Provided by: gmt_4.5.11-1build1_amd64 bug

NAME

       grdspotter - Create CVA image directly from gravity or bathymetry grids

SYNOPSIS

       grdspotter       [grdfile]       -Erotations_file      -GCVAgrid      -Ixinc[unit][=|+][/yinc[unit][=|+]]
       -Rwest/east/south/north[r] [ -Aagegrid ] [ -Bn_try ] [ -C ] [ -DDIgrid ] [ -F ] [ -L IT(IDgrid) ] [ -M  ]
       [  -Nupper_age ] [ -PPAgrid ] [ -QIDinfo ] [ -S ] [ -T ] [ -Ufixed_val ] [ -V ] [ -Zz_min[/z_max[/z_inc]]
       ]

DESCRIPTION

       grdspotter reads a grid file with residual bathymetry or gravity and calculates flowlines from each  node
       that exceeds a minimum value using the specified rotations file.  These flowlines are then convolved with
       the volume of the prism represented by each grid node and added up to give a Cumulative Volcano Amplitude
       grid (CVA).
            No  space between the option flag and the associated arguments.  Use upper case for the option flags
       and lower case for modifiers.

       grdfile
              Data grid to be processed, typically residual bathymetry or free-air anomalies.

       -E     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 -C is set then a total reconstruction rotation is
              expected and tstop is implicitly set to 0  and  should  not  be  specified  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.

       -G     Specify name for output CVA grid file.

       -I     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 c to indicate arc seconds.
              If one of the units e, k, i, or n is appended instead, the increment is assumed  to  be  given  in
              meter, km, miles, or nautical miles, respectively, and will be converted to the equivalent degrees
              longitude  at  the middle latitude of the region (the conversion depends on 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 = 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 + 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  Appendix  B  for
              details.   Note:  if  -Rgrdfile  is used then grid spacing has already been initialized; use -I to
              override the values.

       -R     west, east, south, and north specify the Region of interest, and you may specify them  in  decimal
              degrees  or  in  [+-]dd:mm[:ss.xxx][W|E|S|N]  format.   Append r if lower left and upper right map
              coordinates are given instead of w/e/s/n.  The two shorthands -Rg and -Rd stand for global  domain
              (0/360  and -180/+180 in longitude respectively, with -90/+90 in latitude). Alternatively, specify
              the name of an existing grid file and the -R settings (and grid spacing, if applicable) are copied
              from the grid.

OPTIONS

       -A     Supply a crustal age grid that is co-registered with the input data grid.  These ages  become  the
              upper  ages  to use when constructing flowlines [Default extend flowlines back to oldest age found
              in the rotation file; but see -N].

       -B     Get n_try bootstrap estimates of the maximum CVA location; the longitude and latitude results  are
              written to stdout [Default is no bootstrapping].  Cannot be used with -M.

       -C     Expect  Total Reconstruction Rotations rather than Forward Stage Rotations [Default].  File format
              is similar to the stage pole format except that the tstart column is not present (assumed to be  0
              Ma).

       -D     Use  flowlines  to  determine  the  maximum  CVA encountered along each flowline and create a Data
              Importance (DI) grid with these values at the originating nodes.

       -F     Force pixel registration [Default is grid registration].

       -L     Supply a co-registered grid with seamount chain IDs for each node.  This option requires that  you
              also use -Q.

       -M     Do  not  attempt  to  keep all flowlines in memory when using -D and/or -P.  Should you run out of
              memory you can use this option to compute flowlines on-the-fly.  It will be slower as we no longer
              can reuse the flowlines calculated for the CVA step.  Cannot be used with -B  or  the  multi-slice
              mode in -Z.

       -N     Set  the  upper  age  to  assign to nodes whose crustal age is unknown (i.e., NaN) [no upper age].
              Also see -A.

       -P     Use flowlines to determine the flowline age at  the  CVA  maximum  for  each  node  and  create  a
              Predicted Age (PA) grid with these values at the originating nodes.

       -Q     Either  give  (1)  a single ID to use or (2) the name of a file with a list of IDs to use [Default
              uses all IDs].  Each line would be TAG ID [w e s  n].   The  w/e/s/n  zoom  box  is  optional;  if
              specified  it  means  we only trace the flowline if inside this region [Default uses region set by
              -R].  Requires -L.

       -S     Normalize the resulting CVA grid to percentages of the CVA maximum.  This also normalizes  the  DI
              grid (if requested).

       -T     Truncate  crustal  ages  given  via  the  -A  option  that  exceed  the  upper age set with -N [no
              truncation].

       -U     After a node passes the test implied by -Z,  use  this  fixed_val  instead  in  the  calculations.
              [Default uses individual node values].

       -V     Selects verbose mode, which will send progress reports to stderr [Default runs "silently"].

       -Z     Ignore  nodes  with  z-values  lower  than z_min [0] and optionally larger than z_max [Inf].  Give
              z_min/z_max/z_inc to make separate CVA grids for  each  z-slice  [Default  makes  one  CVA  grid].
              Multi-slicing cannot be used with -M.

EXAMPLES

       To  create  a  CVA image from the Pacific topography grid Pac_res_topo.grd, using the DC85.d Euler poles,
       and only output a grid for the specified domain, run

       grdspotter Pac_res_topo.grd -E DC85.d -G CVA.grd -R 190/220/15/25 -I 2m -N 145 -T -V

       This file can then be plotted with grdimage.

COORDINATES

       Data coordinates are assumed to be geodetic and will automatically  be  converted  to  geocentric  before
       spherical  rotations  are  performed.  We convert back to geodetic coordinates for output.  Note: If your
       data already are geocentric, you can avoid the conversion by using --ELLIPSOID=sphere.

SEE ALSO

       GMT(1),   grdimage(1),   grdrotater(1),   project(1),   mapproject(1),   backtracker(1),   hotspotter(1),
       originator(1)

REFERENCES

       Wessel, P., 1999, "Hotspotting" tools released, EOS Trans. AGU, 80 (29), p. 319.

GMT 4.5.11                                         5 Nov 2013                                   GRDSPOTTER(1gmt)