in no parallel scheduler being used. This is useful for debugging.
Passing the path to a JSON scheduler file will use the resources set up by the scheduler.
JSON file schedulers are most useful because schedulers can be started on MPI clusters using dask-mpi
command.
See Advanced Schedulers for more information.
input_db¶
type: | string |
---|---|
default: | null |
A file path that can be read as a pycalphad Database. The parameters to fit will be taken from this database.
For a parameter to be fit, it must be a symbol where the name starts with VV
, e.g. VV0001
.
For a TDB
formatted database, this means that the free parameters must be functions of a single value that are used in your parameters.
For example, the following is a valid symbol to fit:
FUNCTION VV0000 298.15 10000; 6000 N !
restart_trace¶
type: | string |
---|---|
default: | null |
If you have run a previous MCMC calculation, then you will have a trace file that describes the position and history of all of the chains from the run.
You can use these chains to start the emcee run and pick up from where you left off in the MCMC run by passing the trace file (e.g. chain.npy
) to this key.
If you are restarting from a previous calculation, you must also specify the same database file (with input_db
) as you used to run that calculation.
chains_per_parameter¶
type: | int |
---|---|
default: | 2 |
This controls the number of chains to run in the MCMC calculation as an integer multiple of the number of parameters.
This parameter can only be used when initializing the first MCMC run. If you are restarting a calculation, the number of chains per parameter is fixed by the number you chose previously.
Ensemble samplers require at least 2*p
chains for p
fitting parameters to be able to make proposals.
If chains_per_parameter = 2
, then the number of chains if there are 10 parameters to fit is 20.
The value of chains_per_parameter
must be an EVEN integer.
chain_std_deviation¶
type: | float |
---|---|
default: | 0.1 |
The standard deviation to use when initializing chains in a Gaussian distribution from a set of parameters as a fraction of the parameter.
A value of 0.1 means that for parameters with values (-1.5, 2000, 50000)
the chains will be initialized using those values as the mean and (0.15, 200, 5000)
as standard deviations for each parameter, respectively.
This parameter can only be used when initializing the first MCMC run. If you are restarting a calculation, the standard deviation for your chains are fixed by the value you chose previously.
You may technically set this to any positive value, you would like. Be warned that too small of a standard deviation may cause convergence to a local minimum in parameter space and slow convergence, while a standard deviation that is too large may cause convergence to meaningless thermodynamic descriptions.
deterministic¶
type: | bool |
---|---|
default: | True |
Toggles whether ESPEI runs are deterministic. If this is True, running
ESPEI with the same Database and initial settings (either the same
chains_per_parameter
and chain_std_deviation
or the same
restart_trace
) will result in exactly the same results.
Starting two runs with the same TDB or with parameter generation (which is deterministic) will result in the chains being at exactly the same position after 100 iterations. If these are both restarted after 100 iterations for another 50 iterations, then the final chain after 150 iterations will be the same.
It is important to note that this is only explictly True when starting at the same point. If Run 1 and Run 2 are started with the same initial parameters and Run 1 proceeds 50 iterations while Run 2 proceeds 100 iterations, restarting Run 1 for 100 iterations and Run 2 for 50 iterations (so they are both at 150 total iterations) will NOT give the same result.
Theory¶
ESPEI has two types of fitting – parameter generation and MCMC optimization. The parameter generation step uses experimental and DFT data of the Gibbs free energy derivatives (\(C_P, H, S\)) for each phase and for the mixing energies within sublattices for each phase to generate and fit parameters of given CALPHAD models. The MCMC optimization step uses a Bayesian optimization procedure to fit parameters in a Database to experimental phase equilibria.
Parameter generation¶
A simple model with few parameters is better than a complex model that describes the same data marginally better. Parameter generation in ESPEI aims to achieve a balance of a simple parameterization and goodness of fit in the Redlich-Kister polynomial used in CALPHAD assessments. To achieve this, parameters are selected using the corrected Akaike information criterion (AICc) to choose an optimal set of parameters from canditate parameterizations.
The general Redlich Kister polynomial has the form \(G = a + bT + cT\ln T + \sum_n d_n T^n\). Different parameterizations, e.g. only considering \(a\), considering \(a\) and \(b\), \(a\) and \(c\), etc. are fit to all of the input formation or mixing data (depending on the parameter being selected) by a least squares pseudo-inverse optimization.
Each parameterization is compared in the AICc and the most suitable optimization balances the goodness of fit and the number of parameters. The key aspect of this is that ESPEI will avoid overfitting your data and will not add parameters you do not have data for.
This is important for phases that would have a temperature dependent contribution to the Gibbs energy, but the input data only gives 0K formation energies. ESPEI cannot add temperature dependence to the parameterized model. Because of this, an abundance of single-phase data is critical to provide enough degrees of freedom in later optimization.
MCMC optimization¶
Details of Markov Chain Monte Carlo as an algorithm are better covered elsewhere. A good example is MacKay’s (free) book: Information Theory, Inference, and Learning Algorithms.
Using MCMC for optimizing CALPHAD models might appear to have several drawbacks. The parameters in the models are correlated and due to the nature of single phase first-principles data the shape and size of the posterior distribution for each parameter is not known before fitting. Traditional Metropolis-Hastings MCMC algorithms require the a prior to be defined for each parameter, which is a challenge for parameters in CALPHAD models which vary over more than 6 orders of magnitude.
ESPEI solves these potential problems by using an Ensemble sampler, as introduced by Goodman and Weare [1], rather than the Metropolis-Hastings algorithm. Ensemble samplers have the property of affine invariance, which uses multiple (\(\geq 2 N\) for \(N\) parameters) parallel chains to scale new proposal parameters by linear transforms. These chains, together an ensemble, define a proposal distribution to sample parameters from that is scaled to the magnitude and sensitivity of each parameter. Thus, Ensemble samplers directly address the challenges we expect to encounter with traditional MCMC.
ESPEI uses an Ensemble sampler algorithm by using the emcee package that implements parallelizable ensemble samplers. To use emcee, ESPEI defines the initial ensemble of chains and a function that returns the error as a log-probability. ESPEI defines the error as the mean square error between experimental phase equilibria and the equilibria calculated by the CALPHAD database.
Here, again, it is critical to point out the importance of abundant phase equilibria data. Traditional CALPHAD modeling has involved the modeler participating in tight feedback loops between updates to parameters and the resulting phase diagram. ESPEI departs from this by optimizing just a single scalar error function based on phase equilibria. The implication of this is that if there are phase equilibria that are observed to exist, but they are not in the datasets that are considered by ESPEI, those equilibria cannot be optimized against and may deviate from ‘known’ equilibria. A possible approach to address this in ESPEI is to estimate the points for the equilibria.
References¶
[1] | Goodman, J. & Weare, J. Ensemble samplers with affine invariance. Commun. Appl. Math. Comput. Sci. 5, 65–80 (2010). doi:10.2140/camcos.2010.5.65. |
Recipes¶
Here you can find some useful snippets of code to make using ESPEI easier.
Optimal parameter TDBs¶
Creating TDBs of optimal parameters from a tracefile and probfile:
"""
This script updates an input TDB file with the optimal parameters from an ESPEI run.
Change the capitalized variables to your desired input and output filenames.
"""
INPUT_TDB_FILENAME = 'CU-MG_param_gen.tdb'
OUTPUT_TDB_FILENAME = 'CU-MG_opt_params.tdb'
TRACE_FILENAME = 'trace.npy'
LNPROB_FILENAME = 'lnprob.npy'
import numpy as np
from pycalphad import Database
from espei.analysis import truncate_arrays
from espei.utils import database_symbols_to_fit, optimal_parameters
trace = np.load(TRACE_FILENAME)
lnprob = np.load(LNPROB_FILENAME)
trace, lnprob = truncate_arrays(trace, lnprob)
dbf = Database(INPUT_TDB_FILENAME)
opt_params = dict(zip(database_symbols_to_fit(dbf), optimal_parameters(trace, lnprob)))
dbf.symbols.update(opt_params)
dbf.to_file(OUTPUT_TDB_FILENAME)
Plotting phaes equilibria data¶
When compiling ESPEI datasets of phase equilibria data, it can be useful to plot the data to check that it matches visually with what you are expecting. This script plots a binary phase diagram.
TIP: Using this in Jupyter Notebooks make it really fast to update and watch your progress.
"""
This script will create a plot in a couple seconds from a datasets directory
that you can use to check your phase equilibria data.
Change the capitalized variables to the system information and the
directory of datasets you want to plot.
"""
COMPONENTS = ['CU', 'MG', 'VA']
INDEPENDENT_COMPONENT = "MG" # component to plot on the x-axis
PHASES = ['BCC_A2', 'CUMG2', 'FCC_A1', 'LAVES_C15', 'LIQUID']
DATASETS_DIRECTORY = "~/my-datasets/CU-MG"
X_MIN, X_MAX = 0.0, 1.0
Y_MIN, Y_MAX = 400, 1400
# script starts here, you shouldn't have to edit below this line
import os
from espei.plot import dataplot
from espei.datasets import recursive_glob, load_datasets
from pycalphad import variables as v
import matplotlib.pyplot as plt
plt.figure(figsize=(10,8))
ds = load_datasets(recursive_glob(os.path.expanduser(DATASETS_DIRECTORY), '*.json'))
conds = {v.P: 101325, v.T: (1,1,1), v.X(INDEPENDENT_COMPONENT): (1, 1, 1)}
dataplot(COMPONENTS, PHASES, conds, ds)
plt.xlim(X_MIN, X_MAX)
plt.ylim(Y_MIN, Y_MAX)
plt.show()
The script gives the following output:
Advanced Schedulers¶
ESPEI uses dask-distributed for parallelization and provides an easy way to deploy clusters locally via TCP with the mcmc.scheduler: dask
setting.
Sometimes ESPEI’s dask scheduling options are not sufficiently flexible for different environments.
As an alternative to setting the cores with the mcmc.scheduler: dask
setting,
you can provide ESPEI with a scheduler file from dask that has information about
how to connect to a dask parallel scheduler.
This is generally a two step process of
- Starting a scheduler with workers and writing a scheduler file
- Running ESPEI and connecting to the existing scheduler
In order to let the system manage the memory and prevent dask from pausing or killing workers, the memory limit should be set to zero.
Starting a scheduler¶
MPI-based dask scheduler¶
Dask provides a dask-mpi
command that sets this up for you and creates a scheduler file to pass to ESPEI.
The scheduler information will be serialized as a JSON file that you set in your ESPEI input file.
To start the scheduler and workers in the background, you can run the dask-mpi
command (use dask-mpi --help
to check the arguments).
The following command will start a scheduler on the main MPI task, then a worker for each remaining MPI task that mpirun
sees.
mpirun dask-mpi --scheduler-file my_scheduler.json --nthreads 1 --memory-limit 0 &
Generic scheduler¶
If you need further customization of dask schedulers, you can start a distributed Client any way you like, then write out the scheduler file for ESPEI to use.
For example, if you name the following file start_scheduler.py
, you can run this Python script in the background, which will contain the scheduler and workers, then ESPEI will connect to it.
# start_scheduler.py
from distributed import Client, LocalCluster
from tornado.ioloop import IOLoop
if __name__ == '__main__':
loop = IOLoop()
cluster = LocalCluster(n_workers=4, threads_per_worker=1, memory_limit=0)
client = Client(cluster)
client.write_scheduler_file('my-scheduler.json')
loop.start() # keeps the scheduler running
loop.close()
Running start_scheduler.py &
, will run this process in the background with 4 processes.
ESPEI Input¶
After starting the scheduler on the cluster, you run ESPEI like normal.
For the most part, this ESPEI input file is the same as you use locally, except the scheduler
parameter is set to the name of your scheduler file.
Here is an example for multiphase fitting starting from a generated TDB with a scheduler file named my-scheduler.json
:
system:
phase_models: my-phases.json
datasets: my-input-data
mcmc:
iterations: 1000
input_db: my-tdb.tdb
scheduler: my-scheduler.json
Example Queue Script - MPI¶
To run on through a queueing system, you’ll often use queue scripts that start batch jobs.
This example will create an MPI scheduler using dask-mpi
via mpirun
(or other MPI executable).
Since many MPI jobs are run through batch schedulers, an example script for a PBS job looks like:
#!/bin/bash
#PBS -l nodes=1:ppn=20
#PBS -l walltime=48:00:00
#PBS -A open
#PBS -N espei-mpi
#PBS -o espei-mpi.out
#PBS -e espei-mpi.error
# starts the scheduler on MPI and creates the scheduler file called 'my_scheduler.json'
# you can replace this line with any script that starts a scheduler
# e.g. a `start_scheduler.py` file
# make sure it ends with `&` to run the process in the background
mpirun dask-mpi --scheduler-file my_scheduler.json --nthreads 1 --memory-limit 0 &
# runs ESPEI as normal
espei --in espei-mpi-input.yaml
References¶
See http://distributed.readthedocs.io/en/latest/setup.html?highlight=dask-mpi#using-mpi for more details.
API Documentation¶
espei package¶
Subpackages¶
espei.error_functions package¶
Calculate error due to measured activities.
-
espei.error_functions.activity_error.
calculate_activity_error
(dbf, comps, phases, datasets, parameters=None, phase_models=None, callables=None)¶ Return the sum of square error from activity data
Parameters: - dbf (pycalphad.Database) – Database to consider
- comps (list) – List of active component names
- phases (list) – List of phases to consider
- datasets (espei.utils.PickleableTinyDB) – Datasets that contain single phase data
- parameters (dict) – Dictionary of symbols that will be overridden in pycalphad.equilibrium
- phase_models (dict) – Phase models to pass to pycalphad calculations
- callables (dict) – Callables to pass to pycalphad
Returns: A single float of the sum of square errors
Return type: float
Notes
General procedure: 1. Get the datasets 2. For each dataset
- Calculate reference state equilibrium
- Calculate current chemical potentials
- Find the target chemical potentials
- Calculate error due to chemical potentials
-
espei.error_functions.activity_error.
chempot_error
(sample_chempots, target_chempots)¶ Return the sum of square error from chemical potentials
- sample_chempots : numpy.ndarray
- Calculated chemical potentials
- target_activity : numpy.ndarray
- Chemical potentials to target
Returns: Error due to chemical potentials Return type: float
-
espei.error_functions.activity_error.
target_chempots_from_activity
(component, target_activity, temperatures, reference_result)¶ Return an array of experimental chemical potentials for the component
Parameters: - component (str) – Name of the component
- target_activity (numpy.ndarray) – Array of experimental activities
- temperatures (numpy.ndarray) – Ravelled array of temperatures (of same size as
exp_activity
). - reference_result (xarray.Dataset) – Dataset of the equilibrium reference state. Should contain a singe point calculation.
Returns: Array of experimental chemical potentials
Return type: numpy.ndarray
Calculate error due to thermochemical quantities: heat capacity, entropy, enthalpy.
-
espei.error_functions.thermochemical_error.
calculate_points_array
(phase_constituents, configuration, occupancies=None)¶ Calculate the points array to use in pycalphad calculate calls.
Converts the configuration data (and occupancies for mixing data) into the points array by looking up the indices in the active phase constituents.
Parameters: - phase_constituents (list) – List of active constituents in a phase
- configuration (list) – List of the sublattice configuration
- occupancies (list) – List of sublattice occupancies. Required for mixing sublattices, otherwise takes no effect.
Returns: Return type: numpy.ndarray
Notes
Errors will be raised if components in the configuration are not in the corresponding phase constituents sublattice.
-
espei.error_functions.thermochemical_error.
calculate_thermochemical_error
(dbf, comps, phases, datasets, parameters=None, phase_models=None, callables=None)¶ Calculate the weighted single phase error in the Database
Parameters: - dbf (pycalphad.Database) – Database to consider
- comps (list) – List of active component names
- phases (list) – List of phases to consider
- datasets (espei.utils.PickleableTinyDB) – Datasets that contain single phase data
- parameters (dict) – Dictionary of symbols that will be overridden in pycalphad.calculate
- phase_models (dict) – Phase models to pass to pycalphad calculations. Ideal mixing contributions must be removed.
- callables (dict) – Dictionary of {output_property: callables_dict} where callables_dict is a dictionary of {phase_name: callables} to pass to pycalphad. These must have ideal mixing portions removed.
Returns: A single float of the residual sum of square errors
Return type: float
Notes
There are different single phase values, HM_MIX, SM_FORM, CP_FORM, etc. Each of these have different units and the error cannot be compared directly. To normalize all of the errors, a normalization factor must be used. Equation 2.59 and 2.60 in Lukas, Fries, and Sundman “Computational Thermodynamics” shows how this can be considered. Each type of error will be weighted by the reciprocal of the estimated uncertainty in the measured value and conditions. The weighting factor is calculated by $ p_i = (Delta L_i)^{-1} $ where $ Delta L_i $ is the uncertainty in the measurement. We will neglect the uncertainty for quantities such as temperature, assuming they are small.
-
espei.error_functions.thermochemical_error.
get_prop_data
(comps, phase_name, prop, datasets)¶ Return datasets that match the components, phase and property
Parameters: - comps (list) – List of components to get data for
- phase_name (str) – Name of the phase to get data for
- prop (str) – Property to get data for
- datasets (espei.utils.PickleableTinyDB) – Datasets to search for data
Returns: List of dictionary datasets that match the criteria
Return type: list
-
espei.error_functions.thermochemical_error.
get_prop_samples
(dbf, comps, phase_name, desired_data)¶ Return data values and the conditions to calculate them by pycalphad calculate from the datasets
Parameters: - dbf (pycalphad.Database) – Database to consider
- comps (list) – List of active component names
- phase_name (str) – Name of the phase to consider from the Database
- desired_data (list) – List of dictionary datasets that contain the values to sample
Returns: Dictionary of condition kwargs for pycalphad’s calculate and the expected values
Return type: dict
Calculate error due to ZPF tielines.
The general approach is similar to the PanOptimizer rough search method.
- With all phases active, calculate the chemical potentials of the tieline
endpoints via
equilibrium
calls. Done inestimate_hyperplane
. - Calculate the target chemical potentials, which are the average chemical potentials of all of the current chemical potentials at the tieline endpoints.
- Calculate the current chemical potentials of the desired single phases
- The error is the difference between these chemical potentials
There’s some special handling for tieline endpoints where we do not know the composition conditions to calculate chemical potentials at.
-
espei.error_functions.zpf_error.
calculate_zpf_error
(dbf, comps, phases, datasets, phase_models, parameters=None, callables=None)¶ Calculate error due to phase equilibria data
Parameters: - dbf (pycalphad.Database) – Database to consider
- comps (list) – List of active component names
- phases (list) – List of phases to consider
- datasets (espei.utils.PickleableTinyDB) – Datasets that contain single phase data
- phase_models (dict) – Phase models to pass to pycalphad calculations
- parameters (dict) – Dictionary of symbols that will be overridden in pycalphad.equilibrium
- callables (dict) – Callables to pass to pycalphad
Returns: List of errors from phase equilibria data
Return type: list
-
espei.error_functions.zpf_error.
estimate_hyperplane
(dbf, comps, phases, current_statevars, comp_dicts, phase_models, parameters, callables=None)¶ Calculate the chemical potentials for a hyperplane, one vertex at a time
Parameters: - dbf (pycalphad.Database) – Database to consider
- comps (list) – List of active component names
- phases (list) – List of phases to consider
- current_statevars (dict) – Dictionary of state variables, e.g. v.P and v.T, no compositions.
- comp_dicts (list) – List of tuples of composition dictionaries and phase flags. Composition dictionaries are pycalphad variable dicts and the flag is a string e.g. ({v.X(‘CU’): 0.5}, ‘disordered’)
- phase_models (dict) – Phase models to pass to pycalphad calculations
- parameters (dict) – Dictionary of symbols that will be overridden in pycalphad.equilibrium
- callables (dict) – Callables to pass to pycalphad
Returns: Array of chemical potentials.
Return type: numpy.ndarray
Notes
This takes just one set of phase equilibria, e.g. a dataset point of [[‘FCC_A1’, [‘CU’], [0.1]], [‘LAVES_C15’, [‘CU’], [0.3]]] and calculates the chemical potentials given all the phases possible at the given compositions. Then the average chemical potentials of each end point are taken as the target hyperplane for the given equilibria.
-
espei.error_functions.zpf_error.
tieline_error
(dbf, comps, current_phase, cond_dict, region_chemical_potentials, phase_flag, phase_models, parameters, debug_mode=False, callables=None)¶ Parameters: - dbf (pycalphad.Database) – Database to consider
- comps (list) – List of active component names
- current_phase (list) – List of phases to consider
- current_statevars (dict) – Dictionary of state variables, e.g. v.P and v.T, no compositions.
- comp_dicts (list) – List of tuples of composition dictionaries and phase flags. Composition dictionaries are pycalphad variable dicts and the flag is a string e.g. ({v.X(‘CU’): 0.5}, ‘disordered’)
- phase_models (dict) – Phase models to pass to pycalphad calculations
- parameters (dict) – Dictionary of symbols that will be overridden in pycalphad.equilibrium
- callables (dict) – Callables to pass to pycalphad
- cond_dict –
- region_chemical_potentials (numpy.ndarray) – Array of chemical potentials for target equilibrium hyperplane.
- phase_flag (str) – String of phase flag, e.g. ‘disordered’.
- phase_models – Phase models to pass to pycalphad calculations
- parameters – Dictionary of symbols that will be overridden in pycalphad.equilibrium
- debug_mode (bool) – If True, will write out scripts when pycalphad fails to find a stable equilibrium. These scripts can be used to debug pycalphad.
Returns: Single value for the total error between the current hyperplane and target hyperplane.
Return type: float
Functions for calculating error.
espei.parameter_selection package¶
Building candidate models
-
espei.parameter_selection.model_building.
build_candidate_models
(configuration, features)¶ Return a dictionary of features and candidate models
Parameters: - configuration (tuple) – Configuration tuple, e.g. ((‘A’, ‘B’, ‘C’), ‘A’)
- features (dict) – Dictionary of {str: list} of generic features for a model, not considering the configuration. For example: {‘CPM_FORM’: [sympy.S.One, v.T, v.T**2, v.T**3]}
Returns: Dictionary of {feature: [candidate_models])
Return type: dict
Notes
Currently only works for binary and ternary interactions.
Candidate models match the following spec: 1. Candidates with multiple features specified will have 2. orders of parameters (L0, L0 and L1, …) have the same number of temperatures
Note that high orders of parameters with multiple temperatures are not required to contain all the temperatures of the low order parameters. For example, the following parameters can be generated L0: A L1: A + BT
-
espei.parameter_selection.model_building.
build_feature_sets
(temperature_features, interaction_features)¶ Return a list of broadcasted features
Parameters: - temperature_features (list) – List of temperature features that will become a successive_list, such as [TlogT, T-1, T2]
- interaction_features (list) – List of interaction features that will become a successive_list, such as [YS, YS*Z, YS*Z**2]
Returns: Return type: list
Notes
This allows two sets of features, e.g. [TlogT, T-1, T2] and [YS, YS*Z, YS*Z**2] and generates a list of feature sets where the temperatures and interactions are broadcasted successively.
Generates candidate feature sets like: L0: A + BT, L1: A L0: A , L1: A + BT
but not lists that are not successive: L0: A + BT, L1: Nothing, L2: A L0: Nothing, L1: A + BT
There’s still some debate whether it makes sense from an information theory perspective to add a L1 B term without an L0 B term. However this might be more representative of how people usually model thermodynamics.
Does not distribute multiplication/sums or make assumptions about the elements of the feature lists. They can be strings, ints, objects, tuples, etc..
The number of features (related to the complexity) is a geometric series. For $N$ temperature features and $M$ interaction features, the total number of feature sets should be $N*(1-N**M)/(1-N)$. If $N=1$, then there are $M$ total feature sets.
-
espei.parameter_selection.model_building.
make_successive
(xs)¶ Return a list of successive combinations
Parameters: xs (list) – List of elements, e.g. [X, Y, Z] Returns: List of combinations where each combination include all the preceding elements Return type: list Examples
>>> make_successive(['W', 'X', 'Y', 'Z']) [['W'], ['W', 'X'], ['W', 'X', 'Y'], ['W', 'X', 'Y', 'Z']]
Tools for construction Redlich-Kister polynomials used in parameter selection.
-
espei.parameter_selection.redlich_kister.
calc_interaction_product
(site_fractions)¶ Calculate the interaction product for sublattice configurations
Parameters: site_fractions (list) – List of sublattice configurations. Sites on each sublattice be in order with respect to the elements in the sublattice. The list should be 3d of (configurations, sublattices, values) Returns: List of interaction products, Z, for each sublattice Return type: list Examples
>>> # interaction product for an (A) configuration >>> calc_interaction_product([[1.0]]) # doctest: +ELLIPSIS [1.0] >>> # interaction product for [(A,B), (A,B)(A)] configurations that are equal >>> calc_interaction_product([[[0.5, 0.5]], [[0.5, 0.5], 1]]) # doctest: +ELLIPSIS [0.0, 0.0] >>> # interaction product for an [(A,B)] configuration >>> calc_interaction_product([[[0.1, 0.9]]]) # doctest: +ELLIPSIS [-0.8] >>> # interaction product for an [(A,B)(A,B)] configuration >>> calc_interaction_product([[[0.2, 0.8], [0.4, 0.6]]]) # doctest: +ELLIPSIS [0.12] >>> # ternary case, (A,B,C) interaction >>> calc_interaction_product([[[0.333, 0.333, 0.334]]]) [[0.333, 0.333, 0.334]] >>> # ternary 2SL case, (A,B,C)(A) interaction >>> calc_interaction_product([[[0.333, 0.333, 0.334], 1.0]]) [[0.333, 0.333, 0.334]]
-
espei.parameter_selection.redlich_kister.
calc_site_fraction_product
(site_fractions)¶ Calculate the site fraction product for sublattice configurations
Parameters: site_fractions (list) – List of sublattice configurations. The list should be 3d of (configurations, sublattices, values) Returns: List of site fraction products, YS, for each sublattice Return type: list Examples
>>> # site fraction product for an (A,B)(A) configuration >>> calc_site_fraction_product([[[0.2, 0.8], 1.0]]) # doctest: +ELLIPSIS [0.16...] >>> # site fraction product for [(A,B)(A), (A,B)(A)] configurations >>> calc_site_fraction_product([[[0.2, 0.8], 1.0], [[0.3, 0.7], 1.0]]) # doctest: +ELLIPSIS [0.16..., 0.21] >>> # site fraction product for [(A,B)(A,B)] configurations >>> calc_site_fraction_product([[[0.2, 0.8], [0.4, 0.6]]]) # doctest: +ELLIPSIS [0.0384...] >>> # ternary case, (A,B,C) interaction >>> calc_site_fraction_product([[[0.25, 0.25, 0.5]]]) [0.03125]
Fit, score and select models
-
espei.parameter_selection.selection.
fit_model
(feature_matrix, data_quantities, ridge_alpha)¶ Return model coefficients fit by scikit-learn’s LinearRegression
Parameters: - feature_matrix (ndarray) – (M*N) regressor matrix. The transformed model inputs (y_i, T, P, etc.)
- data_quantities (ndarray) – (M,) response vector. Target values of the output (e.g. HM_MIX) to reproduce.
- ridge_alpha (float) – Value of the $alpha$ hyperparameter used in ridge regression. Defaults to 1.0e-100, which should be degenerate with ordinary least squares regression. For now, the parameter is applied to all features.
Returns: List of model coefficients of shape (N,)
Return type: list
Notes
Solve Ax = b. x are the desired model coefficients. A is the ‘feature_matrix’. b corrresponds to ‘data_quantities’.
-
espei.parameter_selection.selection.
score_model
(feature_matrix, data_quantities, model_coefficients, feature_list, rss_numerical_limit=1e-16)¶ Use the AICc to score a model that has been fit.
Parameters: - feature_matrix (ndarray) – (M*N) regressor matrix. The transformed model inputs (y_i, T, P, etc.)
- data_quantities (ndarray) – (M,) response vector. Target values of the output (e.g. HM_MIX) to reproduce.
- model_coefficients (list) – List of fitted model coefficients to be scored. Has shape (N,).
- feature_list (list) – Polynomial coefficients corresponding to each column of ‘feature_matrix’. Has shape (N,). Purely a logging aid.
- rss_numerical_limit (float) – Anything with an absolute value smaller than this is set to zero.
Returns: A model score
Return type: float
Notes
Solve Ax = b, where ‘feature_matrix’ is A and ‘data_quantities’ is b.
The likelihood function is a simple least squares with no regularization. The form of the AIC is valid under assumption all sample variances are random and Gaussian, model is univariate. It is assumed the model here is univariate with T.
-
espei.parameter_selection.selection.
select_model
(candidate_models, ridge_alpha)¶ Select a model from a series of candidates by fitting and scoring them
Parameters: - candidate_models (list) – List of tuples of (features, feature_matrix, data_quantities)
- ridge_alpha (float) – Value of the $alpha$ hyperparameter used in ridge regression. Defaults to 1.0e-100, which should be degenerate with ordinary least squares regression. For now, the parameter is applied to all features.
Returns: Tuple of (feature_list, model_coefficients) for the highest scoring model
Return type: tuple
Build fittable models for ternary parameter selection
-
espei.parameter_selection.ternary_parameters.
build_ternary_feature_matrix
(prop, candidate_models, desired_data)¶ Return an MxN matrix of M data sample and N features.
Parameters: - prop (str) – String name of the property, e.g. ‘HM_MIX’
- candidate_models (list) – List of SymPy parameters that can be fit for this property.
- desired_data (dict) – Full dataset dictionary containing values, conditions, etc.
Returns: An MxN matrix of M samples (from desired data) and N features.
Return type: numpy.ndarray
Tools used across parameter selection modules
-
espei.parameter_selection.utils.
shift_reference_state
(desired_data, feature_transform, fixed_model)¶ Shift data to a new common reference state.
Submodules¶
espei.analysis module¶
Tools for analyzing ESPEI runs
-
espei.analysis.
truncate_arrays
(trace_array, prob_array=None)¶ Return slides of ESPEI output arrays with any empty remaining iterations (zeros) removed.
Parameters: - trace_array (np.ndarray) – Array of the trace from an ESPEI run. Should have shape (chains, iterations, parameters)
- prob_array (np.ndarray) – Array of the lnprob output from an ESPEI run. Should have shape (chains, iterations)
Returns: A slide of the zeros-removed trace array is returned if only the trace is passed. Otherwise a tuple of both the trace and lnprob are returned.
Return type: np.ndarry or (np.ndarray, np.ndarray)
espei.core_utils module¶
Internal utilities for developer use. May not be useful to users.
-
espei.core_utils.
get_data
(comps, phase_name, configuration, symmetry, datasets, prop)¶ Return list of cleaned single phase datasets matching the passed arguments.
Parameters: - comps (list) – List of string component names
- phase_name (str) – Name of phase
- configuration (tuple) – Sublattice configuration as a tuple, e.g. (“CU”, (“CU”, “MG”))
- symmetry (list of lists) – List of sublattice indices with symmetry
- datasets (espei.utils.PickleableTinyDB) – Database of datasets to search for data
- prop (list) – String name of the property of interest.
Returns: List of datasets matching the arguments.
Return type: list
-
espei.core_utils.
get_samples
(desired_data)¶ Return the data values from desired_data, transformed to interaction products.
Parameters: desired_data (list) – List of matched desired data, e.g. for a single property Returns: List of sample values that are properly transformed. Return type: list Notes
Transforms data to interaction products, e.g. YS*{}^{xs}G=YS*XS*DXS^{n} {}^{n}L
-
espei.core_utils.
ravel_conditions
(values, *conditions, **kwargs)¶ Broadcast and flatten conditions to the shape dictated by the values.
Special handling for ZPF data that does not have nice array values.
Parameters: - values (list) – Multidimensional lists of values
- conditions (list) – List of conditions to broadcast. Must be the same length as the number of dimensions of the values array. In code, the following must be True: all([s == len(cond) for s, cond in zip(values.shape, conditions)])
- zpf (bool, optional) – Whether to consider values as a special case of ZPF data (not an even grid of conditions) Default is False
Returns: Tuple of ravelled conditions
Return type: tuple
Notes
The current implementation of ZPF data only has the shape for one condition and this assumption is hardcoded in various places.
Here we try to be as general as possible by explicitly calculating the shape of the ZPF values.
A complication of this is that the user of this function must pass the correct conditions because usually T and P are specified in ZPF (but, again, only one can actually be a condition given the current shape).
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espei.core_utils.
ravel_zpf_values
(desired_data, independent_comps, conditions=None)¶ Unpack the phases and compositions from ZPF data. Dependent components are converted to independent components.
Parameters: - desired_data (espei.utils.PickleableTinyDB) – The selected data
- independent_comps (list) – List of indepdendent components. Used for mass balance component conversion
- conditions (dict) – Conditions to filter for. Right now only considers fixed temperatures
Returns: A dictonary of list of lists of tuples. Each dictionary key is the number of phases in equilibrium, e.g. a key “2” might have values [[(PHASE_NAME_1, {‘C1’: X1, ‘C2’: X2}, refkey), (PHASE_NAME_2, {‘C1’: X1, ‘C2’: X2}, refkey)], …] Three would have three inner tuples and so on.
Return type: dict
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espei.core_utils.
recursive_map
(f, x)¶ map, but over nested lists
Parameters: - f (callable) – Function to apply to x
- x (list or value) – Value passed to v
Returns: Return type: list or value
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espei.core_utils.
symmetry_filter
(x, config, symmetry)¶ Return True if the candidate sublattice configuration has any symmetry which matches the phase model symmetry.
Parameters: - x (dict) – the candidate dataset ‘solver’ dict. Must contain the “sublattice_configurations” key
- config (list) – the configuration of interest: e.g. [‘AL’, [‘AL’, ‘NI’], ‘VA’]
- symmetry (list) – tuple of tuples where each inner tuple is a group of equivalent sublattices. A value of ((0, 1), (2, 3, 4)) means that sublattices at indices 0 and 1 are symmetrically equivalent to each other and sublattices at indices 2, 3, and 4 are symetrically equivalent to each other.
Returns: Return type: bool
espei.datasets module¶
-
exception
espei.datasets.
DatasetError
¶ Bases:
Exception
Exception raised when datasets are invalid.
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espei.datasets.
check_dataset
(dataset)¶ Ensure that the dataset is valid and consistent.
Currently supports the following validation checks: * data shape is valid * phases and components used match phases and components entered * individual shapes of keys, such as ZPF, sublattice configs and site ratios
Planned validation checks: * all required keys are present
Note that this follows some of the implicit assumptions in ESPEI at the time of writing, such that conditions are only P, T, configs for single phase and essentially only T for ZPF data.
Parameters: dataset (dict) – Dictionary of the standard ESPEI dataset. Returns: Return type: None Raises: DatasetError
– If an error is found in the dataset
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espei.datasets.
clean_dataset
(dataset)¶ Clean an ESPEI dataset dictionary.
Parameters: dataset (dict) – Dictionary of the standard ESPEI dataset. dataset : dic Returns: Modified dataset that has been cleaned Return type: dict Notes
Assumes a valid, checked dataset. Currently handles * Converting expected numeric values to floats
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espei.datasets.
load_datasets
(dataset_filenames)¶ Create a PickelableTinyDB with the data from a list of filenames.
Parameters: dataset_filenames ([str]) – List of filenames to load as datasets Returns: Return type: PickleableTinyDB
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espei.datasets.
recursive_glob
(start, pattern)¶ Recursively glob for the given pattern from the start directory.
Parameters: - start (str) – Path of the directory to walk while for file globbing
- pattern (str) – Filename pattern to match in the glob
Returns: List of matched filenames
Return type: [str]
espei.espei_script module¶
Automated fitting script.
A minimal run must specify an input.json and a datasets folder containing input files.
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espei.espei_script.
get_run_settings
(input_dict)¶ Validate settings from a dict of possible input.
Performs the following actions: 1. Normalize (apply defaults) 2. Validate against the schema
Parameters: input_dict (dict) – Dictionary of input settings Returns: Validated run settings Return type: dict Raises: ValueError
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espei.espei_script.
log_version_info
()¶ Print version info to the log
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espei.espei_script.
main
()¶ Handle starting ESPEI from the command line. Parse command line arguments and input file.
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espei.espei_script.
run_espei
(run_settings)¶ Wrapper around the ESPEI fitting procedure, taking only a settings dictionary.
Parameters: run_settings (dict) – Dictionary of input settings Returns: Return type: Either a Database (for generate parameters only) or a tuple of (Database, sampler)
espei.mcmc module¶
Module for running MCMC in ESPEI
MCMC uses an EnsembleSampler based on Goodman and Weare, Ensemble Samplers with Affine Invariance. Commun. Appl. Math. Comput. Sci. 5, 65-80 (2010).
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espei.mcmc.
generate_parameter_distribution
(parameters, num_samples, std_deviation, deterministic=True)¶ Return an array of num_samples from a Gaussian distribution about each parameter.
Parameters: - parameters (ndarray) – 1D array of initial parameters that will be the mean of the distribution.
- num_samples (int) – Number of chains to initialize.
- std_deviation (float) – Fractional standard deviation of the parameters to use for initialization.
- deterministic (bool) – True if the parameters should be generated deterministically.
Returns: Return type: ndarray
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espei.mcmc.
lnprob
(params, comps=None, dbf=None, phases=None, datasets=None, symbols_to_fit=None, phase_models=None, scheduler=None, callables=None, thermochemical_callables=None)¶ Returns the error from multiphase fitting as a log probability.
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espei.mcmc.
mcmc_fit
(dbf, datasets, iterations=1000, save_interval=100, chains_per_parameter=2, chain_std_deviation=0.1, scheduler=None, tracefile=None, probfile=None, restart_trace=None, deterministic=True)¶ Run Markov Chain Monte Carlo on the Database given datasets
Parameters: - dbf (Database) – A pycalphad Database to fit with symbols to fit prefixed with VV followed by a number, e.g. VV0001
- datasets (PickleableTinyDB) – A database of single- and multi-phase to fit
- iterations (int) – Number of trace iterations to calculate in MCMC. Default is 1000 iterations.
- save_interval (int) – interval of iterations to save the tracefile and probfile
- chains_per_parameter (int) – number of chains for each parameter. Must be an even integer greater or equal to 2. Defaults to 2.
- chain_std_deviation (float) – standard deviation of normal for parameter initialization as a fraction of each parameter. Must be greater than 0. Default is 0.1, which is 10%.
- scheduler (callable) – Scheduler to use with emcee. Must implement a map method.
- tracefile (str) – filename to store the trace with NumPy.save. Array has shape (chains, iterations, parameters)
- probfile (str) – filename to store the log probability with NumPy.save. Has shape (chains, iterations)
- restart_trace (np.ndarray) – ndarray of the previous trace. Should have shape (chains, iterations, parameters)
- deterministic (bool) – If True, the emcee sampler will be seeded to give deterministic sampling draws. This will ensure that the runs with the exact same database, chains_per_parameter, and chain_std_deviation (or restart_trace) will produce exactly the same results.
Returns: - dbf (Database) – Resulting pycalphad database of optimized parameters
- sampler (EnsembleSampler, ndarray)) – emcee sampler for further data wrangling
espei.paramselect module¶
The paramselect module handles automated parameter selection for linear models.
Automated Parameter Selection End-members
Note: All magnetic parameters from literature for now. Note: No fitting below 298 K (so neglect third law issues for now).
For each step, add one parameter at a time and compute AICc with max likelihood.
Cp - TlnT, T**2, T**-1, T**3 - 4 candidate models (S and H only have one required parameter each. Will fit in full MCMC procedure)
Choose parameter set with best AICc score.
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espei.paramselect.
fit_formation_energy
(dbf, comps, phase_name, configuration, symmetry, datasets, ridge_alpha=1e-100, features=None)¶ Find suitable linear model parameters for the given phase. We do this by successively fitting heat capacities, entropies and enthalpies of formation, and selecting against criteria to prevent overfitting. The “best” set of parameters minimizes the error without overfitting.
Parameters: - dbf (Database) – pycalphad Database. Partially complete, so we know what degrees of freedom to fix.
- comps ([str]) – Names of the relevant components.
- phase_name (str) – Name of the desired phase for which the parameters will be found.
- configuration (ndarray) – Configuration of the sublattices for the fitting procedure.
- symmetry ([[int]]) – Symmetry of the sublattice configuration.
- datasets (PickleableTinyDB) – All the datasets desired to fit to.
- ridge_alpha (float) – Value of the $alpha$ hyperparameter used in ridge regression. Defaults to 1.0e-100, which should be degenerate with ordinary least squares regression. For now, the parameter is applied to all features.
- features (dict) – Maps “property” to a list of features for the linear model. These will be transformed from “GM” coefficients e.g., {“CPM_FORM”: (v.T*sympy.log(v.T), v.T**2, v.T**-1, v.T**3)} (Default value = None)
Returns: {feature: estimated_value}
Return type: dict
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espei.paramselect.
fit_ternary_interactions
(dbf, phase_name, symmetry, endmembers, datasets, ridge_alpha=0.0)¶ Fit ternary interactions for a database in place
Parameters: - dbf (Database) – pycalphad Database to add parameters to
- phase_name (str) – Name of the phase to fit
- symmetry (list) – List of symmetric sublattices, e.g. [[0, 1, 2], [3, 4]]
- endmembers (list) – List of endmember tuples, e.g. [(‘CU’, ‘MG’)]
- datasets (PickleableTinyDB) – TinyDB database of datasets
- ridge_alpha (float) – Value of the $alpha$ hyperparameter used in ridge regression. Defaults to 1.0e-100, which should be degenerate with ordinary least squares regression. For now, the parameter is applied to all features.
Returns: Modified the Database in place
Return type: None
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espei.paramselect.
generate_parameters
(phase_models, datasets, ref_state, excess_model, ridge_alpha=1e-100)¶ Generate parameters from given phase models and datasets
Parameters: - phase_models (dict) – Dictionary of components and phases to fit.
- datasets (PickleableTinyDB) – database of single- and multi-phase to fit.
- ref_state (str) – String of the reference data to use, e.g. ‘SGTE91’ or ‘SR2016’
- excess_model (str) – String of the type of excess model to fit to, e.g. ‘linear’
- ridge_alpha (float) – Value of the $alpha$ hyperparameter used in ridge regression. Defaults to 1.0e-100, which should be degenerate with ordinary least squares regression. For now, the parameter is applied to all features.
Returns: Return type: pycalphad.Database
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espei.paramselect.
get_next_symbol
(dbf)¶ Return a string name of the next free symbol to set
Parameters: dbf (Database) – pycalphad Database. Must have the varcounter
attribute set to an integer.Returns: Return type: str
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espei.paramselect.
phase_fit
(dbf, phase_name, symmetry, subl_model, site_ratios, datasets, refdata, ridge_alpha, aliases=None)¶ Generate an initial CALPHAD model for a given phase and sublattice model.
Parameters: - dbf (Database) – pycalphad Database to add parameters to.
- phase_name (str) – Name of the phase.
- symmetry ([[int]]) – Sublattice model symmetry.
- subl_model ([[str]]) – Sublattice model for the phase of interest.
- site_ratios ([float]) – Number of sites in each sublattice, normalized to one atom.
- datasets (PickleableTinyDB) – All datasets to consider for the calculation.
- refdata (dict) – Maps tuple(element, phase_name) -> SymPy object defining energy relative to SER
- ridge_alpha (float) – Value of the $alpha$ hyperparameter used in ridge regression. Defaults to 1.0e-100, which should be degenerate with ordinary least squares regression. For now, the parameter is applied to all features.
- aliases ([str]) – Alternative phase names. Useful for matching against reference data or other datasets. (Default value = None)
Returns: Modifies the dbf.
Return type: None
espei.plot module¶
Plotting of input data and calculated database quantities
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espei.plot.
dataplot
(comps, phases, conds, datasets, ax=None, plot_kwargs=None, tieline_plot_kwargs=None)¶ Plot datapoints corresponding to the components, phases, and conditions.
Parameters: - comps (list) – Names of components to consider in the calculation.
- phases ([]) – Names of phases to consider in the calculation.
- conds (dict) – Maps StateVariables to values and/or iterables of values.
- datasets (PickleableTinyDB) –
- ax (matplotlib.Axes) – Default axes used if not specified.
- plot_kwargs (dict) – Additional keyword arguments to pass to the matplotlib plot function for points
- tieline_plot_kwargs (dict) – Additional keyword arguments to pass to the matplotlib plot function for tielines
Returns: A plot of phase equilibria points as a figure
Return type: matplotlib.Axes
Examples
>>> from espei.datasets import load_datasets, recursive_glob # doctest: +SKIP >>> from espei.plot import dataplot # doctest: +SKIP >>> datasets = load_datasets(recursive_glob('.', '*.json')) # doctest: +SKIP >>> my_phases = ['BCC_A2', 'CUMG2', 'FCC_A1', 'LAVES_C15', 'LIQUID'] # doctest: +SKIP >>> my_components = ['CU', 'MG' 'VA'] # doctest: +SKIP >>> conditions = {v.P: 101325, v.T: (500, 1000, 10), v.X('MG'): (0, 1, 0.01)} # doctest: +SKIP >>> dataplot(my_components, my_phases, conditions, datasets) # doctest: +SKIP
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espei.plot.
eqdataplot
(eq, datasets, ax=None, plot_kwargs=None)¶ Plot datapoints corresponding to the components and phases in the eq Dataset. A convenience function for dataplot.
Parameters: - eq (xarray.Dataset) – Result of equilibrium calculation.
- datasets (PickleableTinyDB) – Database of phase equilibria datasets
- ax (matplotlib.Axes) – Default axes used if not specified.
- plot_kwargs (dict) – Keyword arguments to pass to dataplot
Returns: Return type: A plot of phase equilibria points as a figure
Examples
>>> from pycalphad import equilibrium, Database, variables as v # doctest: +SKIP >>> from pycalphad.plot.eqplot import eqplot # doctest: +SKIP >>> from espei.datasets import load_datasets, recursive_glob # doctest: +SKIP >>> datasets = load_datasets(recursive_glob('.', '*.json')) # doctest: +SKIP >>> dbf = Database('my_databases.tdb') # doctest: +SKIP >>> my_phases = list(dbf.phases.keys()) # doctest: +SKIP >>> eq = equilibrium(dbf, ['CU', 'MG', 'VA'], my_phases, {v.P: 101325, v.T: (500, 1000, 10), v.X('MG'): (0, 1, 0.01)}) # doctest: +SKIP >>> ax = eqplot(eq) # doctest: +SKIP >>> ax = eqdataplot(eq, datasets, ax=ax) # doctest: +SKIP
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espei.plot.
multiplot
(dbf, comps, phases, conds, datasets, eq_kwargs=None, plot_kwargs=None, data_kwargs=None)¶ Plot a phase diagram with datapoints described by datasets. This is a wrapper around pycalphad.equilibrium, pycalphad’s eqplot, and dataplot.
Parameters: - dbf (Database) – pycalphad thermodynamic database containing the relevant parameters.
- comps (list) – Names of components to consider in the calculation.
- phases (list) – Names of phases to consider in the calculation.
- conds (dict) – Maps StateVariables to values and/or iterables of values.
- datasets (PickleableTinyDB) – Database of phase equilibria datasets
- eq_kwargs (dict) – Keyword arguments passed to pycalphad equilibrium()
- plot_kwargs (dict) – Keyword arguments passed to pycalphad eqplot()
- data_kwargs (dict) – Keyword arguments passed to dataplot()
Returns: Return type: A phase diagram with phase equilibria data as a figure
Examples
>>> from pycalphad import Database, variables as v # doctest: +SKIP >>> from pycalphad.plot.eqplot import eqplot # doctest: +SKIP >>> from espei.datasets import load_datasets, recursive_glob # doctest: +SKIP >>> datasets = load_datasets(recursive_glob('.', '*.json')) # doctest: +SKIP >>> dbf = Database('my_databases.tdb') # doctest: +SKIP >>> my_phases = list(dbf.phases.keys()) # doctest: +SKIP >>> multiplot(dbf, ['CU', 'MG', 'VA'], my_phases, {v.P: 101325, v.T: 1000, v.X('MG'): (0, 1, 0.01)}, datasets) # doctest: +SKIP
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espei.plot.
plot_parameters
(dbf, comps, phase_name, configuration, symmetry, datasets=None, fig=None, require_data=True)¶ Plot parameters of interest compared with data in subplots of a single figure
Parameters: - dbf (Database) – pycalphad thermodynamic database containing the relevant parameters.
- comps (list) – Names of components to consider in the calculation.
- phase_name (str) – Name of the considered phase phase
- configuration (tuple) – Sublattice configuration to plot, such as (‘CU’, ‘CU’) or ((‘CU’, ‘MG’), ‘CU’)
- symmetry (list) – List of lists containing indices of symmetric sublattices e.g. [[0, 1], [2, 3]]
- datasets (PickleableTinyDB) – ESPEI datasets to compare against. If None, nothing is plotted.
- fig (matplotlib.Figure) – Figure to create with axes as subplots.
- require_data (bool) – If True, plot parameters that have data corresponding data. Defaults to True. Will raise an error for non-interaction configurations.
Returns: Return type: None
Examples
>>> # plot the LAVES_C15 (Cu)(Mg) endmember >>> plot_parameters(dbf, ['CU', 'MG'], 'LAVES_C15', ('CU', 'MG'), symmetry=None, datasets=datasets) # doctest: +SKIP >>> # plot the mixing interaction in the first sublattice >>> plot_parameters(dbf, ['CU', 'MG'], 'LAVES_C15', (('CU', 'MG'), 'MG'), symmetry=None, datasets=datasets) # doctest: +SKIP
espei.refdata module¶
Create a new Mock object. Mock takes several optional arguments that specify the behaviour of the Mock object:
spec: This can be either a list of strings or an existing object (a class or instance) that acts as the specification for the mock object. If you pass in an object then a list of strings is formed by calling dir on the object (excluding unsupported magic attributes and methods). Accessing any attribute not in this list will raise an AttributeError.
If spec is an object (rather than a list of strings) then mock.__class__ returns the class of the spec object. This allows mocks to pass isinstance tests.
spec_set: A stricter variant of spec. If used, attempting to set or get an attribute on the mock that isn’t on the object passed as spec_set will raise an AttributeError.
side_effect: A function to be called whenever the Mock is called. See the side_effect attribute. Useful for raising exceptions or dynamically changing return values. The function is called with the same arguments as the mock, and unless it returns DEFAULT, the return value of this function is used as the return value.
If side_effect is an iterable then each call to the mock will return the next value from the iterable. If any of the members of the iterable are exceptions they will be raised instead of returned.
return_value: The value returned when the mock is called. By default this is a new Mock (created on first access). See the return_value attribute.
wraps: Item for the mock object to wrap. If wraps is not None then calling the Mock will pass the call through to the wrapped object (returning the real result). Attribute access on the mock will return a Mock object that wraps the corresponding attribute of the wrapped object (so attempting to access an attribute that doesn’t exist will raise an AttributeError).
If the mock has an explicit return_value set then calls are not passed to the wrapped object and the return_value is returned instead.
name: If the mock has a name then it will be used in the repr of the mock. This can be useful for debugging. The name is propagated to child mocks.
Mocks can also be called with arbitrary keyword arguments. These will be used to set attributes on the mock after it is created.
espei.rstate module¶
espei.sublattice_tools module¶
Utilities for manipulating sublattice models.
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espei.sublattice_tools.
canonical_sort_key
(x)¶ Wrap strings in tuples so they’ll sort.
Parameters: x (list) – List of strings to sort Returns: tuple of strings that can be sorted Return type: tuple
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espei.sublattice_tools.
canonicalize
(configuration, equivalent_sublattices)¶ Sort a sequence with symmetry. This routine gives the sequence a deterministic ordering while respecting symmetry.
Parameters: - configuration ([str]) – Sublattice configuration to sort.
- equivalent_sublattices ({{int}}) – Indices of ‘configuration’ which should be equivalent by symmetry, i.e., [[0, 4], [1, 2, 3]] means permuting elements 0 and 4, or 1, 2 and 3, respectively, has no effect on the equivalence of the sequence.
Returns: sorted tuple that has been canonicalized.
Return type: str
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espei.sublattice_tools.
endmembers_from_interaction
(configuration)¶ For a given configuration with possible interactions, return all the endmembers
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espei.sublattice_tools.
generate_endmembers
(sublattice_model, symmetry=None)¶ Return all the unique endmembers by symmetry for a given sublattice model.
Parameters: - sublattice_model (list of lists) – General sublattice model, with each sublattice as a sublist.
- symmetry (list of lists, optional) – List of lists containing symmetrically equivalent sublattice indices. If None (default), all endmembers will be returned.
Returns: List of endmember tuples
Return type: list
Examples
>>> subl_model = [['A', 'B'], ['A','B']] >>> generate_endmembers(subl_model) # four endmembers [('A', 'A'), ('A', 'B'), ('B', 'A'), ('B', 'B')] >>> # three endmembers, ('A', 'B') is equivalent to ('B', 'A') by symmetry. >>> generate_endmembers(subl_model, [[0, 1]]) # the first and second sublattices are symmetrically equivalent. [('A', 'A'), ('A', 'B'), ('B', 'B')]
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espei.sublattice_tools.
generate_interactions
(endmembers, order, symmetry)¶ Returns a list of sorted interactions of a certain order
Parameters: - endmembers (list) – List of tuples/strings of all endmembers (including symmetrically equivalent)
- order (int) – Highest expected interaction order, e.g. ternary interactions should be 3
- symmetry (list of lists) – List of lists containing symmetrically equivalent sublattice indices, e.g. [[0, 1], [2, 3]] means that sublattices 0 and 1 are equivalent and sublattices 2 and 3 are also equivalent.
Returns: List of interaction tuples, e.g. [(‘A’, (‘A’, ‘B’))]
Return type: list
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espei.sublattice_tools.
generate_symmetric_group
(configuration, symmetry)¶ For a particular configuration and list of sublattices with symmetry, generate all the symmetrically equivalent configurations.
Parameters: - configuration (tuple) – Tuple of a sublattice configuration.
- symmetry (list of lists) – List of lists containing symmetrically equivalent sublattice indices, e.g. [[0, 1], [2, 3]] means that sublattices 0 and 1 are equivalent and sublattices 2 and 3 are also equivalent.
Returns: Tuple of configuration tuples that are all symmetrically equivalent.
Return type: tuple
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espei.sublattice_tools.
interaction_test
(configuration, order=None)¶ Returns True if the configuration has an interaction
Parameters: order (int, optional) – Specific order to check for. E.g. a value of 3 checks for ternary interactions Returns: True if there is an interaction. Return type: bool Examples
>>> configuration = [['A'], ['A','B']] >>> interaction_test(configuration) True >>> interaction_test(configuration, order=2) True >>> interaction_test(configuration, order=3) False
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espei.sublattice_tools.
recursive_tuplify
(x)¶ Recursively convert a nested list to a tuple
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espei.sublattice_tools.
sorted_interactions
(interactions, max_interaction_order, symmetry)¶ Return interactions sorted by interaction order
Parameters: - interactions (list) – List of tuples/strings of potential interactions
- max_interaction_order (int) – Highest expected interaction order, e.g. ternary interactions should be 3
- symmetry (list of lists) – List of lists containing symmetrically equivalent sublattice indices, e.g. [[0, 1], [2, 3]] means that sublattices 0 and 1 are equivalent and sublattices 2 and 3 are also equivalent.
Returns: Sorted list of interactions
Return type: list
Notes
Sort by number of full interactions, e.g. (A:A,B) is before (A,B:A,B) The goal is to return a sort key that can sort through multiple interaction orders, e.g. (A:A,B,C), which should be before (A,B:A,B,C), which should be before (A,B,C:A,B,C).
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espei.sublattice_tools.
tuplify
(x)¶ Convert a list to a tuple, or wrap an object in a tuple if it’s not a list or tuple.
espei.utils module¶
Utilities for ESPEI
Classes and functions defined here should have some reuse potential.
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espei.utils.
add_bibtex_to_bib_database
(bibtex, bib_db=None)¶ Add entries from a BibTeX file to the bibliography database
Parameters: - bibtex (str) – Either a multiline string, a path, or a file-like object of a BibTeX file
- bib_db (PickleableTinyDB) – Database to put the BibTeX entries. Defaults to a module-level default database
Returns: Return type: The modified bibliographic database
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espei.utils.
bib_marker_map
(bib_keys, markers=None)¶ Return a dict with reference keys and marker dicts
Parameters: - bib_keys –
- markers (list) – List of 2-tuples of (‘fillstyle’, ‘marker’) e.g. [(‘top’, ‘o’), (‘full’, ‘s’)]. Defaults to cycling through the filled markers, the different fill styles.
Returns: Dictionary with bib_keys as keys, dict values of formatted strings and marker dicts
Return type: dict
Examples
>>> mm = bib_marker_map(['otis2016', 'bocklund2018']) >>> mm == {'bocklund2018': {'formatted': 'bocklund2018', 'markers': {'fillstyle': 'none', 'marker': 'o'}}, 'otis2016': {'formatted': 'otis2016', 'markers': {'fillstyle': 'none', 'marker': 'v'}}} True
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espei.utils.
build_sitefractions
(phase_name, sublattice_configurations, sublattice_occupancies)¶ Convert nested lists of sublattice configurations and occupancies to a list of dictionaries. The dictionaries map SiteFraction symbols to occupancy values. Note that zero occupancy site fractions will need to be added separately since the total degrees of freedom aren’t known in this function.
Parameters: - phase_name (str) – Name of the phase
- sublattice_configurations ([[str]]) – sublattice configuration
- sublattice_occupancies ([[float]]) – occupancy of each sublattice
Returns: a list of site fractions over sublattices
Return type: [[float]]
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espei.utils.
database_symbols_to_fit
(dbf, symbol_regex='^V[V]?([0-9]+)$')¶ Return names of the symbols to fit that match the regular expression
Parameters: - dbf (Database) – pycalphad Database
- symbol_regex (str) – Regular expression of the fitting symbols. Defaults to V or VV followed by one or more numbers.
Returns: Return type: list
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espei.utils.
flexible_open_string
(obj)¶ Return the string of a an object that is either file-like, a file path, or the raw string.
Parameters: obj (string-like or file-like) – Either a multiline string, a path, or a file-like object Returns: Return type: str
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espei.utils.
formatted_constituent_array
(constituent_array)¶ Given a constituent array of Species, return the classic CALPHAD-style interaction.
Parameters: constituent_array (list) – List of sublattices, which are lists of Species in that sublattice Returns: String of the constituent array formatted in the classic CALPHAD style Return type: str Examples
>>> from pycalphad import variables as v >>> const_array = [[v.Species('CU'), v.Species('MG')], [v.Species('MG')]] >>> formatted_constituent_array(const_array) 'CU,MG:MG'
-
espei.utils.
formatted_parameter
(dbf, symbol, unique=True)¶ Get the deconstructed pretty parts of the parameter/term a symbol belongs to in a Database.
Parameters: - dbf (pycalphad.Database) –
- symbol (string or sympy.Symbol) – Symbol in the Database to get the parameter for.
- unique (bool) – If True, will raise if more than one parameter containing the symbol is found.
Returns: A named tuple with the following attributes:
phase_name
,interaction
,symbol
,term
,parameter_type
orterm_symbol
(which is just the Symbol * temperature term)Return type: FormattedParameter
-
espei.utils.
optimal_parameters
(trace_array, lnprob_array, kth=0)¶ Return the optimal parameters in the trace based on the highest likelihood. If kth is specified, return the kth set of unique optimal parameters.
Parameters: - trace_array (ndarray) – Array of shape (number of chains, iterations, number of parameters)
- lnprob_array (ndarray) – Array of shape (number of chains, iterations)
- kth (int) – Zero-indexed optimum. 0 (the default) is the most optimal solution. 1 is the second most optimal, etc.. Only unique solutions will be returned.
Returns: Return type: Array of optimal parameters
Notes
It is ok if the calculation did not finish and the arrays are padded with zeros. The number of chains and iterations in the trace and lnprob arrays must match.
-
espei.utils.
parameter_term
(expression, symbol)¶ Determine the term, e.g. T*log(T) that belongs to the symbol in expression
Parameters: - expression –
- symbol –
-
espei.utils.
sigfigs
(x, n)¶ Round x to n significant digits
Module contents¶
ESPEI
Contributing to ESPEI¶
This is the place to start as a new ESPEI contributor.
The next sections lay out the basics of getting an ESPEI development set up and the development standards. Then the Software design sections walk through the key parts of the codebase.
Installing in develop mode¶
It is suggested to use ESPEI in development mode if you will be contributing features to the source code. As usual, you should install ESPEI into a virtual environment.
All of the dependencies can be installed either by conda or pip.
Then clone the source and install ESPEI in development mode with pip:
git clone https://github.com/PhasesResearchLab/espei.git
pip install --editable espei
Even if you use Anaconda, it is recommended that you use either pip
or python setup.py develop
to install ESPEI in development mode.
This is because the conda-build
tool, which would typically be used for this, is not well maintained at the time of writing.
Develop mode on Windows¶
Because of compiler issues, ESPEI’s dependencies are challenging to install on Windows.
As mentioned above, ideally the conda-build
tool could be used, but it is not able to be used.
Therefore the recommended way to install ESPEI is to
- Install ESPEI into a virtual environment from Anaconda, pulling all of the packages with it
- Remove ESPEI without removing the other packages
- Install ESPEI in develop mode with pip or setuptools from the source repository
The steps to do this on the command line are as follows
conda create -n espei_dev espei
activate espei_dev
conda remove --force espei
git clone https://github.com/PhasesResearchLab/espei.git
pip install --editable espei
Tests¶
Even though much of ESPEI is devoted to being a multi-core, stochastic user tool, we strive to test all logic and functionality. We are continuously maintaining tests and writing tests for previously untested code.
As a general rule, any time you write a new function or modify an existing function you should write or maintain a test for that function.
ESPEI uses pytest as a test runner.
Some tips for testing:
- Ideally you would practicing test driven development by writing tests of your intended results before you write the function.
- If possible, keep the tests small and fast. If you do have a long running tests (longer than ~15 second run time) mark the test with the
@pytest.mark.slow
decorator. - See the NumPy/SciPy testing guidelines for more tips
Style¶
Code style¶
For most naming and style, follow PEP8. One exception to PEP8 is regarding the line length, which we suggest a 120 character maximum, but may be longer within reason.
Code documentation¶
ESPEI uses the NumPy documentation style. All functions and classes should be documented with at least a description, parameters, and return values, if applicable.
Using Examples
in the documentation is especially encouraged for utilities that are likely to be run by users.
See espei.plot.multiplot()
for an example.
If you add any new external (non-ESPEI) imports in any code, they must be added to the MOCK_MODULES
list in docs/conf.py
.
Web documention¶
Documentation on ESPEI is split into user tutorials, reference and developer documentation.
- Tutorials are resources for users new to ESPEI or new to certain features of ESPEI to be guided through typical actions.
- Reference pages should be concise articles that explain how to complete specific goals for users who know what they want to accomplish.
- Developer documentation should describe what should be considered when contributing source code back to ESPEI.
You can check changes you make to the documentation by going to the documentation folder in the root repository cd docs/
.
Running the command make html && cd build/html && python3 -m http.server && cd ../.. && make clean
from that folder will build the docs and run them on a local HTTP server.
You can see the documentation when the server is running by
visting the URL at the end of the output, usually localhost port 8000 <http://0.0.0.0:8000>``_.
When you are finished, type ``Ctrl-C
to stop the server and the command will clean up the build for you.
Make sure to fix any warnings that come up if you are adding documentation.
Logging¶
Since ESPEI is intended to be run by users, we must provide useful feedback on how their runs are progressing. ESPEI uses the logging module to allow control over verbosity of the output.
There are 5 different logging levels provided by Python. They should be used as follows:
- Critical or Error (
logging.critical
orlogging.error
) - Never use these. These log levels would only be used when there is an unrecoverable error that requires the run to be stopped.
In that case, it is better to
raise
an appropriate error instead. - Warning (
logging.warning
) - Warnings are best used when we are able to recover from something bad that has happened. The warning should inform the user about potentially incorrect results or let them know about something they have the potential to fix. Again, anything unrecoverable should not be logged and should instead be raised with a good error message.
- Info (
logging.info
) - Info logging should report on the progress of the program. Usually info should give feedback on milestones of a run or on actions that were taken as a result of a user setting. An example of a milestone is starting and finishing parameter generation. An example of an action taken as a result of a user setting is the logging of the number of chains in an mcmc run.
- Debug (
logging.debug
) - Debugging is the lowest level of logging we provide in ESPEI. Debug messages should consist of possibly useful information that is beyond the user’s direct control. Examples are the values of initial parameters, progress of checking datasets and building phase models, and the acceptance ratios of MCMC iterations.
Software design¶
The following sections elaborate on the design principles on the software side. The goal is to make it clear how different modules in ESPEI fit together and where to find specific functionality to override or improve.
ESPEI provides tools to
- Parameterize CALPHAD models by optimizing the compromise between model accuracy and complexity. We typically call this parameter generation or model selection.
- Fit parameterized CALPHAD models to multi-phase or other custom data with uncertainty quantification via Markov chain Monte Carlo
API¶
ESPEI has two levels of API that users should expect to interact with:
- Input from YAML files on the command line (via
espei --input <input_file>
or by Python via theespei.espei_script.run_espei
function - Work directly with the Python functions for parameter selection
espei.paramselect.generate_parameters
and MCMCespei.mcmc.mcmc_fit
YAML files are the recommended way to use ESPEI and should have a way to express most if not all of the options that
the Python functions support. The schema for YAML files is located in the root of the ESPEI directory as input-schema.yaml
and is validated in the espei_script.py
module by the Cerberus package.
Module Hierarchy¶
espei_script.py
is the main entry point for the YAML input API.paramselect.py
is where parameter generation happens.mcmc.py
creates the likelihood function and runs MCMC.error_functions
is a package with modules for each type of likelihood function.parameter_selection
is a package with core pieces of parameter selection.utils.py
are utilities with reuse potential across several parts of ESPEI.plot.py
holds plotting functions.datasets.py
manages validating and loading datasets into a TinyDB in memory database.core_utils.py
are legacy utility functions that should be refactored out to be closer to individual modules and packages where they are used.
Parameter selection¶
Parameter selection goes through the generate_parameters
function in the espei.paramselect
module.
The goal of parameter selection is go through each phase (one at a time) and fit a CALPHAD model to the data.
For each phase, the endmembers are fit first, followed by binary and ternary interactions. For each individual endmember or interaction to fit, a series of candidate models are generated that have increasing complexity in both temperature and interaction order (an L0 excess parameter, L0 and L1, …).
Each model is then fit by espei.parameter_selection.selection.fit_model
, which currently uses a simple
pseudo-inverse linear model from scikit-learn. Then the tradeoff between the goodness of fit and the model complexity
is scored by the AICc (see Theory) in espei.parameter_selection.selection.score_model
.
The optimal scoring model is accepted as the model with the fit model parameters set as degrees of freedom for the MCMC step.
The main principle is that ESPEI transforms the data and candidate models to vectors and matricies that fit a typical machine learning type problem of \(Ax = b\). Extending ESPEI to use different or custom models in the current scheme basically comes down to formulating candidate models in terms of this type of problem. The main ways to improve on the fitting or scoring methods used in parameter selection is to override the fit and score functions.
Currently the capabilities for providing custom models or contributions (e.g. magnetic data) in the form of generic pycalphad Model objects are limited. This is also true for custom types of data that one would use in fitting a custom model.
MCMC optimization and uncertainty quantification¶
Most of the Markov chain Monte Carlo optimization and uncertainty quantification happen in the espei.mcmc
module through the espei.mcmc.mcmc_fit
function.
The main reason ESPEI’s parameter selection and MCMC routines are split up is that custom Models or existing TDB files can be provided and fit. In other words, if you are using a model that doesn’t need parameter selection or is for a property that is not Gibbs energy, MCMC can fit it with uncertainty quantification.
The general process is
- Take a database with degrees of freedom as database symbols named
VV####
, where####
is a number, e.g.0001
. The symbols correspond toFUNCTION
in the TDB files. - Initialize those degrees of freedom to a starting distribution for ensemble MCMC (see Theory).
The starting distribution is controlled by the
espei.mcmc.generate_parameter_distribution
function, which currently supports initializing the parameters to a Gaussian ball. - Use the emcee package to run ensemble MCMC
ESPEI’s MCMC is quite flexible for customization. To fit a custom model, it just needs to be read by pycalphad and
have correctly named degrees of freedom (VV####
).
To fit an existing or custom model to new types of data, just write a function that takes in datasets and the parameters
that are required to calculate the values (e.g. pycalphad Database, components, phases, …) and returns the error.
Then override the espei.mcmc.lnprob
function to include your custom error contribution.
There are examples of these functions espei.error_functions
that ESPEI uses by default.
In addition, custom starting distributions can be obtained by overriding espei.mcmc.generate_parameter_distribution
.
Getting Help¶
For help on installing and using ESPEI, please join the PhasesResearchLab/ESPEI Gitter room.
Bugs and software issues should be reported on GitHub.
License¶
ESPEI is MIT licensed.
The MIT License (MIT)
Copyright (c) 2015-2018 Richard Otis
Copyright (c) 2017-2018 Brandon Bocklund
Permission is hereby granted, free of charge, to any person obtaining a copy
of this software and associated documentation files (the "Software"), to deal
in the Software without restriction, including without limitation the rights
to use, copy, modify, merge, publish, distribute, sublicense, and/or sell
copies of the Software, and to permit persons to whom the Software is
furnished to do so, subject to the following conditions:
The above copyright notice and this permission notice shall be included in all
copies or substantial portions of the Software.
THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR
IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY,
FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE
AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER
LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM,
OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN THE
SOFTWARE.
Citing ESPEI¶
A publication is in preparation. For now, ESPEI can be cited via the following publication:
R.A. Otis, Z.-K. Liu, High-Throughput Thermodynamic Modeling and Uncertainty Quantification for ICME, JOM. 69 (2017) 886–892. doi:10.1007/s11837-017-2318-6.