Source code for pyesmda.esmda_rs

"""
Implement the ES-MDA-RS algorithms.

@author: acollet
"""
from typing import Any, Callable, Dict, List, Optional, Sequence, Union

import numpy as np
import numpy.typing as npt
from scipy.sparse import spmatrix

from pyesmda.esmda import ESMDABase
from pyesmda.utils import (
    NDArrayFloat,
    approximate_covariance_matrix_from_ensembles,
    compute_ensemble_average_normalized_objective_function,
    get_ensemble_variance,
    inflate_ensemble_around_its_mean,
)

# pylint: disable=C0103 # Does not conform to snake_case naming style


[docs]class ESMDA_RS(ESMDABase): r""" Restricted Step Ensemble Smoother with Multiple Data Assimilation. Implement an adaptative version of the original ES-MDA algorithm proposed by Emerick, A. A. and A. C. Reynolds :cite:p:`emerickEnsembleSmootherMultiple2013, emerickHistoryMatchingProductionSeismic2013`. This adaptative version introduced by :cite:p:`leAdaptiveEnsembleSmoother2016` provides an automatic procedure for choosing the inflation factor for the next data-assimilation step adaptively as the history match proceeds. The procedure also decides when to stop, i.e. the number of assimilation, which is no longer a user input. Attributes ---------- d_dim : int Number of observation values :math:`N_{obs}`, and consequently of predicted values. obs : npt.NDArray[np.float64] Obsevrations vector with dimensions (:math:`N_{obs}`). cov_obs: npt.NDArray[np.float64] Covariance matrix of observed data measurement errors with dimensions (:math:`N_{obs}`, :math:`N_{obs}`). Also denoted :math:`R`. std_m_prior: npt.NDArray[np.float64] Vector of a priori standard deviation :math:`sigma` of the estimated parameter. The expected dimension is (:math:`N_{m}`). It is the diagonal of :math:`C_{M}`. d_obs_uc: npt.NDArray[np.float64] Vectors of pertubed observations with dimension (:math:`N_{e}`, :math:`N_{obs}`). d_pred: npt.NDArray[np.float64] Vectors of predicted values (one for each ensemble member) with dimensions (:math:`N_{e}`, :math:`N_{obs}`). d_history: List[npt.NDArray[np.float64]] List of vectors of predicted values obtained at each assimilation step. m_prior: Vectors of parameter values (one vector for each ensemble member) used in the last assimilation step. Dimensions are (:math:`N_{e}`, :math:`N_{m}`). m_bounds : npt.NDArray[np.float64] Lower and upper bounds for the :math:`N_{m}` parameter values. Expected dimensions are (:math:`N_{m}`, 2) with lower bounds on the first column and upper on the second one. m_history: List[npt.NDArray[np.float64]] List of successive `m_prior`. cov_md: npt.NDArray[np.float64] Cross-covariance matrix between the forecast state vector and predicted data. Dimensions are (:math:`N_{m}, N_{obs}`). cov_dd: npt.NDArray[np.float64] Autocovariance matrix of predicted data. Dimensions are (:math:`N_{obs}, N_{obs}`). cov_mm: npt.NDArray[np.float64] Autocovariance matrix of estimated parameters. Dimensions are (:math:`N_{m}, N_{m}`). forward_model: callable Function calling the non-linear observation model (forward model) for all ensemble members and returning the predicted data for each ensemble member. forward_model_args: Tuple[Any] Additional args for the callable forward_model. forward_model_kwargs: Dict[str, Any] Additional kwargs for the callable forward_model. n_assimilations : int Number of data assimilations (:math:`N_{a}`) performed. Automatically determined. Initially at 0. cov_mm_initial_inflation_factor: float List of factors used to inflate the adjusted parameters covariance among iterations: Each realization of the ensemble at the end of each update step i, is linearly inflated around its mean. See :cite:p:`andersonExploringNeedLocalization2007`. dd_correlation_matrix : Optional[csr_matrix] Correlation matrix based on spatial and temporal distances between observations and observations :math:`\rho_{DD}`. It is used to localize the autocovariance matrix of predicted data by applying an elementwise multiplication by this matrix. Expected dimensions are (:math:`N_{obs}`, :math:`N_{obs}`). md_correlation_matrix : Optional[spmatrix] Correlation matrix based on spatial and temporal distances between parameters and observations :math:`\rho_{MD}`. It is used to localize the cross-covariance matrix between the forecast state vector (parameters) and predicted data by applying an elementwise multiplication by this matrix. Expected dimensions are (:math:`N_{m}`, :math:`N_{obs}`). save_ensembles_history: bool Whether to save the history predictions and parameters over the assimilations. rng: np.random.Generator The random number generator used in the predictions perturbation step. is_forecast_for_last_assimilation: bool Whether to compute the predictions for the ensemble obtained at the last assimilation step. batch_size: int Number of parameters that are assimilated at once. This option is available to overcome memory limitations when the number of parameters is large. In that case, the size of the covariance matrices tends to explode and the update step must be performed by chunks of parameters. is_parallel_analyse_step: bool, optional Whether to use parallel computing for the analyse step if the number of batch is above one. The default is True. n_batches: int Number of batches required during the update step. """ # pylint: disable=R0902 # Too many instance attributes __slots__: List[str] = ["std_m_prior", "_cov_obs_inflation_factors"]
[docs] def __init__( self, obs: npt.NDArray[np.float64], m_init: npt.NDArray[np.float64], cov_obs: npt.NDArray[np.float64], forward_model: Callable[..., npt.NDArray[np.float64]], forward_model_args: Sequence[Any] = (), forward_model_kwargs: Optional[Dict[str, Any]] = None, std_m_prior: Optional[npt.NDArray[np.float64]] = None, cov_mm_inflation_factor: float = 1.0, dd_correlation_matrix: Optional[Union[NDArrayFloat, spmatrix]] = None, md_correlation_matrix: Optional[Union[NDArrayFloat, spmatrix]] = None, m_bounds: Optional[npt.NDArray[np.float64]] = None, save_ensembles_history: bool = False, seed: Optional[int] = None, is_forecast_for_last_assimilation: bool = True, random_state: Optional[ Union[int, np.random.Generator, np.random.RandomState] ] = 198873, batch_size: int = 5000, is_parallel_analyse_step: bool = True, ) -> None: # pylint: disable=R0913 # Too many arguments # pylint: disable=R0914 # Too many local variables r"""Construct the instance. Parameters ---------- obs : npt.NDArray[np.float64] Obsevrations vector with dimension :math:`N_{obs}`. m_init : npt.NDArray[np.float64] Initial ensemble of parameters vector with dimensions (:math:`N_{e}`, :math:`N_{m}`). cov_obs: npt.NDArray[np.float64] Covariance matrix of observed data measurement errors with dimensions (:math:`N_{obs}`, :math:`N_{obs}`). Also denoted :math:`R`. forward_model: callable Function calling the non-linear observation model (forward model) for all ensemble members and returning the predicted data for each ensemble member. forward_model_args: Optional[Tuple[Any]] Additional args for the callable forward_model. The default is None. forward_model_kwargs: Optional[Dict[str, Any]] Additional kwargs for the callable forward_model. The default is None. std_m_prior: Optional[npt.NDArray[np.float64]] Vector of a priori standard deviation :math:`sigma` of the estimated parameter. The expected dimension is (:math:`N_{m}`). It is the diagonal of :math:`C_{M}`. If not provided, then it is inffered from the inflated initial ensemble (see `cov_mm_inflation_factor`). The default is None. cov_mm_inflation_factor: float Factor used to inflate the initial ensemble variance around its mean. See :cite:p:`andersonExploringNeedLocalization2007`. The default is 1.0, which means no inflation. dd_correlation_matrix : Optional[Union[NDArrayFloat, spmatrix]] Correlation matrix based on spatial and temporal distances between observations and observations :math:`\rho_{DD}`. It is used to localize the autocovariance matrix of predicted data by applying an elementwise multiplication by this matrix. Expected dimensions are (:math:`N_{obs}`, :math:`N_{obs}`). The default is None. md_correlation_matrix : Optional[Union[NDArrayFloat, spmatrix]] Correlation matrix based on spatial and temporal distances between parameters and observations :math:`\rho_{MD}`. It is used to localize the cross-covariance matrix between the forecast state vector (parameters) and predicted data by applying an elementwise multiplication by this matrix. Expected dimensions are (:math:`N_{m}`, :math:`N_{obs}`). The default is None. m_bounds : Optional[NDArrayFloat], optional Lower and upper bounds for the :math:`N_{m}` parameter values. Expected dimensions are (:math:`N_{m}`, 2) with lower bounds on the first column and upper on the second one. The default is None. save_ensembles_history: bool, optional Whether to save the history predictions and parameters over the assimilations. The default is False. seed: Optional[int] .. deprecated:: 0.4.2 Since 0.4.2, you can use the parameter `random_state` instead. is_forecast_for_last_assimilation: bool, optional Whether to compute the predictions for the ensemble obtained at the last assimilation step. The default is True. random_state: Optional[Union[int, np.random.Generator, np.random.RandomState]] Pseudorandom number generator state used to generate resamples. If `random_state` is ``None`` (or `np.random`), the `numpy.random.RandomState` singleton is used. If `random_state` is an int, a new ``RandomState`` instance is used, seeded with `random_state`. If `random_state` is already a ``Generator`` or ``RandomState`` instance then that instance is used. batch_size: int Number of parameters that are assimilated at once. This option is available to overcome memory limitations when the number of parameters is large. In that case, the size of the covariance matrices tends to explode and the update step must be performed by chunks of parameters. The default is 5000. is_parallel_analyse_step: bool, optional Whether to use parallel computing for the analyse step if the number of batch is above one. It relies on `concurrent.futures` multiprocessing. The default is True. """ super().__init__( obs=obs, # only inflate the initial ensemble because we don't known # the number of assimilations m_init=inflate_ensemble_around_its_mean( m_init, inflation_factor=cov_mm_inflation_factor ), cov_obs=cov_obs, forward_model=forward_model, forward_model_args=forward_model_args, forward_model_kwargs=forward_model_kwargs, n_assimilations=1, # in esmda-rs this number is determined automatically dd_correlation_matrix=dd_correlation_matrix, md_correlation_matrix=md_correlation_matrix, # cov_mm_inflation_factors=None, # [cov_mm_inflation_factor], m_bounds=m_bounds, save_ensembles_history=save_ensembles_history, seed=seed, is_forecast_for_last_assimilation=is_forecast_for_last_assimilation, random_state=random_state, batch_size=batch_size, is_parallel_analyse_step=is_parallel_analyse_step, ) # Initialize an empty list self.cov_obs_inflation_factors = [] # I am still wondering whether this should remain constant of if it should be # updated at each iteration ? I still have a doubt. I asked the authors of the # paper and I am still waiting for the answer if std_m_prior is not None: # in that case the user impose the ensemble variance self.std_m_prior: npt.NDArray[np.float64] = std_m_prior else: # otherwise, it is inffered from the inflated ensemble self.std_m_prior: npt.NDArray[np.float64] = np.sqrt( get_ensemble_variance(self.m_prior) )
@property def n_assimilations(self) -> int: """Get the number of assimilations performed. Read-only.""" return self._assimilation_step @property def cov_obs_inflation_factors(self) -> List[float]: r""" Get the inlfation factors for the covariance matrix of the measurement errors. Single and multiple data assimilation are equivalent for the linear-Gaussian case as long as the factor :math:`\alpha_{l}` used to inflate the covariance matrix of the measurement errors satisfy the following condition: .. math:: \sum_{l=1}^{N_{a}} \frac{1}{\alpha_{l}} = 1 In practise, :math:`\alpha_{l} = N_{a}` is a good choice :cite:p:`emerickEnsembleSmootherMultiple2013`. """ return self._cov_obs_inflation_factors @cov_obs_inflation_factors.setter def cov_obs_inflation_factors(self, a: List[float]) -> None: """Set the inflation factors the covariance matrix of the measurement errors.""" self._cov_obs_inflation_factors = a
[docs] def solve(self) -> None: """Solve the optimization problem with ES-MDA-RS algorithm.""" if self.save_ensembles_history: self.m_history.append(self.m_prior) # save m_init current_inflation_factor: float = 10.0 # to initiate the while m_pred = self.m_prior while not self._is_unity_reached(current_inflation_factor): self._assimilation_step += 1 print(f"Assimilation # {self._assimilation_step}") self._forecast() # Divide per 2, because it is multiplied by 2 as the beginning # of the second while loop current_inflation_factor: float = ( self._compute_initial_inflation_factor() / 2 ) is_valid_parameter_change: bool = False while not is_valid_parameter_change: current_inflation_factor *= 2 # double the inflation (dumping) factor self._pertrub(current_inflation_factor) if self.n_batches == 1: self._approximate_covariance_matrices() m_pred = self._apply_bounds(self._analyse(current_inflation_factor)) else: # covariance approximation dd self.cov_dd = approximate_covariance_matrix_from_ensembles( self.d_pred, self.d_pred ) # Spatial and temporal localization: obs - obs if self.dd_correlation_matrix is not None: self.cov_dd = self.dd_correlation_matrix.multiply( self.cov_dd ).toarray() # Update the prior parameter for next iteration m_pred = self._apply_bounds( self._local_analyse(current_inflation_factor) ) is_valid_parameter_change: bool = self._is_valid_parameter_change( m_pred ) # If the criteria is reached -> Get exactly one for the sum if self._is_unity_reached(current_inflation_factor): current_inflation_factor = 1 / ( 1 - np.sum([1 / a for a in self.cov_obs_inflation_factors]) ) self._pertrub(current_inflation_factor) self._approximate_covariance_matrices() m_pred = self._analyse(current_inflation_factor) is_valid_parameter_change: bool = self._is_valid_parameter_change( m_pred ) self.cov_obs_inflation_factors.append(current_inflation_factor) print(f"- Inflation factor = {current_inflation_factor:.3f}") # Update the prior parameter for next iteration self.m_prior = m_pred # Saving the parameters history if self.save_ensembles_history: self.m_history.append(m_pred) # Last assimilation if self.is_forecast_for_last_assimilation: self._forecast()
[docs] def _compute_initial_inflation_factor(self) -> float: r"""Compute the :math:`\alpha_{l}` inflation (dumping) factor.""" return 0.25 * compute_ensemble_average_normalized_objective_function( self.d_pred, self.obs, self.cov_obs )
[docs] def _is_unity_reached(self, current_inflation_factor: float) -> bool: """ Whether the sum of the inverse inflation factors is above one. It includes all factors up to the current iteration. Parameters ---------- current_inflation_factor: float Multiplication factor used to inflate the covariance matrix of the measurement errors for the current (last) iteration. """ return ( np.sum([1 / a for a in self.cov_obs_inflation_factors]) + 1 / current_inflation_factor >= 1 )
[docs] def _is_valid_parameter_change(self, m_pred: npt.NDArray[np.float64]) -> bool: """Check if all change residuals are below 2 sigma. Parameters ---------- m_pred : npt.NDArray[np.float64] _description_ Returns ------- bool _description_ """ def is_lower(residuals) -> bool: return np.all(residuals < 2 * self.std_m_prior) return np.all(list(map(is_lower, np.abs(m_pred - self.m_prior))))