.. _equivalent_sources: Equivalent Sources ================== .. toctree:: :hidden: eqs-parameters-estimation block-averaged-eqs gradient-boosted-eqs eq-sources-spherical Most potential field surveys gather data along scattered and uneven flight lines or ground measurements. For a great number of applications we may need to interpolate these data points onto a regular grid at a constant altitude. Upward-continuation is also a routine task for smoothing, noise attenuation, source separation, etc. Both tasks can be done simultaneously through an *equivalent sources* [Dampney1969]_ (a.k.a *equivalent layer*). The equivalent sources technique consists in defining a finite set of geometric bodies (like point sources) beneath the observation points and adjust their coefficients so they generate the same measured field on the observation points. These fitted sources can be then used to *predict* the values of this field on any unobserved location, like a regular grid, points at different heights, any set of scattered points or even along a profile. The equivalent sources have two major advantages over any general purpose interpolator: * it takes into account the 3D nature of the potential fields being measured by considering the observation heights, and * its predictions are always harmonic. Its main drawback is the increased computational load it takes to fit the sources' coefficients, both in terms of memory and computation time). Harmonica has a few different classes for applying the equivalent sources techniques. Here we will explore how we can use the :class:`harmonica.EquivalentSources` to interpolate some gravity disturbance scattered points on a regular grid with a small upward continuation. We can start by downloading some sample gravity data over the Bushveld Igneous Complex in Southern Africa: .. jupyter-execute:: import ensaio import pandas as pd fname = ensaio.fetch_bushveld_gravity(version=1) data = pd.read_csv(fname) data The :class:`harmonica.EquivalentSources` class works exclusively in Cartesian coordinates, so we need to project these gravity observations: .. jupyter-execute:: import pyproj import verde as vd projection = pyproj.Proj(proj="merc", lat_ts=data.latitude.values.mean()) easting, northing = projection(data.longitude.values, data.latitude.values) region = vd.get_region((easting, northing)) Now we can initialize the :class:`harmonica.EquivalentSources` class. .. jupyter-execute:: import harmonica as hm equivalent_sources = hm.EquivalentSources(depth=10e3, damping=10) equivalent_sources By default, it places the sources one beneath each data point at a relative depth from the elevation of the data point following [Cooper2000]_. This *relative depth* can be set through the ``depth`` argument. Deepest sources generate smoother predictions (*underfitting*), while shallow ones tend to overfit the data. .. note:: If instead we want to place every source at a constant depth, we can change it by passing ``depth_type="constant"``. In that case, the ``depth`` argument will be the exact depth at which the sources will be located. The ``damping`` parameter is used to smooth the coefficients of the sources and stabilize the least square problem. A higher ``damping`` will create smoother predictions, while a lower one could overfit the data and create artifacts. Now we can estimate the source coefficients through the :meth:`harmonica.EquivalentSources.fit` method against the observed gravity disturbance. .. jupyter-execute:: coordinates = (easting, northing, data.height_geometric_m) equivalent_sources.fit(coordinates, data.gravity_disturbance_mgal) Once the fitting process finishes, we can predict the values of the field on any set of points using the :meth:`harmonica.EquivalentSources.predict` method. For example, lets predict on the same observation points to check if the sources are able to reproduce the observed field. .. jupyter-execute:: disturbance = equivalent_sources.predict(coordinates) And plot it: .. jupyter-execute:: import pygmt # Get max absolute value for the observed gravity disturbance maxabs = vd.maxabs(data.gravity_disturbance_mgal) # Set figure properties w, e, s, n = region fig_height = 10 fig_width = fig_height * (e - w) / (n - s) fig_ratio = (n - s) / (fig_height / 100) fig_proj = f"x1:{fig_ratio}" fig = pygmt.Figure() pygmt.makecpt(cmap="polar+h0", series=[-maxabs, maxabs]) title="Predicted gravity disturbance" with pygmt.config(FONT_TITLE="14p"): fig.plot( x=easting, y=northing, color=disturbance, cmap=True, style="c3p", projection=fig_proj, region=region, frame=['ag', f"+t{title}"], ) fig.colorbar(cmap=True, position="JMR", frame=["a50f25", "y+lmGal"]) fig.shift_origin(yshift=fig_height + 2) title="Observed gravity disturbance" with pygmt.config(FONT_TITLE="14p"): fig.plot( x=easting, y=northing, color=data.gravity_disturbance_mgal, cmap=True, style="c3p", frame=['ag', f"+t{title}"], ) fig.colorbar(cmap=True, position="JMR", frame=["a50f25", "y+lmGal"]) fig.show() We can also *grid* and *upper continue* the field by predicting its values on a regular grid at a constant height higher than the observations. To do so we can use the :func:`verde.grid_coordinates` function to create the coordinates of the grid and then use the :meth:`harmonica.EquivalentSources.grid` method. First, lets get the maximum height of the observations: .. jupyter-execute:: data.height_geometric_m.max() Then create the grid coordinates at a constant height of and a spacing of 2km; and use the equivalent sources to generate a gravity disturbance grid. .. jupyter-execute:: # Build the grid coordinates grid_coords = vd.grid_coordinates(region=region, spacing=2e3, extra_coords=2.2e3) # Grid the gravity disturbances grid = equivalent_sources.grid(grid_coords, data_names=["gravity_disturbance"]) grid And plot it .. jupyter-execute:: maxabs = vd.maxabs(grid.gravity_disturbance) fig = pygmt.Figure() pygmt.makecpt(cmap="polar+h0", series=[-maxabs, maxabs]) fig.grdimage( frame=['af', 'WSen'], grid=grid.gravity_disturbance, region=region, projection=fig_proj, cmap=True, ) fig.colorbar(cmap=True, frame=["a50f25", "x+lgravity disturbance", "y+lmGal"]) fig.show()