This chapter briefly explains the things you must
understand to use the software correctly and to avoid meaningless output.
Source faults
have slip, and so they impart stress to the surrounding crust and faults. Receiver faults have no
slip (slip=0.0 m in the input files). Source
and receiver faults otherwise look identical in the input files. The stress imparted by source faults are resolved on
the receiver faults through the command Functions > Stress > Calc.
stress on faults. Further options for resolving the stress on the receiver fault are
controlled by the Stress on faults control panel, which automatically appears.
1. Launch Matlab; set
the Matlab path to working directory ÒCoulomb 3.1 folderÓ.
2. Type ÒcoulombÓ in
Matlab Command Window.
3. In Coulomb 3.1 window menu bar,
choose Input> Open existing input file.
4. In Coulomb 3.1 window menu bar,
choose Functions > Grid, Displacements, Strain, or Stress. Many of these
selections trigger requests for additional input, and let you modify the
parameters in temporary windows. When you click ÒCalc. & viewÓ,
calculations are performed and a new image is displayed.
5. You can perform
many operations to the image on the Coulomb 3.1 window, including Zoom In, Zoom Out, Pan, Rotate 3D, Data Cursor, Insert Color
Bar,
Insert Color Legend, etc. You can choose these operations either by
clicking the lower menu in the Coulomb 3.1 window or the Tools pull down menu
bar. While the graphic plot is open, you save this plot.
6. To print a plot, save it as a pdf,
and then print the small vector file from Acrobat Reader or an illustration
program. Currently, the File > Print cmd in
Matlab does not work properly.
7. After you have
finished all calculations, quit MATLAB.
Most of the settings and parameters can be changed
either by modifying an input file using a text editor, or by changing them
interactively within Coulomb. Choose Functions > Change parameters. Parameters changed within the software interactively
are transient and will not permanently modify the input file. Every time you select Input > Save input file, all current selections will be saved in an input file.
Change the name of the file if you do not want it overwritten.
Coulomb
3.1 calculates in the (x, y, z)
Cartesian coordinate system. When the lat/lon of the
corner grid points are specified in the input file, it can also plot in lat/lon.
In the map view projection on the monitor, x is positive from left to right, y is positive from bottom to top, z is positive upwards for displacement. DEPTH is
positive downwards from the EarthÕs surface. We use the standard Aki &
Richards (1980, 2002) sign
conventions for fault geometry and slip. The units for the input parameters are
the following (see Chapters on Input and Output files for more detail):
Input parameters and their dimensions (think bars and meters)
PR1 PoissonÕs
ratio: [dimensionless, -1 to 0.5]; 0.25 is typically used, and 0.5 is an
imcompressible volume, such as can be used to make balanced cross-sections.
E1 YoungÕs
modulus: [bars]; 8x105 bars is typically used
FRIC Friction
coefficient: [dimensionless; roughly 0-1]; 0.4 is often used; 0.65 is for dry
ByerleeÕs law friction, 0.0-1.0 is typically considered the limits for the
crust.
Sym Obsolete
legacy from Coulomb 1.0; ignore it
Directions,
angle, and dip: [degrees; dip must be positive]
Grid and
fault positions (x, y): [km]
Depth: [km]
downward is positive
Displacements:
[m]
Faults:
Right-lateral is positive, and reverse slip is positive [m]
Dikes:
Opening displacement is positive [m]
Point
Source: Inflation is positive [m3]
Regional
stress tensor, S1, S2, S3: positive in compression [bars]
Output parameters and their dimensions
Displacement:
[m] North, East, and Up are positive
Shear Strain: [dimensionless]
Right-lateral is positive
Principal Strain:
[dimensionless] Extension is positive (tensor notation)
Dilatational
Strain: [dimensionless] Dilatation is positive
Stress: [bars] Right-lateral
and unclamping are positive
Shear modulus, G. YoungÕs modulus [E] and
PoissonÕs Ratio [PR] are specified in the input file. G = E/[2(1+PR)]. So the shear modulus for
PR=0.25 and E=8x105 bars, G=3.2x105 bars or 3.2x1011
dyne-cm.