# grdgradient¶

Compute directional gradients from a grid

## Synopsis¶

**gmt grdgradient** *ingrid* **-G***outgrid*
[ **-A***azim*[/*azim2*] ] [ **-D**[**a**][**c**][**o**][**n**] ]
[ **-E**[**m**|**s**|**p**]*azim/elev*[**+a***ambient*][**+d***diffuse*][**+p***specular*][**+s***shine*] ]
[ **-N**[**e**|**t**][*amp*][**+a***ambient*][**+s***sigma*][**+o***offset*] ]
[ **-Q****c**|**r**|**R**[**+f***file*]]
[ **-R***region* ] [ **-S***slopefile* ]
[ **-V**[*level*] ] [ **-f**flags ]
[ **-n**flags ]
[ **--PAR**=*value* ]

**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 to find the direction (**-D**) [and the magnitude
(**-S**)] of the vector gradient of the data.

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

## Required Arguments¶

*ingrid*[=*ID*|?*varname*][**+b***band*][**+d***divisor*][**+n***invalid*][**+o***offset*][**+s***scale*]

2-D grid file from which to compute directional derivative. Optionally, append =

IDfor reading a specific file format [Default is =nf] or ?varnamefor a specific netCDF variable [Default is the first 2-D grid found by GMT] (See full description). The following modifiers are supported:

+b- Select aband(for images only) [Default is 0].

+d- Divide data values by the givendivisor[Default is 1].

+n- Replace data values matchinginvalidwith NaN.

+o- Offset data values by the givenoffset[Default is 0].

+s- Scale data values by the givenscale[Default is 1].Note: Any offset is added after any scaling.

**-G***outgrid*[=*ID*][**+d***divisor*][**+n***invalid*][**+o***offset*|**a**][**+s***scale*|**a**][:*driver*[*dataType*][**+c***options*]]

Give the name of the output grid file for the directional derivative. Optionally, append =

IDfor writing a specific file format (See full description). The following modifiers are supported:

+d- Divide data values by givendivisor[Default is 1].

+n- Replace data values matchinginvalidwith a NaN.

+o- Offset data values by the givenoffset, or appendafor automatic range offset to preserve precision for integer grids [Default is 0].

+s- Scale data values by the givenscale, or appendafor automatic scaling to preserve precision for integer grids [Default is 1].

Note: Any offset is added before any scaling.+saalso sets+oa(unless overridden). To write specific formats via GDAL, use =gdand supplydriver(and optionallydataType) and/or one or more concatenated GDAL-cooptions using+c. See the “Writing grids and images” cookbook section for more details.

## Optional Arguments¶

**-A***azim*[/*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, \(-(\frac{dz}{dx}\sin(a) + \frac{dz}{dy}\cos(a))\) , is found where \(a\) is the*azimuth*; negation yields positive values when the slope of \(z(x,y)\) is downhill in the \(a\) 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 \(a\) direction. Optionally, supply two azimuths,**-A***azim*/*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.,**-A***0*/*270*illuminates from the north (top) and west (left). Finally, if*azim*is a file it must be a grid of the same domain, spacing and registration as*ingrid*and we will update the azimuth at each output node when computing the directional derivatives.

**-D**[**a**][**c**][**o**][**n**]Instead of finding the gradient in a given direction (

**-A**), find the direction of the positive (up-slope) gradient of the data. The following modifiers are supported:**a**- Find the aspect (i.e., the down-slope direction).**c**- Use the conventional Cartesian angles measured counterclockwise from the positive x (east direction) [Default measures directions clockwise from north, as*azim*in**-A**].**o**- Report orientations (0-180) rather than directions (0-360).**n**- Add 90 degrees to all angles (e.g., to give local strikes of the surface).

**-E**[**m**|**s**|**p**]*azim/elev*[**+a***ambient*][**+d***diffuse*][**+p***specular*][**+s***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. Here,

*azim*and*elev*are the azimuth and elevation of the light vector. Optionally, supply*ambient*[0.55],*diffuse*[0.6],*specular*[0.4], or*shine*[10], which are parameters that control the reflectance properties of the surface. Default values are given in the brackets. Use**-Es**for a simpler Lambertian algorithm. Note that with this form you only have to provide azimuth and elevation. Alternatively, use**-Ep**for 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.)

**-N**[**e**|**t**][*amp*][**+a***ambient*][**+s***sigma*][**+o***offset*]Normalization [Default is no normalization.] The actual gradients \(g\) are offset and scaled to produce normalized gradients \(g_n\) 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 \(g\). The following forms are supported, where \(o\) is the offset and \(a\) is the*amp*:**-N**- Normalize using \(g_n = a(\frac{g - o}{max(|g - o|)})\)**-Ne**- Normalize using a cumulative Laplace distribution yielding: \(g_n = a(1 - \exp{(\sqrt{2}\frac{g - o}{\sigma}))}\), where \(\sigma\) is estimated using the L1 norm of \((g - o)\) if it is not given.**-Nt**- Normalize using a cumulative Cauchy distribution yielding: \(g_n = \frac{2a}{\pi}(\tan^{-1}(\frac{g - o}{\sigma}))\) where \(\sigma\) is estimated using the L2 norm of \((g -o)\) if it is not given.

To use \(o\) and/or \(\sigma\) from a previous calculation, leave out the argument to the modifier(s) and see

**-Q**for usage. As a final option, you may add**+a***ambient*to add*ambient*to all nodes after gradient calculations are completed.

**-Qc**|**r**|**R**[**+f***file*]Controls how normalization via

**-N**is carried out. When multiple grids should be normalized the same way (i.e., with the same*offset*and/or*sigma*), we must pass these values via**-N**. However, this is inconvenient if we compute these values from a grid. Use**-Qc**to save the results of*offset*and*sigma*to a statistics file; if grid output is not needed for this run then do not specify**-G**. For subsequent runs, just use**-Qr**to read these values. Using**-QR**will read then delete the statistics file. See Tiles for more information. Optionally, append**+f***file*to write/read the statistics to/from the specified*file*.

**-R***xmin*/*xmax*/*ymin*/*ymax*[**+r**][**+u***unit*]Specify the region of interest. Using the

**-R**option will select a subsection of*ingrid*grid. If this subsection exceeds the boundaries of the grid, only the common region will be extracted. (See full description) (See cookbook information).

**-S***slopefile*Name of output grid file with scalar magnitudes of gradient vectors. Requires

**-D**but makes**-G**optional.

**-V**[*level*]Select verbosity level [

**w**]. (See full description) (See cookbook information).

**-f**flagsGeographic 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**][**+b***BC*][**+c**][**+t***threshold*] (more …)Select interpolation mode for grids.

**-^**or just**-**Print a short message about the syntax of the command, then exit (

**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 exit.

**-?**or no argumentsPrint a complete usage (help) message, including the explanation of all options, then exit.

**--PAR**=*value*Temporarily override a GMT default setting; repeatable. See gmt.conf for parameters.

## Grid Distance Units¶

If the grid does not have meter as the horizontal unit, append **+u***unit* to the input file name to convert from the
specified unit to meter. If your grid is geographic, convert distances to meters by supplying **-f**flags 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**-Ne**0.6.Usually 255 shades are more than enough for visualization purposes. You can save 75% disk space by appending =nb/a to the output filename

*outgrid*.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.

## Tiles¶

For very large datasets (or very large plots) you may need to break the job into multiple
tiles. It is then important that the normalization of the intensities are handled the
same way for each tile. By default, *offset* and *sigma* are recalculated for each tile.
Hence, different tiles of the same large grid will compute different *offset* and *sigma* values.
Thus, the intensity for the same directional slope will be different across the final map.
This inconsistency can lead to visible changes in image appearance across tile seams.
The way to ensure compatible results is to specify the same *offset* and *sigma* via
the modifiers to **-N**. However, if these need to be estimated from the large grid then
the **-Q** option can help: Run **grdgradient** on the full grid (or as large portion of
the grid that your computer can handle) and specify **-Qc** to create a statistics file
with the resulting *offset* and *sigma*. Then, for each of your grid tile calculations, give
**+o** and/or **+s** without arguments to **-N** and specify **-Qr**. This option will read
the values from the hidden statistics file and use them in the normalization.
If you use **-QR** for the final tile then the statistics file is removed after use.

## Ambient¶

The *ambient* light offset is used to darken or brighten all intensities. This
modifier is typically used to darken an entire image by subtracting a constant from
all the intensities. E.g., if you use **+a**-0.5 then you subtract 0.5 from all
intensities, making them more negative and hence darken the image.

## Special Effects¶

Users who wishes to highlight just an area of a grid are encouraged to consider creative uses of the vast number of operators in grdmath and the grid clipping schemes in grdmask and grdclip. Many separate intensity grids can be combined into one via grid algebra and boolean operators in grdmath. The sky is the limit.

## Examples¶

**Note**: Below are some examples of valid syntax for this module.
The examples that use remote files (file names starting with `@`

)
can be cut and pasted into your terminal for testing.
Other commands requiring input files are just dummy examples of the types
of uses that are common but cannot be run verbatim as written.

To make a file for illuminating a portion of the data in the remote file @earth_relief_05 using exponentially normalized gradients in the range [-0.6,0.6] imitating light sources in the north and west directions:

```
gmt grdgradient @earth_relief_05m -R0/20/0/20 -A0/270 -Ggradients.nc -Ne0.6 -V
```

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

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

To determine the offset and sigma suitable for normalizing the intensities from topo.nc, do

gmt grdgradient topo.nc -A30 -Nt0.6 -Qc -V

Without **-G**, only the hidden statistics file is created and no output grid is written.

To use the previously determined offset and sigma to normalize the intensities in tile_3.nc, do

gmt grdgradient tile_3.nc -A30 -Nt0.6+o+s -Qr -V -Gtile_3_int.nc

## 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, grdinfo, grdmath, grdimage, grdview, grdvector