# surface¶

Grid table data using adjustable tension continuous curvature splines

## Synopsis¶

**gmt surface** [ *table* ] **-G***outgrid*
**-I***increment*
**-R***region*
[ **-A***aspect_ratio*|**m** ]
[ **-C***convergence_limit*[%] ]
[ **-J***parameters* ]
[ **-D***breakline_file*[**+z**[*level*]] ]
[ **-L****l***lower* ] [ **-L****u***upper* ]
[ **-M***max_radius* ]
[ **-N***max_iterations* ]
[ **-Q** ]
[ **-S***search_radius*[**m**|**s**] ]
[ **-T**[**b**|**i**]*tension_factor* ]
[ **-V**[*level*] ]
[ **-W**[*logfile*] ]
[ **-Z***over-relaxation_factor* ]
[ **-a**flags ]
[ **-bi**binary ]
[ **-di**[**+c***col*]nodata ]
[ **-e**regexp ]
[ **-f**flags ]
[ **-h**headers ]
[ **-i**flags ]
[ **-qi**flags ]
[ **-r**reg ]
[ **-w**flags ]
[ **-:**[**i**|**o**] ]
[ **--PAR**=*value* ]

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

## Description¶

**surface** reads randomly-spaced (x,y,z) triples from standard input
[or *table*] and produces a binary grid file of gridded values z(x,y) by
solving the differential equation (away from data points)

where *t* is a tension factor between 0 and 1, and \(\nabla\) indicates the
Laplacian operator. Here, *t* = 0 gives the “minimum curvature” solution which
is equivalent to SuperMISP and the ISM packages. Minimum curvature can
cause undesired oscillations and false local maxima or minima (See Smith
and Wessel, 1990), and you may wish to use *t* > 0 to suppress these
effects. Experience suggests *t* ~ 0.25 usually looks good for potential
field data and *t* should be larger (*t* ~ 0.35) for steep topography data.
*t* = 1 gives a harmonic surface (no maxima or minima are possible except
at control data points). It is recommended that the user pre-process the
data with blockmean, blockmedian, or blockmode to avoid
spatial aliasing and eliminate redundant data. You may impose lower
and/or upper bounds on the solution. These may be entered in the form of
a fixed value, a grid with values, or simply be the minimum/maximum
input data values. Natural boundary conditions are applied at the edges,
except for geographic data with 360-degree range where we apply periodic
boundary conditions in the longitude direction.

## Required Arguments¶

*table*One or more ASCII (or binary, see

**-bi**[*ncols*][*type*]) data table file(s) holding a number of data columns. If no tables are given then we read from standard input.

**-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. Note that the smallest grid dimension must be at least 4. 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.

**-I***x_inc*[**+e**|**n**][/*y_inc*[**+e**|**n**]]Set the grid spacing as

*x_inc*[and optionally*y_inc*].**Geographical (degrees) coordinates**: Optionally, append an increment unit. Choose among:**m**to indicate arc minutes**s**to indicate arc seconds**e**(meter),**f**(foot),**k**(km),**M**(mile),**n**(nautical mile) or**u**(US survey foot), in which case the increment 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**: The following modifiers are supported:**+e**to slightly adjust the max*x*(*east*) or*y*(*north*) to fit exactly the given increment if needed [Default is to slightly adjust the increment to fit the given domain].**+n**to define the*number of nodes*rather than the increment, in which case the increment is recalculated from the number of nodes, the*registration*(see GMT File Formats), and the domain.**Note**: If**-R***grdfile*is used then the grid spacing and the registration have already been initialized; use**-I**and**-R**to override these values.

**-R***xmin*/*xmax*/*ymin*/*ymax*[**+r**][**+u***unit*]Specify the region of interest. (See full description) (See cookbook information).

## Optional Arguments¶

**-A***aspect_ratio*|**m**Aspect ratio. If desired, grid anisotropy can be added to the equations. Enter

*aspect_ratio*, where dy = dx /*aspect_ratio*relates the grid dimensions. For geographic data, you may use**-Am**to set the aspect ratio to the cosine of the mean latitude [Default = 1 assumes isotropic grid.]

**-C***convergence_limit*[%]Convergence limit. Iteration is assumed to have converged when the maximum absolute change in any grid value is less than

*convergence_limit*. (Units same as data z units). Alternatively, give limit in percentage of rms deviation by appending %. [Default is scaled to \(10^{-4}\) of the root-mean-square deviation of the data from a best-fit (least-squares) plane.]. This is the final convergence limit at the desired grid spacing; for intermediate (coarser) grids the effective convergence limit is divided by the grid spacing multiplier.

**-J***parameters*Specify the projection. Select the data map projection. This projection is only used to add a referencing info to the grid formats that support it. E.g. netCDF, GeoTIFF, and others supported by GDAL.

**-D***breakline*[**+z**[*level*]]Use xyz data in the

*breakline*file as a ‘soft breakline’. A ‘soft breakline’ is a line whose vertices will be used to constrain the nearest grid nodes without any further interpolation. A coastline or a lake shore are good examples of ‘soft breaklines’. Multi-segments files are accepted. If your lines do not have*z*-values or you wish to override those with a constant z-value, then append**+z***level*to the filename. If no value is given then we default to 0.

**-Ll***lower*and**-Lu***upper*Impose limits on the output solution.

**l***lower*sets the lower bound.*lower*can be the name of a grid file with lower bound values, a fixed value,**d**to set to minimum input value, or**u**for unconstrained [Default].**u***upper*sets the upper bound and can be the name of a grid file with upper bound values, a fixed value,**d**to set to maximum input value, or**u**for unconstrained [Default]. Grid files used to set the limits may contain NaNs. In the presence of NaNs, the limit of a node masked with NaN is unconstrained.

**-M***max_radius*After solving for the surface, apply a mask so that nodes farther than

*max_radius*away from a data constraint is set to NaN [no masking]. Append a distance unit (see Units) if needed. One can also select the nodes to mask by using the**-M***n_cells***c**form. Here*n_cells*means the number of cells around the node controlled by a data point. As an example**-M0c**means that only the cell where point lies is filled,**-M1c**keeps one cell beyond that (i.e. makes a 3x3 neighborhood), and so on.

**-N***max_iterations*Number of iterations. Iteration will cease when

*convergence_limit*is reached or when number of iterations reaches*max_iterations*. This is the final iteration limit at the desired grid spacing; for intermediate (coarser) grids the effective iteration limit is scaled by the grid spacing multiplier [Default is 500].

**-Q**Suggest grid dimensions which have a highly composite greatest common factor. This allows surface to use several intermediate steps in the solution, yielding faster run times and better results. The sizes suggested by

**-Q**can be achieved by altering**-R**and/or**-I**. You can recover the**-R**and**-I**you want later by using grdsample or grdcut on the output of**surface**.

**-S***search_radius*[**m**|**s**]Search radius. Enter

*search_radius*in same units as x,y data; append**m**to indicate arc minutes or**s**for arc seconds. This is used to initialize the grid before the first iteration; it is not worth the time unless the grid lattice is prime and cannot have regional stages. [Default = 0.0 and no search is made.]

**-T**[**b**|**i**]*tension_factor*Tension factor[s]. These must be between 0 and 1. Tension may be used in the interior solution (above equation, where it suppresses spurious oscillations) and in the boundary conditions (where it tends to flatten the solution approaching the edges). Using zero for both values results in a minimum curvature surface with free edges, i.e., a natural bicubic spline. Use

**-Ti***tension_factor*to set interior tension, and**-Tb***tension_factor*to set boundary tension. If you do not prepend**i**or**b**, both will be set to the same value. [Default = 0 for both gives minimum curvature solution.]

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

**w**].**-V3**will report the convergence after each iteration;**-V**will report only after each regional grid is converged. (See full description) (See cookbook information).

**-W**[*logfile*]Write convergence information to

*logfile*[Default is*surface_log.txt*].

**-Z***over-relaxation_factor*Over-relaxation factor. This parameter is used to accelerate the convergence; it is a number between 1 and 2. A value of 1 iterates the equations exactly, and will always assure stable convergence. Larger values overestimate the incremental changes during convergence, and will reach a solution more rapidly but may become unstable. If you use a large value for this factor, it is a good idea to monitor each iteration with the

**-Vi**option. [Default = 1.4 converges quickly and is almost always stable.]

**-a**[[*col*=]*name*[,*…*]] (more …)Set aspatial column associations

*col*=*name*.

**-bi***record*[**+b**|**l**] (more …)Select native binary format for primary table input. [Default is 3 input columns].

**-di***nodata*[**+c***col*] (more …)Replace input columns that equal

*nodata*with NaN.

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

**-f**[**i**|**o**]*colinfo*(more …)Specify data types of input and/or output columns.

**-h**[**i**|**o**][*n*][**+c**][**+d**][**+m***segheader*][**+r***remark*][**+t***title*] (more …)Skip or produce header record(s). Not used with binary data.

**-i***cols*[**+l**][**+d***divisor*][**+s***scale*|**d**|**k**][**+o***offset*][,*…*][,**t**[*word*]] (more …)Select input columns and transformations (0 is first column,

**t**is trailing text, append*word*to read one word only).

**-qi**[~]*rows*|*limits*[**+c***col*][**+a**|**f**|**s**] (more …)Select input rows or data limit(s) [default is all rows].

**-r**[**g**|**p**] (more …)Set node registration [gridline].

**-wy**|**a**|**w**|**d**|**h**|**m**|**s**|**c***period*[/*phase*][**+c***col*] (more …)Convert an input coordinate to a cyclical coordinate.

**-:**[**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 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 Values Precision¶

Regardless of the precision of the input data, GMT programs that create grid files will internally hold the grids in 4-byte floating point arrays. This is done to conserve memory and furthermore most if not all real data can be stored using 4-byte floating point values. Data with higher precision (i.e., double precision values) will lose that precision once GMT operates on the grid or writes out new grids. To limit loss of precision when processing data you should always consider normalizing the data prior to processing.

## 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 (**-jg**) using the authalic radius
(see PROJ_MEAN_RADIUS). You can use **-jf** to perform
“Flat Earth” calculations (quicker but less accurate) or **-je** to perform
exact geodesic calculations (slower but more accurate; see
PROJ_GEODESIC for method used).

## 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 grid 5 by 5 minute gravity block means from the ASCII data in
hawaii_5x5.xyg, using a *tension_factor* = 0.25, a
*convergence_limit* = 0.1 milligal, writing the result to a file called
hawaii_grd.nc, and monitoring each iteration, try:

gmt surface hawaii_5x5.xyg -R198/208/18/25 -I5m -Ghawaii_grd.nc -T0.25 -C0.1 -Vi

## Gridding Geographic Data: Boundary Conditions¶

The surface finite difference algorithm is Cartesian at heart, hence the *ad hoc*
option to change the aspect ratio for a suitable mean latitude (**-A**). When
geographic data are supplied and the output grid has a 360 degree longitude range we will
impose periodic boundary conditions in longitude. However, no equivalent geographic
boundary condition can be applied at the poles since the finite difference solution
will not be valid there (actual spacing between the nodes at the poles is zero).
If you attempt this type of gridding you will be severely warned but the calculations
will continue. Because the result is a geographic grid, the GMT i/o machinery will
interfere and detect inconsistencies at the pole points and replace all values along
a pole with their mean value. This will introduce further distortion into the
grid near the poles. We recommend you instead consider spherical gridding for global
data sets; see greenspline (for modest data sets) or sphinterpolate.

## Gridding Geographic Data: Setting Increments¶

Specifying grid increments in distance units (meters, km, etc.) for geographic (lon, lat)
grids triggers a conversion from the given increment to the equivalent increment in degrees.
This is done differently for longitude and latitude and also depends on chosen ellipsoid,
but ultimately is a great-circle approximation. For latitude we divide your *y*-increment
with the number of you chosen unit per degree latitude, while for longitude we divide your
*x*-increment by the number of such units per degree along the mid-parallel in your region. The
resulting degree increments may therefore not exactly match the increments you entered explicitly.
Hence, there may be rounding off in ways you don’t want and cannot easily control, resulting in prime grid
dimensions. You can handle the situation via **-Q** but with the never-ending decimals in some
increments that is still a challenge. Another approach is to *not* grid geographic data
using length units as increments, due to the above conversion. It may be cleaner to specify
grid intervals in spherical degrees, minutes or seconds. That way you can control the grid
dimensions directly and avoid the round-off. Alternatively, if your region is far from Equator
and your are concerned about the difference in longitude and latitude increments in degrees
you could project all data to a local projection (e.g., UTM) to yield units of meters, and then
grid the projected data using meters as the final grid increment. Either approach avoids
“ugly” increments like 0.161697s and will let you specify intervals that are easily divisible
into the range. If increment choice is dictated by a need for a desired increment in meters
then the projection route will yield better results.

## Bugs¶

**surface** will complain when more than one data point is found for any
node and suggest that you run blockmean, blockmedian, or
blockmode first. If you did run these decimators and still get this
message it usually means that your grid spacing is so small that you
need more decimals in the output format used. You may
specify more decimal places by editing the parameter
FORMAT_FLOAT_OUT in your gmt.conf file prior to running
the decimators or choose binary input and/or output using single or
double precision storage.

Note that only gridline registration is possible with **surface**. If
you need a pixel-registered grid you can resample a gridline registered
grid using grdsample **-T**.

## See Also¶

blockmean, blockmedian, blockmode, gmt, grdcut, grdsample, greenspline, nearneighbor, triangulate, sphinterpolate

## References¶

Smith, W. H. F, and P. Wessel, 1990, Gridding with continuous curvature
splines in tension, *Geophysics*, 55, 293-305.