# ncl_csa3ls man page

CSA3LS — cubic spline approximation, simple entry for three-dimensional input, list output

## Synopsis

CALL CSA3LS (NI, XI, UI, KNOTS, NO, XO, YO, ZO, UO,

NWRK, WORK, IER)

## Description

- NI
(integer,input) The number of input data points. It must be that NI .gt. 3 and, depending on the size of KNOTS below, NI may have to be larger.

- XI
(real, input) An array containing the X - Y - Z coordinates of the input data points. XI is dimensioned for 3 x NI. XI(1,L) is the X coordinate, XI(2,L) is the Y coordinate, and XI(3,L) is the Z coordinate for the input domain for L=1,NI.

- UI
(real, input) An array dimensioned for NI containing function values at the input XI values, that is, UI(L) is the value of the input function at XI(L) for L=1,NI.

- KNOTS
(integer, input) An array dimensioned for 3 containing the number of knots to be used in each coordinate direction for constructing the approximation spline. KNOTS(I) must be at least 4 for I=1,3. The larger the value for KNOTS, the closer the approximated curve will come to passing through the input function values.

- NO
(integer, input) The number of coordinate values in the output list. NO can be any positive number.

- XO
(real, input) An array dimensioned for NO containing the X coordinates of the output list.

- YO
(real, input) An array dimensioned for NO containing the Y coordinates of the output list.

- ZO
(real, input) An array dimensioned for NO containing the Z coordinates of the output list.

- UO
(real, output) An array dimensioned for NO containing the calculated function values for the output spline. UO(I) is the calculated functional value at (XO(I),YO(I),ZO(I)) for I=1,NO.

- NWRK
(integer, input) The size of the WORK array. NWRK must be at least NK * (NK+3) where NK = KNOTS(1) * KNOTS(2) * KNOTS(3).

- WORK
(real, input) A work array dimensioned for NWRK.

- IER
(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 man page for csagrid_errors for details.

## Usage

CSA3LS 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 CSA3LXS.

## Access

To use CSA3LS, load the NCAR Graphics library ngmath.

## See Also

csagrid, csa3s, csa3xs, csa3lxs

Complete documentation for Csagrid is available at URL

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

## Copyright

Copyright (C) 2000

University Corporation for Atmospheric Research

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