xenial (1) grdgradient.1gmt.gz

Provided by: gmt-common_5.2.1+dfsg-3build1_all bug

NAME

       grdgradient - Compute directional derivative or gradient from a grid

SYNOPSIS

       grdgradient     in_grdfile     out_grdfile     [     azim[/azim2]     ]     [     [a][c][o][n]     ]    [
       [s|p]azim/elev[/ambient/diffuse/specular/shine] ] [ flag ] [ [e][t][amp][/sigma[/offset]] ] [ region ]  [
       slopefile ] [ [level] ] [ -fg ] [ -n<flags> ]

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

DESCRIPTION

       grdgradient may be used to compute the directional derivative in a given direction (-A), or the direction
       (-S) [and the magnitude (-D)] of the vector gradient of the data.

       Estimated values in the first/last row/column of output depend on boundary conditions (see -L).

REQUIRED ARGUMENTS

       in_grdfile
              2-D grid file from which to compute directional derivative. (See GRID FILE FORMATS below).

       -Gout_grdfile
              Name of the output grid file for the directional derivative. (See GRID FILE FORMATS below).

OPTIONAL ARGUMENTS

       -Aazim[/azim2]
              Azimuthal direction for a directional derivative; azim is the angle in the x,y plane  measured  in
              degrees  positive  clockwise  from  north  (the  +y direction) toward east (the +x direction). The
              negative of the directional derivative, -[dz/dx*sin(azim) + dz/dy*cos(azim)], is  found;  negation
              yields  positive  values  when  the slope of z(x,y) is downhill in the azim direction, the correct
              sense for shading the illumination of an image (see grdimage and grdview) by a light source  above
              the  x,y  plane shining from the azim direction. Optionally, supply two azimuths, -Aazim/azim2, in
              which case the gradients in each of  these  directions  are  calculated  and  the  one  larger  in
              magnitude  is  retained;  this  is  useful  for  illuminating data with two directions of lineated
              structures, e.g., -A0/270 illuminates from the north (top) and west (left).

       -D[a][c][o][n]
              Find the direction of the positive (up-slope) gradient of the data.  To instead  find  the  aspect
              (the down-slope direction), use -Da.  By default, directions are measured clockwise from north, as
              azim in -A above. Append c to use conventional Cartesian angles measured counterclockwise from the
              positive  x  (east)  direction.  Append  o  to  report orientations (0-180) rather than directions
              (0-360).  Append n to add 90 degrees to all angles (e.g., to give local strikes of the surface ).

       -E[s|p]azim/elev[/ambient/diffuse/specular/shine]
              Compute Lambertian radiance  appropriate  to  use  with  grdimage  and  grdview.   The  Lambertian
              Reflection  assumes  an  ideal surface that reflects all the light that strikes it and the surface
              appears equally bright from all viewing directions. azim and elev are the azimuth and elevation of
              light  vector. Optionally, supply ambient diffuse specular shine which are parameters that control
              the reflectance properties of the surface. Default values are: 0.55/0.6/0.4/10 To  leave  some  of
              the values untouched, specify = as the new value. For example -E60/30/=/0.5 sets the azim elev and
              diffuse to 60, 30 and 0.5 and leaves the other reflectance parameters untouched. Append s to use a
              simpler  Lambertian  algorithm.  Note that with this form you only have to provide the azimuth and
              elevation parameters. Append p to use the Peucker  piecewise  linear  approximation  (simpler  but
              faster  algorithm;  in this case the azim and elev are hardwired to 315 and 45 degrees. This means
              that even if you provide other values they will be ignored.)

       -Lflag Boundary condition flag may be x or y or xy indicating data is periodic in range  of  x  or  y  or
              both,  or  flag  may  be g indicating geographical conditions (x and y are lon and lat).  [Default
              uses "natural" conditions (second partial derivative normal to edge is zero).]

       -N[e][t][amp][/sigma[/offset]]
              Normalization. [Default: no normalization.] The actual  gradients  g  are  offset  and  scaled  to
              produce  normalized  gradients  gn  with  a  maximum output magnitude of amp. If amp is not given,
              default amp = 1. If offset is not given, it is set to the average of g. -N yields gn = amp * (g  -
              offset)/max(abs(g - offset)). -Ne normalizes using a cumulative Laplace distribution yielding gn =
              amp * (1.0 - exp(sqrt(2) * (g - offset)/ sigma)) where sigma is estimated using the L1 norm of  (g
              -  offset) if it is not given. -Nt normalizes using a cumulative Cauchy distribution yielding gn =
              (2 * amp / PI) * atan( (g - offset)/ sigma) where sigma is estimated using the L2  norm  of  (g  -
              offset) if it is not given.

       -R[unit]xmin/xmax/ymin/ymax[r] (more ...)
              Specify  the  region of interest. Using the -R option will select a subsection of in_grdfile grid.
              If this subsection exceeds the boundaries of the grid, only the common region will be extracted.

       -Sslopefile
              Name of output grid file with scalar magnitudes of gradient vectors.  Requires  -D  but  makes  -G
              optional.

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

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

       -n[b|c|l|n][+a][+bBC][+c][+tthreshold] (more ...)
              Select interpolation mode for grids.

       -^ or just -
              Print a short message about the syntax of the command, then exits (NOTE: on Windows use just -).

       -+ 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 options, then exits.

       --version
              Print GMT version and exit.

       --show-datadir
              Print full path to GMT share directory and exit.

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.

HINTS

       If  you don't know what -N options to use to make an intensity file for grdimage or grdview, a good first
       try is -Ne0.6.

       Usually 255 shades are more than enough for visualization purposes.  You  can  save  75%  disk  space  by
       appending =nb/a to the output filename out_grdfile.

       If  you  want  to  make  several  illuminated  maps  of  subregions of a large data set, and you need the
       illumination effects to be consistent across all the maps, use the -N option and supply the same value of
       sigma  and  offset to grdgradient for each map. A good guess is offset = 0 and sigma found by grdinfo -L2
       or -L1 applied to an unnormalized gradient grd.

       If you simply need the x- or y-derivatives of the grid, use grdmath.

GRID FILE FORMATS

       By default GMT writes out grid as single precision floats  in  a  COARDS-complaint  netCDF  file  format.
       However,  GMT  is  able  to  produce  grid  files  in many other commonly used grid file formats and also
       facilitates so called "packing" of grids, writing out floating point data as 1- or  2-byte  integers.  To
       specify  the  precision, scale and offset, the user should add the suffix =id[/scale/offset[/nan]], where
       id is a two-letter identifier of the grid type and precision, and scale and  offset  are  optional  scale
       factor  and  offset to be applied to all grid values, and nan is the value used to indicate missing data.
       In case the two characters id is not provided, as in =/scale than  a  id=nf  is  assumed.   When  reading
       grids,  the  format  is generally automatically recognized. If not, the same suffix can be added to input
       grid file names. See grdconvert and Section grid-file-format of the GMT Technical Reference and  Cookbook
       for more information.

       When  reading  a  netCDF  file  that  contains  multiple  grids,  GMT  will  read,  by default, the first
       2-dimensional grid that can find in that  file.  To  coax  GMT  into  reading  another  multi-dimensional
       variable  in  the grid file, append ?varname to the file name, where varname is the name of the variable.
       Note that you may need to escape the special meaning of ? in your shell program by putting a backslash in
       front  of  it, or by placing the filename and suffix between quotes or double quotes. The ?varname suffix
       can also be used for output grids to specify a  variable  name  different  from  the  default:  "z".  See
       grdconvert and Sections modifiers-for-CF and grid-file-format of the GMT Technical Reference and Cookbook
       for more information, particularly on how to read splices of 3-, 4-, or 5-dimensional grids.

EXAMPLES

       To make a file for illuminating the data in  geoid.nc  using  exp-  normalized  gradients  in  the  range
       [-0.6,0.6] imitating light sources in the north and west directions:

              gmt grdgradient geoid.nc -A0/270 -Ggradients.nc=nb/a -Ne0.6 -V

       To find the azimuth orientations of seafloor fabric in the file topo.nc:

              gmt grdgradient topo.nc -Dno -Gazimuths.nc -V

REFERENCES

       Horn,  B.K.P.,  Hill-Shading  and  the  Reflectance Map, Proceedings of the IEEE, Vol. 69, No. 1, January
       1981, pp. 14-47.  (http://people.csail.mit.edu/bkph/papers/Hill-Shading.pdf)

SEE ALSO

       gmt, gmt.conf grdhisteq, grdmath, grdimage, grdview, grdvector

       2015, P. Wessel, W. H. F. Smith, R. Scharroo, J. Luis, and F. Wobbe