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

NAME

       grdgravmag3d - Compute the gravity effect of a grid by the method of Okabe

SYNOPSIS

       grdgravmag3d grdfile_top [grdfile_bot] [  -Cdensity ] [  -Ethick ] [  -Fxy_file ] [  -Goutgrid ] [  -H<…>
       ]  [   -Iincrement  ]  [   -Lz_obs ] [  -Q[nn_pad]|[pad_dist]|[<w/e/s/n>] ] [  -Rregion ] [  -Sradius ] [
       -V[level] ] [  -Zlevel[b|t] ] [ -fg ] [ -x+a|n|-n ]

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

DESCRIPTION

       grdgravmag3d will compute the gravity anomaly of a body described by one or (optionally)  two  grids  The
       output can either be along a given set of xy locations or on a grid. This method is not particularly fast
       but allows computing the anomaly of arbitrarily complex shapes.

REQUIRED ARGUMENTS

       grdfile_top [grdfile_bot]
              Grid  file  whose  gravity  effect  is  going  to  be computed. If two grids are provided then the
              gravity/magnetic effect of the volume between them is computed.

       -Cdensity
              Sets body density in SI. This option is mutually exclusive with -H

       -Fxy_file
              Provide locations where the anomaly will be computed. Note this option is mutually exclusive  with
              -G.

       -Goutgrid
              Output the gravity anomaly at nodes of this grid file.

OPTIONAL ARGUMENTS

       -Ethickness
              To provide the layer thickness in m [Default = 500 m].

       -Hf_dec/f_dip/m_int/m_dec/m_dip -H+m<magfile>  -Hx|y|z|h|t -H+i|+g|+r|+f|+n
              Sets parameters for computation of magnetic anomaly (Can be used multiple times).
                 f_dec/f_dip -> geomagnetic declination/inclination

                 m_int/m_dec/m_dip -> body magnetic intensity/declination/inclination

              OR for a grid mode
                 +m<magfile> where ‘magfile’ is the name of the magnetic intensity file.

              To compute a component, specify any of:
                 x|X|e|E  to compute the E-W component.

                 y|Y|n|N  to compute the N-S component.

                 z|Z      to compute the Vertical component.

                 h|H      to compute the Horizontal component.

                 t|T|f|F  to compute the total field.

                 For a variable inclination and declination use IGRF. Set any of -H+i|+g|+r|+f|+n to do that

       -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.

       -Lz_obs
              Sets level of observation [Default = 0]. That is the height (z) at which anomalies are computed.

       -Q[nn_pad]|[pad_dist]|[<w/e/s/n>]

              Extend the domain of computation with respect to output -R region.
                     -Qnn_pad artificially extends the width of the outer rim of cells to have a fake  width  of
                     n_pad * dx[/dy].

                     -Qpad_dist extend the region by west-pad, east+pad, etc.

                     -Qregion Same syntax as -R.

       -Rxmin/xmax/ymin/ymax[+r][+uunit] (more …)
              Specify  the  region  of  interest. Note: this overrides the source grid region (Default: use same
              region as input)

       -Sradius
              Set search radius in km (valid only in the two grids mode OR when -E) [Default  =  30  km].   This
              option  serves  to speed up the computation by not computing the effect of prisms that are further
              away than radius from the current node.

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

       -Zlevel[b|t]
              level of reference plane [Default = 0]. Use this option when the triangles describe  a  non-closed
              surface  and the volume is defined from each triangle and this reference level. An example will be
              the water depth to compute a Bouguer anomaly. Use -Zb or Zt to close the body at its  bottom  (for
              example, to compute the effect of a dome) or at its top (to compute the effect of a spoon).

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

       -x+a|n|-n
              Choose the number of processors used  in  multi-threading  (Only  available  with  multi-threading
              builds).
                 +a Use all available processors.

                 n  Use n processors (not more than max available off course).

                 -n Use (all - n) processors.

       -^ 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.

GRID DISTANCE UNITS

       If the grid does not have meter as the horizontal unit, append +uunit to the input file name  to  convert
       from  the  specified  unit to meter. If your grid is geographic, convert distances to meters by supplying
       -fg instead.

EXAMPLES

       Suppose you want to compute the gravity effect of the  phantom  “Sandy  Island”  together  with  its  not
       phantom seamount

              gmt grdgravmag3d sandy_bat.grd -C1700 -Z-4300 -fg -I1m -Gsandy_okb.grd -V

       To  compute  the  vertical  component due to a magnetization stored in mag.grd over a zone defined by the
       surface bat.grd, using variable declination and inclination provided the the IGRF and using 4 processors,
       do:

              gmt grdgravmag3d bat.grd -E10000 -Gcomp_Z.grd -Hz -H+n -H+mmag.grd -x4 -V -S50

SEE ALSO

       gmt, gmtgravmag3d, talwani2d, talwani3d

REFERENCE

       Okabe, M., Analytical expressions for gravity anomalies due to polyhedral  bodies  and  translation  into
       magnetic anomalies, Geophysics, 44, (1979), p 730-741.

COPYRIGHT

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

5.4.3                                             Jan 03, 2018                                GRDGRAVMAG3D(1gmt)