bionic (1) talwani3d.1gmt.gz

Provided by: gmt-common_5.4.3+dfsg-1_all bug

NAME

       talwani3d - Compute free-air, geoid or vertical gravity gradients anomalies over 3-D bodies

SYNOPSIS

       talwani3d  [ modeltable ] [  -A ] [  -Drho ] ] [  -Ff|n|v ] [  -Goutfile ] [  -Iincrement ] [  -M[h][v] ]
       [  -Ntrackfile ] [  -Rregion ] [  -Zlevel|obsgrid ] [  -V[level] ] [ -bibinary ] [ -dnodata ] [  -eregexp
       ] [ -fg ] [ -iflags ] [ -oflags ] [ -r ] [ -x[[-]n] ]

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

DESCRIPTION

       talwani3d  will  read  the  multi-segment  modeltable  from  file  or standard input.  This file contains
       contours of a 3-D body at different z-levels, with one contour per  segment.   The  segment  header  must
       contain  the  parameters  zlevel  rho,  which  states  the  z contour level and the density of this slice
       (individual slice densities may be overridden by a fixed density contrast given via -D).  We can  compute
       anomalies  on an equidistant grid (by specifying a new grid with -R and -I or provide an observation grid
       with elevations) or at arbitrary output points specified via -N.  Chose from free-air anomalies, vertical
       gravity  gradient  anomalies,  or  geoid  anomalies.   Options  are  available  to control axes units and
       direction.

REQUIRED ARGUMENTS

       modeltable
              The file describing the horizontal contours of the bodies.  Contours will be automatically  closed
              if not already closed, and repeated vertices will be eliminated.

       -Ixinc[unit][+e|n][/yinc[unit][+e|n]]
              x_inc  [and  optionally  y_inc]  is  the  grid  spacing.  Optionally,  append  a  suffix modifier.
              Geographical (degrees) coordinates: Append m to indicate arc minutes or s to indicate arc seconds.
              If  one  of the units e, f, k, M, n or u is appended instead, the increment is assumed to be given
              in meter, foot, km, Mile, nautical mile or US survey foot, respectively, and will be converted  to
              the  equivalent  degrees longitude at the middle latitude of the region (the conversion depends on
              PROJ_ELLIPSOID). If y_inc is given but set to 0 it will be reset equal to x_inc; otherwise it will
              be  converted to degrees latitude. All coordinates: If +e is appended then the corresponding max x
              (east) or y (north) may be slightly adjusted to fit exactly the given increment  [by  default  the
              increment  may  be  adjusted  slightly  to  fit  the  given domain]. Finally, instead of giving an
              increment you may specify the number of nodes desired by appending  +n  to  the  supplied  integer
              argument;  the  increment  is  then  recalculated  from  the  number  of nodes and the domain. The
              resulting  increment  value  depends  on  whether  you  have  selected  a  gridline-registered  or
              pixel-registered  grid; see App-file-formats for details. Note: if -Rgrdfile is used then the grid
              spacing has already been initialized; use -I to override the values.

       -Rxmin/xmax/ymin/ymax[+r][+uunit] (more …)
              Specify the region of interest.

OPTIONAL ARGUMENTS

       -A     The z-axis should be positive upwards [Default is down].

       -Dunit Sets fixed density contrast that overrides any setting in model file, in kg/m^3.

       -Ff|n|v
              Specify desired gravitational field component.  Choose between f (free-air anomaly)  [Default],  n
              (geoid) or v (vertical gravity gradient).

       -Goutfile
              Specify  the  name  of the output data (for grids, see GRID FILE FORMATS below).  Required when an
              equidistant grid is implied for output.  If -N is used then output is written to stdout  unless  G
              specifies an output file.

       -M[h][v]
              Sets  units  used.   Append  h  to  indicate  horizontal  distances are in km [m], and append z to
              indicate vertical distances are in km [m].

       -Ntrackfile
              Specifies locations where we wish to compute the predicted value.  When this option is used  there
              are no grids and the output data records are written to stdout.

       -V[level] (more …)
              Select verbosity level [c].

       -Zlevel|obsgrid
              Set observation level either as a constant or give the name of a grid with observation levels.  If
              the latter is used the the grid determines the output grid region [0].

       -bi[ncols][t] (more …)
              Select native binary input. [Default is 2 input columns].

       -d[i|o]nodata (more …)
              Replace input columns that equal nodata with NaN and do the reverse on output.

       -e[~]”pattern” | -e[~]/regexp/[i] (more …)
              Only accept data records that match the given pattern.

       -fg    Geographic grids (dimensions of longitude, latitude) will be converted to km via  a  “Flat  Earth”
              approximation using the current ellipsoid parameters.

       -h[i|o][n][+c][+d][+rremark][+rtitle] (more …)
              Skip or produce header record(s). Not used with binary data.

       -icols[+l][+sscale][+ooffset][,] (more …)
              Select input columns and transformations (0 is first column).

       -ocols[,…] (more …)
              Select output columns (0 is first column).

       -r (more …)
              Set pixel node registration [gridline].

       -x[[-]n] (more …)
              Limit number of cores used in multi-threaded algorithms (OpenMP required).

       -:[i|o] (more …)
              Swap 1st and 2nd column on input and/or output.

       -^ 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.

UNITS

       For map distance unit, append unit d for arc degree, m for arc minute, and s for arc  second,  or  e  for
       meter [Default], f for foot, k for km, M for statute mile, n for nautical mile, and u for US survey foot.
       By default we compute such distances using a spherical approximation with great circles. Prepend -  to  a
       distance  (or  the  unit  is no distance is given) to perform “Flat Earth” calculations (quicker but less
       accurate) or prepend + to perform exact geodesic calculations (slower but more accurate).

EXAMPLES

       To compute the free-air anomalies on a grid over a  3-D  body  that  has  been  contoured  and  saved  to
       body.txt, using 1.7 g/cm^3 as the density contrast, try

          gmt talwani3d -R-200/200/-200/200 -I2 -G3dgrav.nc body.txt -D1700 -Fg

       To obtain the vertical gravity gradient anomaly along the track in crossing.txt for the same model, try

          gmt talwani3d -Ncrossing.txt body.txt -D1700 -Fv > vgg_crossing.txt

       Finally,  the  geoid  anomaly  along  the  same  track  in  crossing.txt for the same model is written to
       n_crossing.txt by

          gmt talwani3d -Ncrossing.txt body.txt -D1700 -Fn -Gn_crossing.txt

REFERENCES

       Kim, S.-S., and P. Wessel, 2016, New analytic solutions for modeling vertical gravity gradient anomalies,
       Geochem. Geophys. Geosyst., 17, http://dx.doi.org/10.1002/2016GC006263.

       Talwani,  M.,  and  M.  Ewing,  1960,  Rapid computation of gravitational attraction of three-dimensional
       bodies of arbitrary shape, Geophysics, 25, 203-225.

SEE ALSO

       gmt.conf, gmt, grdmath, gravfft, gmtgravmag3d, grdgravmag3d, talwani2d

       2018, P. Wessel, W. H. F. Smith, R. Scharroo, J. Luis, and F. Wobbe