Source code for harmonica.forward.prism

# Copyright (c) 2018 The Harmonica Developers.
# Distributed under the terms of the BSD 3-Clause License.
# SPDX-License-Identifier: BSD-3-Clause
#
# This code is part of the Fatiando a Terra project (https://www.fatiando.org)
#
"""
Forward modelling for prisms
"""
import numpy as np
from numba import jit, prange

from ..constants import GRAVITATIONAL_CONST


[docs]def prism_gravity( coordinates, prisms, density, field, parallel=True, dtype="float64", disable_checks=False, ): """ Gravitational fields of right-rectangular prisms in Cartesian coordinates The gravitational fields are computed through the analytical solutions given by [Nagy2000]_ and [Nagy2002]_, which are valid on the entire domain. This means that the computation can be done at any point, either outside or inside the prism. This implementation makes use of the modified arctangent function proposed by [Fukushima2019]_ (eq. 12) so that the potential field to satisfies Poisson's equation in the entire domain. Moreover, the logarithm function was also modified in order to solve the singularities that the analytical solution has on some points (see [Nagy2000]_). .. warning:: The **z direction points upwards**, i.e. positive and negative values of ``upward`` represent points above and below the surface, respectively. But remember that the ``g_z`` field returns the downward component of the gravitational acceleration so that positive density contrasts produce positive anomalies. Parameters ---------- coordinates : list or 1d-array List or array containing ``easting``, ``northing`` and ``upward`` of the computation points defined on a Cartesian coordinate system. All coordinates should be in meters. prisms : list, 1d-array, or 2d-array List or array containing the coordinates of the prism(s) in the following order: west, east, south, north, bottom, top in a Cartesian coordinate system. All coordinates should be in meters. Coordinates for more than one prism can be provided. In this case, *prisms* should be a list of lists or 2d-array (with one prism per line). density : list or array List or array containing the density of each prism in kg/m^3. field : str Gravitational field that wants to be computed. The available fields are: - Gravitational potential: ``potential`` - Downward acceleration: ``g_z`` parallel : bool (optional) If True the computations will run in parallel using Numba built-in parallelization. If False, the forward model will run on a single core. Might be useful to disable parallelization if the forward model is run by an already parallelized workflow. Default to True. dtype : data-type (optional) Data type assigned to the resulting gravitational field. Default to ``np.float64``. disable_checks : bool (optional) Flag that controls whether to perform a sanity check on the model. Should be set to ``True`` only when it is certain that the input model is valid and it does not need to be checked. Default to ``False``. Returns ------- result : array Gravitational field generated by the prisms on the computation points. Examples -------- Compute gravitational effect of a single a prism >>> # Define prisms boundaries, it must be beneath the surface >>> prism = [-34, 5, -18, 14, -345, -146] >>> # Set prism density to 2670 kg/m³ >>> density = 2670 >>> # Define a computation point above its center, at 30 meters above the >>> # surface >>> coordinates = (130, 75, 30) >>> # Define three computation points along the easting axe at 30m above >>> # the surface >>> coordinates = ([-40, 0, 40], [0, 0, 0], [30, 30, 30]) >>> # Compute the downward component of the gravitational acceleration that >>> # the prism generates on the computation points >>> gz = prism_gravity(coordinates, prism, density, field="g_z") >>> print("({:.5f}, {:.5f}, {:.5f})".format(*gz)) (0.06551, 0.06628, 0.06173) Define two prisms with positive and negative density contrasts >>> prisms = [[-134, -5, -45, 45, -200, -50], [5, 134, -45, 45, -180, -30]] >>> densities = [-300, 300] >>> # Compute the g_z that the prisms generate on the computation points >>> gz = prism_gravity(coordinates, prisms, densities, field="g_z") >>> print("({:.5f}, {:.5f}, {:.5f})".format(*gz)) (-0.05379, 0.02908, 0.11235) """ kernels = {"potential": kernel_potential, "g_z": kernel_g_z} if field not in kernels: raise ValueError("Gravitational field {} not recognized".format(field)) # Figure out the shape and size of the output array cast = np.broadcast(*coordinates[:3]) result = np.zeros(cast.size, dtype=dtype) # Convert coordinates, prisms and density to arrays with proper shape coordinates = tuple(np.atleast_1d(i).ravel() for i in coordinates[:3]) prisms = np.atleast_2d(prisms) density = np.atleast_1d(density).ravel() # Sanity checks if not disable_checks: if density.size != prisms.shape[0]: raise ValueError( "Number of elements in density ({}) ".format(density.size) + "mismatch the number of prisms ({})".format(prisms.shape[0]) ) _check_prisms(prisms) # Compute gravitational field dispatcher(parallel)(coordinates, prisms, density, kernels[field], result) result *= GRAVITATIONAL_CONST # Convert to more convenient units if field == "g_z": result *= 1e5 # SI to mGal return result.reshape(cast.shape)
def dispatcher(parallel): """ Return the parallelized or serialized forward modelling function """ dispatchers = { True: jit_prism_gravity_parallel, False: jit_prism_gravity_serial, } return dispatchers[parallel] def _check_prisms(prisms): """ Check if prisms boundaries are well defined Parameters ---------- prisms : 2d-array Array containing the boundaries of the prisms in the following order: ``w``, ``e``, ``s``, ``n``, ``bottom``, ``top``. The array must have the following shape: (``n_prisms``, 6), where ``n_prisms`` is the total number of prisms. This array of prisms must have valid boundaries. Run ``_check_prisms`` before. """ west, east, south, north, bottom, top = tuple(prisms[:, i] for i in range(6)) err_msg = "Invalid prism or prisms. " bad_we = west > east bad_sn = south > north bad_bt = bottom > top if bad_we.any(): err_msg += "The west boundary can't be greater than the east one.\n" for prism in prisms[bad_we]: err_msg += "\tInvalid prism: {}\n".format(prism) raise ValueError(err_msg) if bad_sn.any(): err_msg += "The south boundary can't be greater than the north one.\n" for prism in prisms[bad_sn]: err_msg += "\tInvalid prism: {}\n".format(prism) raise ValueError(err_msg) if bad_bt.any(): err_msg += "The bottom radius boundary can't be greater than the top one.\n" for prism in prisms[bad_bt]: err_msg += "\tInvalid tesseroid: {}\n".format(prism) raise ValueError(err_msg) def jit_prism_gravity( coordinates, prisms, density, kernel, out ): # pylint: disable=invalid-name,not-an-iterable """ Compute gravitational field of prisms on computations points Parameters ---------- coordinates : tuple Tuple containing ``easting``, ``northing`` and ``upward`` of the computation points as arrays, all defined on a Cartesian coordinate system and in meters. prisms : 2d-array Two dimensional array containing the coordinates of the prism(s) in the following order: west, east, south, north, bottom, top in a Cartesian coordinate system. All coordinates should be in meters. density : 1d-array Array containing the density of each prism in kg/m^3. Must have the same size as the number of prisms. kernel : func Kernel function that will be used to compute the desired field. out : 1d-array Array where the resulting field values will be stored. Must have the same size as the arrays contained on ``coordinates``. """ # Iterate over computation points and prisms for l in prange(coordinates[0].size): for m in range(prisms.shape[0]): # Iterate over the prism boundaries to compute the result of the # integration (see Nagy et al., 2000) for i in range(2): for j in range(2): for k in range(2): shift_east = prisms[m, 1 - i] shift_north = prisms[m, 3 - j] shift_upward = prisms[m, 5 - k] # If i, j or k is 1, the shift_* will refer to the # lower boundary, meaning the corresponding term should # have a minus sign out[l] += ( density[m] * (-1) ** (i + j + k) * kernel( shift_east - coordinates[0][l], shift_north - coordinates[1][l], shift_upward - coordinates[2][l], ) ) @jit(nopython=True) def kernel_potential(easting, northing, upward): """ Kernel function for potential gravitational field generated by a prism """ radius = np.sqrt(easting ** 2 + northing ** 2 + upward ** 2) kernel = ( easting * northing * safe_log(upward + radius) + northing * upward * safe_log(easting + radius) + easting * upward * safe_log(northing + radius) - 0.5 * easting ** 2 * safe_atan2(upward * northing, easting * radius) - 0.5 * northing ** 2 * safe_atan2(upward * easting, northing * radius) - 0.5 * upward ** 2 * safe_atan2(easting * northing, upward * radius) ) return kernel @jit(nopython=True) def kernel_g_z(easting, northing, upward): """ Kernel for downward component of gravitational acceleration of a prism """ radius = np.sqrt(easting ** 2 + northing ** 2 + upward ** 2) kernel = ( easting * safe_log(northing + radius) + northing * safe_log(easting + radius) - upward * safe_atan2(easting * northing, upward * radius) ) return kernel @jit(nopython=True) def safe_atan2(y, x): """ Principal value of the arctangent expressed as a two variable function This modification has to be made to the arctangent function so the gravitational field of the prism satisfies the Poisson's equation. Therefore, it guarantees that the fields satisfies the symmetry properties of the prism. This modified function has been defined according to [Fukushima2019]_. """ if x != 0: result = np.arctan(y / x) else: if y > 0: result = np.pi / 2 elif y < 0: result = -np.pi / 2 else: result = 0 return result @jit(nopython=True) def safe_log(x): """ Modified log to return 0 for log(0). The limits in the formula terms tend to 0 (see [Nagy2000]_). """ if np.abs(x) < 1e-10: result = 0 else: result = np.log(x) return result # Define jitted versions of the forward modelling function # pylint: disable=invalid-name jit_prism_gravity_serial = jit(nopython=True)(jit_prism_gravity) jit_prism_gravity_parallel = jit(nopython=True, parallel=True)(jit_prism_gravity)