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|
- .. index:: ! grdmath
- .. include:: module_core_purpose.rst_
- *******
- grdmath
- *******
- |grdmath_purpose|
- Synopsis
- --------
- .. include:: common_SYN_OPTs.rst_
- **gmt grdmath**
- [ |SYN_OPT-Area| ]
- [ |-D|\ *resolution*\ [**+f**] ]
- [ |SYN_OPT-I| ]
- [ |-M| ] [ |-N| ]
- [ |SYN_OPT-R| ]
- [ |-S| ]
- [ |SYN_OPT-V| ]
- [ |SYN_OPT-a| ]
- [ |SYN_OPT-bi| ]
- [ |SYN_OPT-di| ]
- [ |SYN_OPT-f| ]
- [ |SYN_OPT-h| ]
- [ |SYN_OPT-i| ]
- [ |SYN_OPT-n| ]
- [ |SYN_OPT-r| ]
- [ |SYN_OPT-x| ]
- [ |SYN_OPT--| ]
- *operand* [ *operand* ] **OPERATOR** [ *operand* ]
- **OPERATOR** ... **=** *outgrdfile*
- |No-spaces|
- Description
- -----------
- **grdmath** will perform operations like add, subtract, multiply, and
- hundreds of other operands on one or more grid files or constants using
- `Reverse Polish Notation (RPN) <https://en.wikipedia.org/wiki/Reverse_Polish_notation>`_
- syntax. Arbitrarily complicated expressions may therefore be evaluated; the
- final result is written to an output grid file. Grid operations are
- element-by-element, not matrix manipulations. Some operators only
- require one operand (see below). If no grid files are used in the
- expression then options **-R**, **-I** must be set (and optionally
- |SYN_OPT-r|). The expression **=** *outgrdfile* can occur as many times as
- the depth of the stack allows in order to save intermediate results.
- Complicated or frequently occurring expressions may be coded as a macro
- for future use or stored and recalled via named memory locations.
- Required Arguments
- ------------------
- *operand*
- If *operand* can be opened as a file it will be read as a grid file.
- If not a file, it is interpreted as a numerical constant or a
- special symbol (see below).
- *outgrdfile*
- The name of a 2-D grid file that will hold the final result. (See
- GRID FILE FORMATS below).
- Optional Arguments
- ------------------
- .. _-A:
- .. |Add_-A| replace:: (**-A** is only relevant to the **LDISTG** operator)
- .. include:: explain_-A.rst_
- .. _-D:
- **-D**\ *resolution*\ [**+f**]
- Selects the resolution of the data set to use with the operator LDISTG
- ((**f**)ull, (**h**)igh, (**i**)ntermediate, (**l**)ow, and (**c**)rude). The
- resolution drops off by 80% between data sets [Default is **l**].
- Append **+f** to automatically select a lower resolution should the one
- requested not be available [abort if not found].
- .. _-I:
- .. include:: explain_-I.rst_
- .. _-M:
- **-M**
- By default any derivatives calculated are in z_units/x(or
- y)\_units. However, the user may choose this option to convert dx,dy
- in degrees of longitude,latitude into meters using a flat Earth
- approximation, so that gradients are in z_units/meter.
- .. _-N:
- **-N**
- Turn off strict domain match checking when multiple grids are
- manipulated [Default will insist that each grid domain is within
- 1e-4 \* grid_spacing of the domain of the first grid listed].
- .. _-R:
- .. |Add_-R| unicode:: 0x20 .. just an invisible code
- .. include:: explain_-R.rst_
- .. _-S:
- **-S**
- Reduce (i.e., collapse) the entire stack to a single grid by applying the
- next operator to all co-registered nodes across the entire stack. You
- must specify **-S** *after* listing all of your grids. **Note**: You can only
- follow **-S** with a reducing operator, i.e., from the list ADD, AND, MAD,
- LMSSCL, MAX, MEAN, MEDIAN, MIN, MODE, MUL, RMS, STD, SUB, VAR or XOR.
- .. _-V:
- .. |Add_-V| unicode:: 0x20 .. just an invisible code
- .. include:: explain_-V.rst_
- .. include:: explain_-aspatial.rst_
- .. |Add_-bi| replace:: The binary input option
- only applies to the data files needed by operators **LDIST**,
- **PDIST**, and **INSIDE**.
- .. include:: explain_-bi.rst_
- .. |Add_-di| unicode:: 0x20 .. just an invisible code
- .. include:: explain_-di.rst_
- .. |Add_-f| unicode:: 0x20 .. just an invisible code
- .. include:: explain_-f.rst_
- .. |Add_-g| unicode:: 0x20 .. just an invisible code
- .. include:: explain_-g.rst_
- .. |Add_-h| unicode:: 0x20 .. just an invisible code
- .. include:: explain_-h.rst_
- .. include:: explain_-icols.rst_
- .. include:: explain_-n.rst_
- .. |Add_nodereg| replace:: Only used with **-R** **-I**.
- .. include:: explain_nodereg.rst_
- .. include:: explain_core.rst_
- .. include:: explain_help.rst_
- Operators
- ---------
- Choose among the following 224 operators. "args" are the number of input
- and output arguments.
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | Operator | args | Returns |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ABS** | 1 1 | abs (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ACOS** | 1 1 | acos (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ACOSH** | 1 1 | acosh (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ACOT** | 1 1 | acot (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ACSC** | 1 1 | acsc (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ADD** | 2 1 | A + B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **AND** | 2 1 | B if A == NaN, else A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ARC** | 2 1 | Return arc(A,B) on [0 pi] |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **AREA** | 0 1 | Area of each gridnode cell (in km^2 if geographic) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ASEC** | 1 1 | asec (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ASIN** | 1 1 | asin (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ASINH** | 1 1 | asinh (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ATAN** | 1 1 | atan (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ATAN2** | 2 1 | atan2 (A, B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ATANH** | 1 1 | atanh (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BCDF** | 3 1 | Binomial cumulative distribution function for p = A, n = B, and x = C |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BPDF** | 3 1 | Binomial probability density function for p = A, n = B, and x = C |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BEI** | 1 1 | bei (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BER** | 1 1 | ber (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BITAND** | 2 1 | A & B (bitwise AND operator) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BITLEFT** | 2 1 | A << B (bitwise left-shift operator) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BITNOT** | 1 1 | ~A (bitwise NOT operator, i.e., return two's complement) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BITOR** | 2 1 | A \| B (bitwise OR operator) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BITRIGHT** | 2 1 | A >> B (bitwise right-shift operator) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BITTEST** | 2 1 | 1 if bit B of A is set, else 0 (bitwise TEST operator) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BITXOR** | 2 1 | A ^ B (bitwise XOR operator) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **BLEND** | 3 1 | Blend A and B using weights in C (0-1 range) as A*C + B*(1-C) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CAZ** | 2 1 | Cartesian azimuth from grid nodes to stack x,y (i.e., A, B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CBAZ** | 2 1 | Cartesian back-azimuth from grid nodes to stack x,y (i.e., A, B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CDIST** | 2 1 | Cartesian distance between grid nodes and stack x,y (i.e., A, B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CDIST2** | 2 1 | As CDIST but only to nodes that are != 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CEIL** | 1 1 | ceil (A) (smallest integer >= A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CHICRIT** | 2 1 | Chi-squared critical value for alpha = A and nu = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CHICDF** | 2 1 | Chi-squared cumulative distribution function for chi2 = A and nu = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CHIPDF** | 2 1 | Chi-squared probability density function for chi2 = A and nu = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **COMB** | 2 1 | Combinations n_C_r, with n = A and r = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CORRCOEFF** | 2 1 | Correlation coefficient r(A, B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **COS** | 1 1 | cos (A) (A in radians) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **COSD** | 1 1 | cos (A) (A in degrees) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **COSH** | 1 1 | cosh (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **COT** | 1 1 | cot (A) (A in radians) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **COTD** | 1 1 | cot (A) (A in degrees) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CSC** | 1 1 | csc (A) (A in radians) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CSCD** | 1 1 | csc (A) (A in degrees) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **CURV** | 1 1 | Curvature of A (Laplacian) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **D2DX2** | 1 1 | d^2(A)/dx^2 2nd derivative |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **D2DY2** | 1 1 | d^2(A)/dy^2 2nd derivative |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **D2DXY** | 1 1 | d^2(A)/dxdy 2nd derivative |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **D2R** | 1 1 | Converts Degrees to Radians |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **DDX** | 1 1 | d(A)/dx Central 1st derivative |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **DAYNIGHT** | 3 1 | 1 where sun at (A, B) shines and 0 elsewhere, with C transition width |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **DDY** | 1 1 | d(A)/dy Central 1st derivative |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **DEG2KM** | 1 1 | Converts Spherical Degrees to Kilometers |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **DENAN** | 2 1 | Replace NaNs in A with values from B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **DILOG** | 1 1 | dilog (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **DIV** | 2 1 | A / B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **DOT** | 2 1 | 2-D (Cartesian) or 3-D (geographic) dot products between nodes and stack (A, B) unit vector(s) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **DUP** | 1 2 | Places duplicate of A on the stack |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ECDF** | 2 1 | Exponential cumulative distribution function for x = A and lambda = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ECRIT** | 2 1 | Exponential distribution critical value for alpha = A and lambda = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **EPDF** | 2 1 | Exponential probability density function for x = A and lambda = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ERF** | 1 1 | Error function erf (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ERFC** | 1 1 | Complementary Error function erfc (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **EQ** | 2 1 | 1 if A == B, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ERFINV** | 1 1 | Inverse error function of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **EXCH** | 2 2 | Exchanges A and B on the stack |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **EXP** | 1 1 | exp (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **FACT** | 1 1 | A! (A factorial) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **EXTREMA** | 1 1 | Local Extrema: +2/-2 is max/min, +1/-1 is saddle with max/min in x, 0 elsewhere |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **FCDF** | 3 1 | F cumulative distribution function for F = A, nu1 = B, and nu2 = C |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **FCRIT** | 3 1 | F distribution critical value for alpha = A, nu1 = B, and nu2 = C |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **FLIPLR** | 1 1 | Reverse order of values in each row |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **FLIPUD** | 1 1 | Reverse order of values in each column |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **FLOOR** | 1 1 | floor (A) (greatest integer <= A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **FMOD** | 2 1 | A % B (remainder after truncated division) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **FPDF** | 3 1 | F probability density function for F = A, nu1 = B, and nu2 = C |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **GE** | 2 1 | 1 if A >= B, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **GT** | 2 1 | 1 if A > B, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **HSV2RGB** | 3 3 | Convert h,s,v triplets to r,g,b triplets, with h = A (0-360), s = B and v = C (both in 0-1) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **HSV2RGB** | 3 3 | Convert h,s,v triplets to r,g,b triplets, with h = A (0-360), s = B and v = C (0-1) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **HSV2XYZ** | 3 3 | Convert h,s,v triplets to x,t,z triplets, with h = A (0-360), s = B and v = C (0-1) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **HYPOT** | 2 1 | hypot (A, B) = sqrt (A\*A + B\*B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **I0** | 1 1 | Modified Bessel function of A (1st kind, order 0) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **I1** | 1 1 | Modified Bessel function of A (1st kind, order 1) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **IFELSE** | 3 1 | B if A != 0, else C |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **IN** | 2 1 | Modified Bessel function of A (1st kind, order B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **INRANGE** | 3 1 | 1 if B <= A <= C, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **INSIDE** | 1 1 | 1 when inside or on polygon(s) in A, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **INV** | 1 1 | 1 / A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ISFINITE** | 1 1 | 1 if A is finite, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ISNAN** | 1 1 | 1 if A == NaN, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **J0** | 1 1 | Bessel function of A (1st kind, order 0) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **J1** | 1 1 | Bessel function of A (1st kind, order 1) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **JN** | 2 1 | Bessel function of A (1st kind, order B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **K0** | 1 1 | Modified Kelvin function of A (2nd kind, order 0) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **K1** | 1 1 | Modified Bessel function of A (2nd kind, order 1) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **KEI** | 1 1 | kei (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **KER** | 1 1 | ker (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **KM2DEG** | 1 1 | Converts Kilometers to Spherical Degrees |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **KN** | 2 1 | Modified Bessel function of A (2nd kind, order B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **KURT** | 1 1 | Kurtosis of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LAB2HSV** | 3 3 | Convert l,a,b triplets to h,s,v triplets |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LAB2RGB** | 3 3 | Convert l,a,b triplets to r,g,b triplets |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LAB2XYZ** | 3 3 | Convert l,a,b triplets to x,y,z triplets |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LCDF** | 1 1 | Laplace cumulative distribution function for z = A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LCRIT** | 1 1 | Laplace distribution critical value for alpha = A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LDIST** | 1 1 | Compute minimum distance (in km if -fg) from lines in multi-segment ASCII file A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LDIST2** | 2 1 | As LDIST, from lines in ASCII file B but only to nodes where A != 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LDISTG** | 0 1 | As LDIST, but operates on the GSHHG dataset (see -A, -D for options). |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LE** | 2 1 | 1 if A <= B, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LOG** | 1 1 | log (A) (natural log) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LOG10** | 1 1 | log10 (A) (base 10) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LOG1P** | 1 1 | log (1+A) (accurate for small A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LOG2** | 1 1 | log2 (A) (base 2) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LMSSCL** | 1 1 | LMS (Least Median of Squares) scale estimate (LMS STD) of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LMSSCLW** | 2 1 | Weighted LMS (Least Median of Squares) scale estimate (LMS STD) of A for weights in B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LOWER** | 1 1 | The lowest (minimum) value of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LPDF** | 1 1 | Laplace probability density function for z = A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LRAND** | 2 1 | Laplace random noise with mean A and std. deviation B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **LT** | 2 1 | 1 if A < B, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MAD** | 1 1 | Median Absolute Deviation (L1 STD) of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MAX** | 2 1 | Maximum of A and B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MEAN** | 1 1 | Mean value of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MEANW** | 2 1 | Weighted mean value of A for weights in B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MEDIAN** | 1 1 | Median value of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MEDIANW** | 2 1 | Weighted median value of A for weights in B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MIN** | 2 1 | Minimum of A and B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MOD** | 2 1 | A mod B (remainder after floored division) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MODE** | 1 1 | Mode value (Least Median of Squares) of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MODEW** | 2 1 | Weighted mode value (Least Median of Squares) of A for weights in B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **MUL** | 2 1 | A \* B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **NAN** | 2 1 | NaN if A == B, else A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **NEG** | 1 1 | -A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **NEQ** | 2 1 | 1 if A != B, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **NORM** | 1 1 | Normalize (A) so max(A)-min(A) = 1 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **NOT** | 1 1 | NaN if A == NaN, 1 if A == 0, else 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **NRAND** | 2 1 | Normal, random values with mean A and std. deviation B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **OR** | 2 1 | NaN if B == NaN, else A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PCDF** | 2 1 | Poisson cumulative distribution function for x = A and lambda = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PDIST** | 1 1 | Compute minimum distance (in km if -fg) from points in ASCII file A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PDIST2** | 2 1 | As PDIST, from points in ASCII file B but only to nodes where A != 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PERM** | 2 1 | Permutations n_P_r, with n = A and r = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PLM** | 3 1 | Associated Legendre polynomial P(A) degree B order C |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PLMg** | 3 1 | Normalized associated Legendre polynomial P(A) degree B order C (geophysical convention) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **POINT** | 1 2 | Compute mean x and y from ASCII file A and place them on the stack |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **POP** | 1 0 | Delete top element from the stack |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **POW** | 2 1 | A ^ B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PPDF** | 2 1 | Poisson distribution P(x,lambda), with x = A and lambda = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PQUANT** | 2 1 | The B'th Quantile (0-100%) of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PQUANTW** | 3 1 | The C'th weighted quantile (0-100%) of A for weights in B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PSI** | 1 1 | Psi (or Digamma) of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **PV** | 3 1 | Legendre function Pv(A) of degree v = real(B) + imag(C) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **QV** | 3 1 | Legendre function Qv(A) of degree v = real(B) + imag(C) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **R2** | 2 1 | R2 = A^2 + B^2 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **R2D** | 1 1 | Convert Radians to Degrees |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **RAND** | 2 1 | Uniform random values between A and B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **RCDF** | 1 1 | Rayleigh cumulative distribution function for z = A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **RCRIT** | 1 1 | Rayleigh distribution critical value for alpha = A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **RGB2HSV** | 3 3 | Convert r,g,b triplets to h,s,v triplets, with r = A, g = B, and b = C (all in 0-255 range) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **RGB2LAB** | 3 3 | Convert r,g,b triplets to l,a,b triplets, with r = A, g = B, and b = C (in 0-255 range) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **RGB2XYZ** | 3 3 | Convert r,g,b triplets to x,y,x triplets, with r = A, g = B, and b = C (in 0-255 range) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **RINT** | 1 1 | rint (A) (round to integral value nearest to A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **RMS** | 1 1 | Root-mean-square of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **RMSW** | 1 1 | Root-mean-square of A for weights in B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **RPDF** | 1 1 | Rayleigh probability density function for z = A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ROLL** | 2 0 | Cyclicly shifts the top A stack items by an amount B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ROTX** | 2 1 | Rotate A by the (constant) shift B in x-direction |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ROTY** | 2 1 | Rotate A by the (constant) shift B in y-direction |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SDIST** | 2 1 | Spherical (Great circle|geodesic) distance (in km) between nodes and stack (A, B) |ex_SDIST| |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SDIST2** | 2 1 | As SDIST but only to nodes that are != 0 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SAZ** | 2 1 | Spherical azimuth from grid nodes to stack lon, lat (i.e., A, B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SBAZ** | 2 1 | Spherical back-azimuth from grid nodes to stack lon, lat (i.e., A, B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SEC** | 1 1 | sec (A) (A in radians) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SECD** | 1 1 | sec (A) (A in degrees) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SIGN** | 1 1 | sign (+1 or -1) of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SIN** | 1 1 | sin (A) (A in radians) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SINC** | 1 1 | sinc (A) (sin (pi\*A)/(pi\*A)) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SIND** | 1 1 | sin (A) (A in degrees) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SINH** | 1 1 | sinh (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SKEW** | 1 1 | Skewness of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SQR** | 1 1 | A^2 |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SQRT** | 1 1 | sqrt (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **STD** | 1 1 | Standard deviation of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **STDW** | 2 1 | Weighted standard deviation of A for weights in B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **STEP** | 1 1 | Heaviside step function: H(A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **STEPX** | 1 1 | Heaviside step function in x: H(x-A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **STEPY** | 1 1 | Heaviside step function in y: H(y-A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SUB** | 2 1 | A - B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **SUM** | 1 1 | Sum of all values in A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **TAN** | 1 1 | tan (A) (A in radians) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **TAND** | 1 1 | tan (A) (A in degrees) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **TANH** | 1 1 | tanh (A) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **TAPER** | 2 1 | Unit weights cosine-tapered to zero within A and B of x and y grid margins |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **TCDF** | 2 1 | Student's t cumulative distribution function for t = A, and nu = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **TCRIT** | 2 1 | Student's t distribution critical value for alpha = A and nu = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **TN** | 2 1 | Chebyshev polynomial Tn(-1<t<+1,n), with t = A, and n = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **TPDF** | 2 1 | Student's t probability density function for t = A, and nu = B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **TRIM** | 3 1 | Alpha-trim C to NaN if values fall in tails A and B (in percentage) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **UPPER** | 1 1 | The highest (maximum) value of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **VAR** | 1 1 | Variance of A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **VARW** | 2 1 | Weighted variance of A for weights in B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **WCDF** | 3 1 | Weibull cumulative distribution function for x = A, scale = B, and shape = C |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **WCRIT** | 3 1 | Weibull distribution critical value for alpha = A, scale = B, and shape = C |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **WPDF** | 3 1 | Weibull density distribution P(x,scale,shape), with x = A, scale = B, and shape = C |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **WRAP** | 1 1 | wrap A in radians onto [-pi,pi] |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **XOR** | 2 1 | 0 if A == NaN and B == NaN, NaN if B == NaN, else A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **XYZ2HSV** | 3 3 | Convert x,y,x triplets to h,s,v triplets |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **XYZ2LAB** | 3 3 | Convert x,y,x triplets to l,a,b triplets |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **XYZ2RGB** | 3 3 | Convert x,y,x triplets to r,g,b triplets |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **Y0** | 1 1 | Bessel function of A (2nd kind, order 0) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **Y1** | 1 1 | Bessel function of A (2nd kind, order 1) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **YLM** | 2 2 | Re and Im orthonormalized spherical harmonics degree A order B |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **YLMg** | 2 2 | Cos and Sin normalized spherical harmonics degree A order B (geophysical convention) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **YN** | 2 1 | Bessel function of A (2nd kind, order B) |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ZCDF** | 1 1 | Normal cumulative distribution function for z = A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ZPDF** | 1 1 | Normal probability density function for z = A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- | **ZCRIT** | 1 1 | Normal distribution critical value for alpha = A |
- +---------------+-------+--------------------------------------------------------------------------------------------------------+
- Symbols
- -------
- The following symbols have special meaning:
- +-------------+-------------------------------------------------+
- | **PI** | 3.1415926... |
- +-------------+-------------------------------------------------+
- | **E** | 2.7182818... |
- +-------------+-------------------------------------------------+
- | **EULER** | 0.5772156... |
- +-------------+-------------------------------------------------+
- | **PHI** | 1.6180339... (golden ratio) |
- +-------------+-------------------------------------------------+
- | **EPS_F** | 1.192092896e-07 (single precision epsilon |
- +-------------+-------------------------------------------------+
- | **XMIN** | Minimum x value |
- +-------------+-------------------------------------------------+
- | **XMAX** | Maximum x value |
- +-------------+-------------------------------------------------+
- | **XRANGE** | Range of x values |
- +-------------+-------------------------------------------------+
- | **XINC** | x increment |
- +-------------+-------------------------------------------------+
- | **NX** | The number of x nodes |
- +-------------+-------------------------------------------------+
- | **YMIN** | Minimum y value |
- +-------------+-------------------------------------------------+
- | **YMAX** | Maximum y value |
- +-------------+-------------------------------------------------+
- | **YRANGE** | Range of y values |
- +-------------+-------------------------------------------------+
- | **YINC** | y increment |
- +-------------+-------------------------------------------------+
- | **NY** | The number of y nodes |
- +-------------+-------------------------------------------------+
- | **X** | Grid with x-coordinates |
- +-------------+-------------------------------------------------+
- | **Y** | Grid with y-coordinates |
- +-------------+-------------------------------------------------+
- | **XNORM** | Grid with normalized [-1 to +1] x-coordinates |
- +-------------+-------------------------------------------------+
- | **YNORM** | Grid with normalized [-1 to +1] y-coordinates |
- +-------------+-------------------------------------------------+
- | **XCOL** | Grid with column numbers 0, 1, ..., NX-1 |
- +-------------+-------------------------------------------------+
- | **YROW** | Grid with row numbers 0, 1, ..., NY-1 |
- +-------------+-------------------------------------------------+
- | **NODE** | Grid with node numbers 0, 1, ..., (NX*NY)-1 |
- +-------------+-------------------------------------------------+
- | **NODEP** | Grid with node numbers in presence of pad |
- +-------------+-------------------------------------------------+
- Notes On Operators
- ------------------
- #. For Cartesian grids the operators **MEAN**, **MEDIAN**, **MODE**,
- **LMSSCL**, **MAD**, **PQUANT**, **RMS**, **STD**, and **VAR** return the
- expected value from the given matrix. However, for geographic grids
- we perform a spherically weighted calculation where each node value
- is weighted by the geographic area represented by that node.
- #. The operator **SDIST** calculates spherical distances in km between the
- (lon, lat) point on the stack and all node positions in the grid. The
- grid domain and the (lon, lat) point are expected to be in degrees.
- Similarly, the **SAZ** and **SBAZ** operators calculate spherical
- azimuth and back-azimuths in degrees, respectively. The operators
- **LDIST** and **PDIST** compute spherical distances in km if **-fg** is
- set or implied, else they return Cartesian distances. **Note**: If the current
- :term:`PROJ_ELLIPSOID` is ellipsoidal then
- geodesics are used in calculations of distances, which can be slow.
- You can trade speed with accuracy by changing the algorithm used to
- compute the geodesic (see :ref:`PROJ_GEODESIC <Projection Parameters>`).
- The operator **LDISTG** is a version of **LDIST** that operates on the
- GSHHG data. Instead of reading an ASCII file, it directly accesses one of
- the GSHHG data sets as determined by the **-D** and **-A** options.
- #. The operator **POINT** reads a ASCII table, computes the mean x and mean
- y values and places these on the stack. If geographic data then we use
- the mean 3-D vector to determine the mean location.
- #. The operator **PLM** calculates the associated Legendre polynomial
- of degree L and order M (0 <= M <= L), and its argument is the sine of
- the latitude. **PLM** is not normalized and includes the Condon-Shortley
- phase (-1)^M. **PLMg** is normalized in the way that is most commonly
- used in geophysics. The C-S phase can be added by using -M as argument.
- **PLM** will overflow at higher degrees, whereas **PLMg** is stable
- until ultra high degrees (at least 3000).
- #. The operators **YLM** and **YLMg** calculate normalized spherical
- harmonics for degree L and order M (0 <= M <= L) for all positions in
- the grid, which is assumed to be in degrees. **YLM** and **YLMg** return
- two grids, the real (cosine) and imaginary (sine) component of the
- complex spherical harmonic. Use the **POP** operator (and **EXCH**) to
- get rid of one of them, or save both by giving two consecutive = file.nc calls.
- The orthonormalized complex harmonics **YLM** are most commonly used in
- physics and seismology. The square of **YLM** integrates to 1 over a
- sphere. In geophysics, **YLMg** is normalized to produce unit power when
- averaging the cosine and sine terms (separately!) over a sphere (i.e.,
- their squares each integrate to 4 pi). The Condon-Shortley phase (-1)^M
- is not included in **YLM** or **YLMg**, but it can be added by using -M
- as argument.
- #. All the derivatives are based on central finite differences, with
- natural boundary conditions, and are Cartesian derivatives.
- #. Files that have the same names as some operators, e.g., **ADD**,
- **SIGN**, **=**, etc. should be identified by prepending the current
- directory (i.e., ./LOG).
- #. Piping of files is not allowed.
- #. The stack depth limit is hard-wired to 100.
- #. All functions expecting a positive radius (e.g., **LOG**, **KEI**,
- etc.) are passed the absolute value of their argument. (9) The bitwise
- operators (**BITAND**, **BITLEFT**, **BITNOT**, **BITOR**, **BITRIGHT**,
- **BITTEST**, and **BITXOR**) convert a grid's single precision values to
- unsigned 32-bit ints to perform the bitwise operations. Consequently,
- the largest whole integer value that can be stored in a float grid is
- 2^24 or 16,777,216. Any higher result will be masked to fit in the lower
- 24 bits. Thus, bit operations are effectively limited to 24 bit. All
- bitwise operators return NaN if given NaN arguments or bit-settings <= 0.
- #. When OpenMP support is compiled in, a few operators will take advantage
- of the ability to spread the load onto several cores. At present, the
- list of such operators is: **LDIST**, **LDIST2**, **PDIST**, **PDIST2**,
- **SAZ**, **SBAZ**, **SDIST**, **YLM**, and **grd_YLMg**.
- #. Operators **DEG2KM** and **KM2DEG** are only exact when a spherical Earth
- is selected with :term:`PROJ_ELLIPSOID`.
- #. Operator **DOT** normalizes 2-D vectors before the dot-product takes place.
- For 3-D vector they are all unit vectors to begin with.
- #. The color-triplet conversion functions (**RGB2HSV**, etc.) includes not
- only r,g,b and h,s,v triplet conversions, but also l,a,b (CIE L a b ) and
- sRGB (x, y, z) conversions between all four color spaces.
- #. The DAYNIGHT operator returns a grid with ones on the side facing the given
- sun location at (A,B). If the transition width (C) is zero then we get
- either 1 or 0, but if C is nonzero then we approximate the step function
- using an atan-approximation instead. Thus, the values are never exactly
- 0 or 1, but close, and the smaller C the closer we get.
- .. include:: explain_float.rst_
- .. include:: explain_grd_inout_short.rst_
- .. include:: explain_grd_coord.rst_
- .. include:: explain_sto_rcl_clr.rst_
- .. include:: explain_gshhg.rst_
- .. include:: explain_inside.rst_
- Macros
- ------
- Users may save their favorite operator combinations as macros via the
- file *grdmath.macros* in their current or user directory. The file may contain
- any number of macros (one per record); comment lines starting with # are
- skipped. The format for the macros is **name** = **arg1 arg2 ... arg2**
- : *comment* where **name** is how the macro will be used. When this
- operator appears on the command line we simply replace it with the
- listed argument list. No macro may call another macro. As an example,
- the following macro expects three arguments (radius x0 y0) and sets the
- modes that are inside the given circle to 1 and those outside to 0:
- INCIRCLE = CDIST EXCH DIV 1 LE : usage: r x y INCIRCLE to return 1
- inside circle
- **Note**: Because geographic or time constants may be present in a macro, it
- is required that the optional comment flag (:) must be followed by a space.
- Examples
- --------
- .. include:: explain_example.rst_
- To compute all distances to north pole, try::
- gmt grdmath -Rg -I1 0 90 SDIST = dist_to_NP.nc
- To take log10 of the average of 2 files, use::
- gmt grdmath file1.nc file2.nc ADD 0.5 MUL LOG10 = file3.nc
- Given the file ages.nc, which holds seafloor ages in m.y., use the
- relation depth(in m) = 2500 + 350 \* sqrt (age) to estimate normal seafloor depths, try::
- gmt grdmath ages.nc SQRT 350 MUL 2500 ADD = depths.nc
- To find the angle a (in degrees) of the largest principal stress from
- the stress tensor given by the three files s_xx.nc s_yy.nc, and
- s_xy.nc from the relation tan (2\*a) = 2 \* s_xy / (s_xx - s_yy), use::
- gmt grdmath 2 s_xy.nc MUL s_xx.nc s_yy.nc SUB DIV ATAN 2 DIV = direction.nc
- To calculate the fully normalized spherical harmonic of degree 8 and
- order 4 on a 1 by 1 degree world map, using the real amplitude 0.4 and
- the imaginary amplitude 1.1, use::
- gmt grdmath -R0/360/-90/90 -I1 8 4 YLM 1.1 MUL EXCH 0.4 MUL ADD = harm.nc
- To extract the locations of local maxima that exceed 100 mGal in the file faa.nc, use::
- gmt grdmath faa.nc DUP EXTREMA 2 EQ MUL DUP 100 GT MUL 0 NAN = z.nc
- gmt grd2xyz z.nc -s > max.xyz
- To demonstrate the use of named variables, consider this radial wave
- where we store and recall the normalized radial arguments in radians by::
- gmt grdmath -R0/10/0/10 -I0.25 5 5 CDIST 2 MUL PI MUL 5 DIV STO@r COS @r SIN MUL = wave.nc
- To create a dumb file saved as a 32 bits float GeoTiff using GDAL, run::
- gmt grdmath -Rd -I10 X Y MUL = lixo.tiff=gd:GTiff
- To compute distances in km from the line trace.txt for the area represented by the
- geographic grid data.grd, run::
- gmt grdmath -Rdata.grd trace.txt LDIST = dist_from_line.grd
- To demonstrate the stack-reducing effect of **-S**, we compute the standard deviation
- per node of all the grids matching the name model_*.grd using::
- gmt grdmath model_*.grd -S STD = std_of_models.grd
- To create a geotiff with resolution 0.5x0.5 degrees with distances in km from the coast line, use::
- grdmath -RNO,IS -Dc -I.5 LDISTG = distance.tif=gd:GTIFF
- References
- ----------
- Abramowitz, M., and I. A. Stegun, 1964, *Handbook of Mathematical
- Functions*, Applied Mathematics Series, vol. 55, Dover, New York.
- Holmes, S. A., and W. E. Featherstone, 2002, A unified approach to the
- Clenshaw summation and the recursive computation of very high degree and
- order normalized associated Legendre functions. *Journal of Geodesy*,
- 76, 279-299.
- Press, W. H., S. A. Teukolsky, W. T. Vetterling, and B. P. Flannery,
- 1992, *Numerical Recipes*, 2nd edition, Cambridge Univ., New York.
- Spanier, J., and K. B. Oldman, 1987, *An Atlas of Functions*, Hemisphere
- Publishing Corp.
- See Also
- --------
- :doc:`gmt`, :doc:`gmtmath`,
- :doc:`grd2xyz`, :doc:`grdedit`,
- :doc:`grdinfo`, :doc:`xyz2grd`
- .. ------------------------------------- Examples per option -------------------
- .. |ex_SDIST| raw:: html
- <a href="#openModal">Example</a>
- <div id="openModal" class="modalDialog">
- <div>
- <a href="#close" title="Close" class="close">X</a>
- <h2>To compute all distances to north pole:</h2>
- <p>gmt grdmath -Rg -I1 0 90 SDIST = dist_to_NP.nc</br></p>
- </div>
- </div>
|