Chapter 6
Here we guide you in calculating
deformation caused by an earthquake and display the results graphically.
1. Input > Preferences and change Coordinates from Cartesian to Lon. &
Lat.
Input > Open existing input file >
ÔExample-2(LL)-lonlat.inpÕ. Then, Functions > Displacements > Horizontal
displ. (vectors). You will see a dense vector image in the Coulomb
3.1
window. To plot fewer vectors, Functions > Change
parameters > Grid size, and change it from 0.06¡ x 0.04¡ to 0.12¡ x 0.08¡,
and hit OK. Now repeat Functions > Displacements > Horizontal
displ. (vectors). After youÕve seen the plot, return the coordinate
system to (x, y) by Input > Preferences and change Coordinates from Lon. &
Lat.
to Cartesian, and click OK.
No reference
point
Reference point by mouse click

2. To change vector scale and reference frame: In the Displacement control panel, either move the
slider (which rescales the vectors on the fly) or type in a number (try 10,000)
in the text field (these means the vector scale is 10,000 x the distance
scale). Then click on Fixed point, hit the Mouse click button and click
on a point to the SE of the fault, and hit ÒCalc. & view.Ó You should now
see a plot like that above right, with the reference point indicated by a red
circle.
3. Numerical
output files are created every time you make a run. Every time when you click ÒCal. & ViewÓ in the Displacement
control panel, a text output file
called ÒDisplacement.couÓ will be created or updated and saved in a sub-folder
called ÒOutput filesÓ within the ÒCoulomb 3.1 folderÓ. When you want to
save your latest runs, remember to rename the ÒDisplacement.couÓ file;
otherwise it will be overwritten by your next displacement calculations. Below
left is an excerpt of a ÒDisplacement.couÓ text output file.
Coordinates
Displacements
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4. Change sampling depth of calculation: In the Displacement
control panel, type your desired value after ÒDepthÓ. Most often for displacements,
one sets DEPTH to 0.0 to compare the results to geodetic data.
5. Make a displacement cross-section: Choose Input > Open existing
input file > Example-2(TH).inp. Next, Functions > Displacements > Horizontal
displ (vectors). In the Displacement control panel, choose ÒCross
sectionÓ. Change the increments to 2 km by 2 km. This is a reverse fault;
the dashed blue line in the plot below is the depth of the vectors in the map
view plot. The cross-section line was included in the input file (this optional
information is shown above right). You can change the cross-section line
interactively in the Cross section control panel. Use
the left mouse button to click the start
(A) point, and the right mouse button to
click the end (B) point, and make sure that the
starting point is to the left of the
ending point. If you do not have a two-button mouse, use ctrl+click for
the right button. To save the changes, choose Input > Save input
file as ascii with a new file name.

For displacement plots, the dip of
the cross section is always vertical. Within the Cross section window, you can chose items on the menu
bars to Zoom In,
Zoom Out, Pan, and 3D Rotate.
6.2 To display observed and
modelled GPS vectors

3. To output a numerical file of
the observed and modelled displacements, follow the instructions in the command window (reproduced
below). The GPS_DATA file can be opened in Excel for further calculations of
residuals. The example below uses the input file, Niigata-Chuetsuoki-2007.may and
the GPS file ÔNiigata-Chuetsuoki-2007-GPS.dat.


1. Using
Example-2(TH).inp, Choose Functions > Displacements > Horizontal
displ. (wireframe). The undistorted grid is in yellow and the distorted
grid in blue. For a cross-section, use the default cross-section line, but
change the horizontal and depth increments to 2 km in the Cross section
control panel to see the images below. These cross-sections conserve area (they are
ÔretrodeformableÕ in geological jargon) if you set PossionÕs ratio to 0.5 by Functions > Change
Parameters >All input parameters:
![]()
2. The wireframe
cross-sections are useful to illustrate deformed strata associated with thrust
and normal faults and ramp-thrusts. You can pop them into Illustrator and color
the layering so it appears like strata.

1. Choose Input
> Open an existing file
ÔExample-2(LL)-latlon.inpÕ; then Functions > Displacements > Vertical
displ. (color & contours). You will see the following left image in the Coulomb
3.1
window.
Tiled
Interpolated

2. Data
smoothing and color scale options: In the Vertical displ. control panel, you can choose
either Mosaic, i.e., un-interpolated data (left image shown above) or Interp.,
i.e., interpolated (right image shown above). Color
saturation: You can adjust color scale by moving the slider bar
under ÒColor saturationÓ or type the value in the box, hit return, and then
click ÔCalc. & ViewÓ in the Displacement control panel (below left).

3. Contours: In the Displacement control panel, choose ÒContoursÓ
and click ÒCalc. & ViewÓ. Contours showing vertical displacements are
superimposed on the color image (image above right). You can choose the contour
interval.
4. Cross section: Choose ÒCross sectionÓ in the
Displacement control panel. The methods of making cross sections are similar to
those described in previous sections.
1. Choose
Functions > Displacements > 3D image drape. The color scale is controlled
by the parameter in your input file.
2. To
control the amount of vertical exaggeration (the ÒmÓ factor in the screen
images), choose Functions > Change parameters > Vertical, and you will see
a pop-up Vertical exaggeration window, in which you can change vertical
exaggeration by entering a new value and then clicking ÒOKÓ.

3. In the Coulomb 3.1 window, you can
use options of Zoom In, Zoom Out, Pan, 3D Rotate, Insert/Remove
ColorBar, and Insert/Remove Legend, as described in previous
sections.
1. Choose Functions > Displacements > 3D image
wireframed surface. The color scale is controlled by the parameter in your
input file.
2. You can use options of Zoom
In,
Zoom Out, Pan, 3D Rotate, Insert/Remove ColorBar, and Insert/Remove
Legend, as described in previous sections. Now try changing the vertical
exaggeration by choosing Functions > Change parameters > Vertical
exaggeration > 8000. Then, again choose Functions > Displacements > 3D image
wireframed surface. Now change the azimuth to 10¡ and Elevation to 40¡
in the Viewpoint window by hitting tab after each number and the screen will
redraw:

Both ÔHorizontal Displ.
(vectors)Õ and ÔHorizontal displ. (wireframe)Õ provide cross-section outputs.
These also produce numerical output files of the ground surface deformation
components, Ux, Uy, and Uz.

1. Choose Functions > Strain. A Strain control
panel will appear (below right).

2. In the Strain control
panel, choose the type of strain you want to calculate. For example, choose Eyy
and
you will see the image above right.
3. Numerical
output files. Every time you click
ÒCal. & ViewÓ in the Strain control panel, an output file called Òdilatation_section.couÓ will
be created or updated. When you want to save your latest runs,
remember to rename the Òdilatation_section.couÓ file within the Òoutput filesÓ
sub-folder; otherwise it will be written over by your future displacement
calculations. Here is an example of Òdilatation_section.couÓ output
file:

4. By choosing parameters
in the Strain control panel, you have the options to switch between the
tiled versus interpolated data grid, change color saturation, and contours, as
explained in previous sections.