# ncl_c_csa3s (3) - Linux Manuals

## ncl_c_csa3s: cubic spline approximation, simple entry for three-dimensional input, gridded output

## NAME

c_csa3s - cubic spline approximation, simple entry for three-dimensional input, gridded output## FUNCTION PROTOTYPE

float *c_csa3s(int, float [], float [], float [], float [], int [], int, int, int, float [], float [], float [], int *);

## SYNOPSIS

float *c_csa3s (int n, float xi[], float yi[], float zi[], float ui[], int knots[3], int nxo, int nyo, int nzo, float xo[], float yo[], float zo[], int *ier);

## DESCRIPTION

- n
- (integer,input) The number of input data points. It must be that n is greater than 3 and, depending on the size of knots below, n may have to be larger.
- xi
- (real, input) An array dimensioned for n containing the X coordinate values for the input function.
- yi
- (real, input) An array dimensioned for n containing the Y coordinate values for the input function.
- zi
- (real, input) An array dimensioned for n containing the Z coordinate values for the input function.
- ui
- (real, input) An array containing the functional values of the input function -- ui[k] is the functional value at (xi[k], yi[k], zi[k]) for k=0,n-1.
- knots
- (integer, input) The number of knots to be used in constructing the approximation spline. knots[0], knots[1] and knots[2] must each be at least 4. The larger the value for knots, the closer the approximated curve will come to passing through the input function values.
- nxo
- (integer, input) The number of X coordinate values to be calculated for the output surface.
- nyo
- (integer, input) The number of Y coordinate values to be calculated for the output surface.
- nzo
- The number of Z coordinate values to be calculated for the output grid.
- xo
- (real, input) An array dimensioned for nxo containing the X coordinates of the output grid.
- yo
- (real, output) An array dimensioned for nyo containing the Y coordinates of the output grid.
- zo
- (real, output) An array dimensioned for nzo containing the Z coordinates of the output grid.
- ier
- (pointer to integer, output) An error return value. If *ier is returned as 0, then no errors were detected. If *ier is non-zero, then refer to the error list in the error table for details.

## USAGE

c_csa3s is called to find an approximating cubic spline for three-dimensional input data. If you want to weight the input data values, calculate derivatives, or handle data sparse areas specially, then you will need to use c_csa3xs.c_csa3s returns a pointer to a linear array of data that is the approximation spline stored in row-major order. That is, if out is declared as

float *out;

and we set:

out = c_csa3s(n, x, y, z, u, nx, ny, nz, xo, yo, zo, &ier);

then out[nz*ny*i + nz*j + k] is the approximation function value at coordinate point (xo[i], yo[j], zo[k]) for 0 <= i < nx, 0 <= j < ny, and 0 <= k < nz. The space for out is allocated internal to c_csa3s and is nx*ny*nz floats in size.

## ACCESS

To use c_csa3s, load the NCAR Graphics library ngmath.## COPYRIGHT

Copyright (C) 2000University Corporation for Atmospheric Research

The use of this Software is governed by a License Agreement.

## SEE ALSO

csagrid, c_csa3xs, c_csa3ls, c_csa3lxs
Complete documentation for Csagrid is available at URL

http://ngwww.ucar.edu/ngdoc/ng/ngmath/csagrid/csahome.html