PyEMD computes the Earth Mover's Distance (Wasserstein distance) between histograms using NumPy.
PyEMD was originally a Python wrapper for Ofir Pele and Michael Werman's C++ implementation of the Earth Mover's Distance.
As of version 1.1, PyEMD uses POT (Python Optimal Transport) as its default backend. POT is a well-maintained, actively developed library that provides faster performance and multi-threading support.
PyEMD is now maintained primarily as a stable wrapper around POT for projects that depend on PyEMD's API. For new projects, consider using POT directly, which offers a broader range of optimal transport functionality.
The original C++ implementation remains available via the backend='cpp'
option for backward compatibility and validation.
>>> from pyemd import emd
>>> import numpy as np
>>> first_histogram = np.array([0.0, 1.0])
>>> second_histogram = np.array([5.0, 3.0])
>>> distance_matrix = np.array([[0.0, 0.5],
... [0.5, 0.0]])
>>> emd(first_histogram, second_histogram, distance_matrix)
3.5You can also get the associated minimum-cost flow:
>>> from pyemd import emd_with_flow
>>> emd_with_flow(first_histogram, second_histogram, distance_matrix)
(3.5, [[0.0, 0.0], [0.0, 1.0]])You can also calculate the EMD directly from two arrays of observations:
>>> from pyemd import emd_samples
>>> first_array = [1, 2, 3, 4]
>>> second_array = [2, 3, 4, 5]
>>> emd_samples(first_array, second_array, bins=2)
0.5PyEMD supports two computation backends:
'pot'(default): Uses the POT (Python Optimal Transport) library. Faster and supports multi-threading.'cpp': Uses the original C++ implementation by Ofir Pele and Michael Werman. Kept for backward compatibility.
You can select the backend using the backend parameter:
>>> emd(first_histogram, second_histogram, distance_matrix, backend='pot') # default
3.5
>>> emd(first_histogram, second_histogram, distance_matrix, backend='cpp')
3.5Both backends produce equivalent results (within floating-point precision).
emd(first_histogram,
second_histogram,
distance_matrix,
extra_mass_penalty=-1.0,
backend='pot')Arguments:
first_histogram(np.ndarray): A 1D array of typenp.float64of length N.second_histogram(np.ndarray): A 1D array ofnp.float64of length N.distance_matrix(np.ndarray): A 2D array ofnp.float64,of size at least N × N. This defines the underlying metric, or ground distance, by giving the pairwise distances between the histogram bins. NOTE: It must represent a metric; there is no warning if it doesn't.
Keyword Arguments:
extra_mass_penalty(float): The penalty for extra mass. If you want the resulting distance to be a metric, it should be at least half the diameter of the space (maximum possible distance between any two points). If you want partial matching you can set it to zero (but then the resulting distance is not guaranteed to be a metric). The default value is-1.0, which means the maximum value in the distance matrix is used.backend(str): The computation backend to use. Options are'pot'(default) or'cpp'.
Returns: (float) The EMD value.
emd_with_flow(first_histogram,
second_histogram,
distance_matrix,
extra_mass_penalty=-1.0,
backend='pot')Arguments are the same as for emd().
Returns: (tuple(float, list(list(float)))) The EMD value and the associated minimum-cost flow.
emd_samples(first_array,
second_array,
extra_mass_penalty=-1.0,
distance='euclidean',
normalized=True,
bins='auto',
range=None,
backend='pot')Arguments:
first_array(Iterable): An array of samples used to generate a histogram.second_array(Iterable): An array of samples used to generate a histogram.
Keyword Arguments:
extra_mass_penalty(float): Same as foremd().distance(string or function): A string or function implementing a metric on a 1Dnp.ndarray. Defaults to the Euclidean distance. Currently limited to 'euclidean' or your own function, which must take a 1D array and return a square 2D array of pairwise distances.normalized(boolean): If true (default), treat histograms as fractions of the dataset. If false, treat histograms as counts. In the latter case the EMD will vary greatly by array length.bins(int or string): The number of bins to include in the generated histogram. If a string, must be one of the bin selection algorithms accepted bynp.histogram(). Defaults to'auto', which gives the maximum of the 'sturges' and 'fd' estimators.range(tuple(int, int)): The lower and upper range of the bins, passed tonumpy.histogram(). Defaults to the range of the union offirst_arrayandsecond_array. Note: if the given range is not a superset of the default range, no warning will be given.backend(str): The computation backend to use. Options are'pot'(default) or'cpp'.
Returns: (float) The EMD value between the histograms of first_array
and second_array.
This project uses uv for dependency management and meson-python as the build backend.
Quick start:
# Install uv (if not already installed) curl -LsSf https://astral.sh/uv/install.sh | sh # Clone and setup git clone https://github.com/wmayner/pyemd.git cd pyemd uv sync --all-extras # Build package uv build
Note: For development workflows, see the DEVELOPING.md file in the repository.
Dependencies are locked in uv.lock for reproducibility.
emd()andemd_with_flow():- The
distance_matrixis assumed to represent a metric; there is no check to ensure that this is true. See the documentation inpyemd/lib/emd_hat.hppfor more information. - The histograms and distance matrix must be numpy arrays of type
np.float64.
- The
emd_with_flow():- The flow matrix does not contain the flows to/from the extra mass bin.
- The POT backend uses the POT (Python Optimal Transport) library by Rémi Flamary et al.
- The C++ backend uses the implementation by Ofir Pele and Michael Werman. See the relevant paper.
- Thanks to the Cython developers for making the C++ wrapper relatively easy to write.
If you use this code, please cite the POT library:
Rémi Flamary et al. POT: Python Optimal Transport. Journal of Machine Learning Research, 22(78):1-8, 2021.
@article{flamary2021pot,
title={POT: Python Optimal Transport},
author={Flamary, R{\'e}mi and Courty, Nicolas and Gramfort, Alexandre and
Alaya, Mokhtar Z. and Boisbunon, Aur{\'e}lie and Chambon, Stanislas and
Chapel, Laetitia and Corenflos, Adrien and Fatras, Kilian and
Fournier, Nemo and Gautheron, L{\'e}o and Gayraud, Nathalie T.H. and
Janati, Hicham and Rakotomamonjy, Alain and Redko, Ievgen and
Rolet, Antoine and Schutz, Antony and Seguy, Vivien and
Sutherland, Danica J. and Tavenard, Romain and Tong, Alexander and
Vayer, Titouan},
journal={Journal of Machine Learning Research},
volume={22},
number={78},
pages={1--8},
year={2021}
}If you use the C++ backend (backend='cpp'), please also cite the original
implementation:
Ofir Pele and Michael Werman. Fast and robust earth mover's distances. Proc. 2009 IEEE 12th Int. Conf. on Computer Vision, Kyoto, Japan, 2009, pp. 460-467.
@INPROCEEDINGS{pele2009,
title={Fast and robust earth mover's distances},
author={Pele, Ofir and Werman, Michael},
booktitle={2009 IEEE 12th International Conference on Computer Vision},
pages={460--467},
year={2009},
month={September},
organization={IEEE}
}Ofir Pele and Michael Werman. A linear time histogram metric for improved SIFT matching. Computer Vision - ECCV 2008, Marseille, France, 2008, pp. 495-508.
@INPROCEEDINGS{pele2008,
title={A linear time histogram metric for improved sift matching},
author={Pele, Ofir and Werman, Michael},
booktitle={Computer Vision--ECCV 2008},
pages={495--508},
year={2008},
month={October},
publisher={Springer}
}