DOKK / manpages / debian 10 / gmt-common / gmtpmodeler.1gmt.en
GMTPMODELER(1gmt) GMT GMTPMODELER(1gmt)

gmtpmodeler - Evaluate a plate motion model at given locations

gmtpmodeler table -Erot_file -Sflags [ -Fpolygonfile ] [ -Tage ] [ -V[level] ] [ -bbinary ] [ -dnodata ] [ -eregexp ] [ -hheaders ] [ -iflags ] [ -oflags ] [ -:[i|o] ]

Note: No space is allowed between the option flag and the associated arguments.

gmtpmodeler reads a table with lon, lat and optionally age triplets and a plate motion model and evaluates one of several model predictions. Optionally, the user may supply a clipping polygon in multiple-segment format; then, only the part of the points inside the polygon are used to determine the model prediction. The results are written to standard output.

Name of one or more tables with geographical (lon, lat) coordinates and optionally a third column with ages in Myr. If no file is given then we read from standard input.

Give file with rotation parameters. This file must contain one record for each rotation; each record must be of the following format:

lon lat tstart [tstop] angle [ khat a b c d e f g df ]

where tstart and tstop are in Myr and lon lat angle are in degrees. tstart and tstop are the ages of the old and young ends of a stage. If tstop is not present in the record then a total reconstruction rotation is expected and tstop is implicitly set to 0 and should not be specified for any of the records in the file. If a covariance matrix C for the rotation is available it must be specified in a format using the nine optional terms listed in brackets. Here, C = (g/khat)*[ a b d; b c e; d e f ] which shows C made up of three row vectors. If the degrees of freedom (df) in fitting the rotation is 0 or not given it is set to 10000. Blank lines and records whose first column contains # will be ignored. You may prepend a leading + to the filename to indicate you wish to invert the rotations. Alternatively, give the filename composed of two plate IDs separated by a hyphen (e.g., PAC-MBL) and we will instead extract that rotation from the GPlates rotation database. We return an error if the rotation cannot be found.


Type of model prediction(s). Append one or more items: choose from a for plate motion azimuth, d for great-circle distance between current location and its origin at the ridge (in km), s for plate motion model stage ID (1 is youngest), v for plate motion rate (in mm/yr), w for plate rotation rate (degree/Myr), x for change in longitude relative to location of crust formation, y for change in latitude relative to location of crust formation, X for longitude of crust formation, and Y for latitude of crust formation. If no arguments are given we default to all [adsvwxyXY].

Specify a multisegment closed polygon file that describes the area where the model should be evaluated; points outside will be skipped [use all data points].

Use a fixed age for model evaluation (i.e., override the ages given in the input table). This lets you evaluate the model at a snapshot in time, and is a required option if the input table does not contain ages.

Select verbosity level [c].

Select native binary input. [Default is 2 input columns].

Replace input columns that equal nodata with NaN and do the reverse on output.

Only accept data records that match the given pattern.

Skip or produce header record(s).

Select input columns and transformations (0 is first column).

Select output columns (0 is first column).

-^ or just -
Print a short message about the syntax of the command, then exits (NOTE: on Windows just use -).
-+ or just +
Print an extensive usage (help) message, including the explanation of any module-specific option (but not the GMT common options), then exits.
-? or no arguments
Print a complete usage (help) message, including the explanation of all options, then exits.

All spherical rotations are applied to geocentric coordinates. This means that incoming data points and grids are considered to represent geodetic coordinates and must first be converted to geocentric coordinates. Rotations are then applied, and the final reconstructed points are converted back to geodetic coordinates. This default behavior can be bypassed if the ellipsoid setting PROJ_ELLIPSOID is changed to Sphere.


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We will use a table with locations and ages of Pacific crust (pac_age.txt), a plate motion model (Pac_APM.txt), and a polygon that contains the outline of the present Pacific plate (pac_clip_path.txt). To evaluate the plate motion azimuths at the present time for the Pacific, try

gmt gmtpmodeler pac_age.txt -EPac_APM.txt -V -Fpac_clip_path.txt \


                 -Sa -T0 > pac_dir_0.txt




To determine the changes in latitude since crust formation for the entire Pacific, try

gmt gmtpmodeler pac_age.txt -EPac_APM.txt -V -Fpac_clip_path.txt \


                -Sy > pac_dlat.txt




To determine the plate motion velocities in effect when the Pacific crust was formed, try

gmt gmtpmodeler pac_age.txt -EPac_APM.txt -V -Fpac_clip_path.txt \


                -Sv > pac_vel.txt




To determine how far the crust has moved since formation, try

gmt gmtpmodeler pac_age.txt -EPac_APM.txt -V -Fpac_clip_path.txt \


                -Sd > pac_dist.txt




To save the coordinates of the crust's formation, try

gmt gmtpmodeler pac_age.txt -EPac_APM.txt -V -Fpac_clip_path.txt \


                -SXY > ac_origin_xy.txt




GMT distributes the EarthByte rotation model Global_EarthByte_230-0Ma_GK07_AREPS.rot. To use an alternate rotation file, create an environmental parameters named GPLATES_ROTATIONS that points to an alternate rotation file.

backtracker, grdpmodeler, grdrotater, grdspotter, hotspotter, originator, rotconverter

2019, P. Wessel, W. H. F. Smith, R. Scharroo, J. Luis, and F. Wobbe

May 21, 2019 5.4.5