sph2grd

Compute grid from spherical harmonic coefficients

Synopsis

gmt sph2grd [ table ] -Ggrdfile -Iincrement -Rregion [ -D[g|n] ] [ -E ] [ -F[k]filter ] [ -Ng|m|s ] [ -Q ] [ -V[level] ] [ -bibinary ] [ -hheaders ] [ -iflags ] [ -rreg ] [ -x[[-]n] ] [ --PAR=value ]

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

Description

sph2grd reads a spherical harmonics coefficient table with records of L, M, C[L,M], S[L,M] and evaluates the spherical harmonic model on the specified grid.

Required Arguments

table

One or more ASCII [or binary, see -bi] files holding the spherical harmonic coefficients. We expect the first four columns to hold the degree L, the order M, followed by the cosine and sine coefficients.

-Ggrdfile

grdfile is the name of the binary output grid file. (See Grid File Formats).

-Ixinc[+e|n][/yinc[+e|n]]

x_inc [and optionally y_inc] is the grid spacing. Geographical (degrees) coordinates: Optionally, append an increment unit. Choose among 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, the registration, and the domain. The resulting increment value depends on whether you have selected a gridline-registered or pixel-registered grid; see GMT File Formats for details. Note: If -Rgrdfile is used then the grid spacing and the registration have already been initialized; use -I and -r to override these values.

-Rxmin/xmax/ymin/ymax[+r][+uunit]

Specify the region of interest. (See full description) (See cookbook information).

Optional Arguments

-D[g|n]

Will evaluate a derived field from a geopotential model. Choose between Dg which will compute the gravitational field or Dn to compute the geoid [Add -E for anomalies on the ellipsoid].

-E

Evaluate expansion on the current ellipsoid [Default is sphere].

-F[k]filter

Filter coefficients according to one of two kinds of filter specifications:. Select -Fk if values are given in km [Default is coefficient harmonic degree L]. a) Cosine band-pass: Append four wavelengths lc/lp/hp/hc. Coefficients outside lc/hc are cut; those inside lp/hp are passed, while the rest are tapered. Replace wavelength by - to skip, e.g., -F-/-/50/75 is a low-pass filter. b) Gaussian band-pass: Append two wavelengths lo/hi where filter amplitudes = 0.5. Replace wavelength by - to skip, e.g., -F70/- is a high-pass Gaussian filter.

-Ng|m|s

Normalization used for coefficients. Choose among m: Mathematical normalization - inner products summed over surface equal 1 [Default]. g Geodesy normalization - inner products summed over surface equal 4pi. s: Schmidt normalization - as used in geomagnetism.

-V[level]

Select verbosity level [w]. (See full description) (See cookbook information).

-birecord[+b|l] (more …)

Select native binary format for primary table input. [Default is 4 input columns].

-h[i|o][n][+c][+d][+msegheader][+rremark][+ttitle] (more …)

Skip or produce header record(s). Not used with binary data.

-icols[+l][+ddivisor][+sscale][+ooffset][,…][,t[word]] (more …)

Select input columns and transformations (0 is first column, t is trailing text, append word to read one word only).

-r[g|p] (more …)

Set node registration [gridline].

-x[[-]n] (more …)

Limit number of cores used in multi-threaded algorithms (OpenMP required).

-^ 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 arguments

Print 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.

Geographical And Time Coordinates

When the output grid type is netCDF, the coordinates will be labeled “longitude”, “latitude”, or “time” based on the attributes of the input data or grid (if any) or on the -f or -R options. For example, both -f0x -f1t and -R90w/90e/0t/3t will result in a longitude/time grid. When the x, y, or z coordinate is time, it will be stored in the grid as relative time since epoch as specified by TIME_UNIT and TIME_EPOCH in the gmt.conf file or on the command line. In addition, the unit attribute of the time variable will indicate both this unit and epoch.

Examples

To create a 1 x 1 degree global grid file from the ASCII coefficients in the remote file EGM96_to_36.txt, use

gmt sph2grd @EGM96_to_36.txt -GEGM96_to_36.nc -Rg -I1 -V

Reference

Holmes, S. A., and Featherstone, W. E., 2002, A unified approach to the Clenshaw summation and the recursive computation of very high degree and order normalized associated Legendre functions: J. Geodesy, v. 76, p. 279-299.

See Also

gmt, grdfft, grdmath