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128 changes: 128 additions & 0 deletions doc/user_guide/topographic_correction.rst
Original file line number Diff line number Diff line change
Expand Up @@ -319,6 +319,134 @@ topography.
fig.colorbar(cmap=True, frame=["af", "x+lTopography", "y+lmeters"])
fig.show()


Terrain correction in spherical coordinates
-------------------------------------------

So far we computed the terrain effect by projecting the topography grid and
the observation points to plain Cartesian coordinates and approximating the
topographic masses with rectangular prisms.
On regional to global scales the curvature of the Earth cannot be neglected:
the projection distorts the geometry of the topographic masses and the
computed terrain effect accumulates errors.
In such cases we can forward model the topographic masses directly in
geocentric spherical coordinates using tesseroids (spherical prisms), which
take the curvature of the Earth into account.

We can build a model of the topographic masses through the
:func:`harmonica.tesseroid_layer` function.
Unlike :func:`harmonica.prism_layer`, its ``surface`` and ``reference``
arguments must be passed as **radii** measured from the center of the Earth,
not as heights above a reference level.
We can obtain the radii of the surface of the reference ellipsoid at each
latitude with :meth:`boule.Ellipsoid.geocentric_radius` and add the
topographic heights to them:

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I would add an admonition here explaining that by assigning the ellipsoidal latitude as coordinates for the tesseroids, we are assuming that there's not significant difference between them and the geocentric spherical latitude.

One alternative way is to convert the ellipsoidal coordinates into geocentric spherical and build the tesseroids from them. For this particular tutorial I'd avoid doing so, because that introduces issues like regridding the topography in geocentric spherical, since a regular grid in ellipsoidal coordinates does not translate into a regular grid in geocentric spherical coordinates.

Let me know if you need any help with this.

.. jupyter-execute::

import boule as bl

ellipsoid = bl.WGS84

longitude, latitude = np.meshgrid(topography.longitude, topography.latitude)
reference = ellipsoid.geocentric_radius(latitude)
surface = reference + topography.values

We will assign the same densities we used for the layer of prisms and define
the layer of tesseroids:

.. jupyter-execute::

density = np.where(topography.values >= 0, 2670, 1040 - 2670)

tesseroids = hm.tesseroid_layer(
coordinates=(topography.longitude, topography.latitude),
surface=surface,
reference=reference,
properties={"density": density},
)
tesseroids

The radial coordinate of the observation points must be expressed in the same
way as the boundaries of the layer: as radii from the center of the Earth.
We will compute them the same way we defined the ``surface`` of the layer, by
adding the observation heights to the geocentric radius of the ellipsoid at
each latitude.
This keeps the observation points consistent with the model of the topographic
masses:

.. jupyter-execute::

radius = ellipsoid.geocentric_radius(data.latitude) + data.height_geometric_m

Tesseroid forward modelling requires every computation point to be located
outside of the tesseroids.
Since our observations were taken on the terrain surface, some of them can
fall slightly below the top boundary of the tesseroid that contains them: the
tops of the tesseroids are given by the topography grid, whose values don't
exactly coincide with the observation heights.
We can make sure every observation point is located on or above the top of its
tesseroid by clamping their radii.
We will clamp against the highest top among the neighboring tesseroids, so
that observation points falling exactly on the boundary between two tesseroids
are safely lifted as well:

.. jupyter-execute::

top = (
tesseroids.top.rolling(longitude=3, latitude=3, center=True, min_periods=1)
.max()
.sel(
longitude=xr.DataArray(data.longitude),
latitude=xr.DataArray(data.latitude),
method="nearest",
)
.values
)
radius = np.maximum(radius, top)
Comment on lines +396 to +406

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I'm a bit confused about this piece of code. I'm not fully understanding why it's necessary to perform the windowing operation. Getting the closest top for each observation point should be enough to build the top array, right?

I'm also thinking if isn't better to adjust the top surface of the tesseroids rather than shifting the observation points. In gravity surveys the height measurements are usually very accurate, carried out through differential GNSS. While the DEMs are models that average the terrain elevation within a region given by the resolution of the model. What do you think?

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Update: I see your point on observation points that fall in the boundaries of tesseroids. My guess is that in those cases the points will never be internal to the tesseroid: they'll always lie on a face or an edge. So I'm not sure if those are going to be problematic.


Now we can compute the terrain effect through the
:meth:`harmonica.DatasetAccessorTesseroidLayer.gravity` method:

.. jupyter-execute::

coordinates_sph = (data.longitude, data.latitude, radius)
terrain_effect_spherical = tesseroids.tesseroid_layer.gravity(
coordinates_sph, field="g_z"
)

And obtain a topography-free gravity disturbance that takes the curvature of
the Earth into account:

.. jupyter-execute::

topo_free_disturbance_spherical = (
data.gravity_disturbance_mgal - terrain_effect_spherical
)

cpt_lims = vd.minmax(topo_free_disturbance_spherical)

fig = pygmt.Figure()
pygmt.makecpt(cmap="viridis", series=cpt_lims)
fig.plot(
x=data.longitude,
y=data.latitude,
fill=topo_free_disturbance_spherical,
cmap=True,
style="c3p",
projection="M15c",
frame=['ag', 'WSen+ggray'],
)
fig.colorbar(
cmap=True,
frame=[
"a50f25",
"x+lTopography-free gravity disturbance (tesseroids)",
"y+lmGal",
],
)
fig.show()

----

.. grid:: 2
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