1c_csa3ls(3NCARG) NCAR GRAPHICS c_csa3ls(3NCARG)
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6 c_csa3ls - cubic spline approximation, simple entry for three-dimen‐
7 sional input, list output
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10 float *c_csa3ls(int, float [], float [], float [], float [],
11 int [], int, float [], float [], float[], int *);
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15 float *c_csa3ls(int n, float xi[], float yi[], float zi[], float ui[],
16 int knots[3], int no, float xo[], float yo[], float zo[],
17 int *);
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21 n (integer,input) The number of input data points. It must be
22 that n is greater than 3 and, depending on the size of
23 knots below, n may have to be larger.
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25 xi (real, input) An array dimensioned for n containing the X
26 coordinate values for the input function.
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28 yi (real, input) An array dimensioned for n containing the Y
29 coordinate values for the input function.
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31 zi (real, input) An array dimensioned for n containing the Z
32 coordinate values for the input function.
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34 ui (real, input) An array containing the functional values of
35 the input function -- ui[k] is the functional value at
36 (xi[k], yi[k], zi[k]) for k=0,n-1.
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38 knots (integer, input) The number of knots to be used in con‐
39 structing the approximation spline. knots[0], knots[1],
40 and knots[2] must be at least 4. The larger the value for
41 knots, the closer the approximated curve will come to pass‐
42 ing through the input function values.
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44 no (integer, input) The number of X - Y coordinate values to
45 be calculated for the output array.
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47 xo (real, input) An array dimensioned for no containing the X
48 coordinates of the output list.
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50 yo (real, output) An array dimensioned for no containing the Y
51 coordinates of the output list.
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53 zo (real, output) An array dimensioned for no containing the Z
54 coordinates of the output list.
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56 ier (pointer to integer, output) An error return value. If *ier
57 is returned as 0, then no errors were detected. If *ier is
58 non-zero, then refer to the error list in the error table
59 for details.
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62 c_csa3ls is called to find values of an approximating cubic spline at
63 specified three-dimensional coordinates. If you want to weight the
64 input data values, calculate derivatives, or handle data sparse areas
65 specially, then you will need to use c_csa3lxs.
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67 c_csa3ls returns a pointer to a linear array of data that contains the
68 approximated values calculated at the input list of coordinate values.
69 That is, if out is declared as
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71 float *out;
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73 and we set:
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75 out = c_csa3ls(n, x, y, z, u, knots, no, xo, yo, zo, &ier);
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77 then out[i] is the approximated function value at coordinate point
78 (xo[i], yo[i], zo[i]) for 0 <= i < no. The space for out is allocated
79 internal to c_csa3ls and is no floats in size.
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82 To use c_csa3ls, load the NCAR Graphics library ngmath.
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85 csagrid, c_csa3s, c_csa3xs, c_csa3lxs
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87 Complete documentation for Csagrid is available at URL
88 http://ngwww.ucar.edu/ngdoc/ng/ngmath/csagrid/csahome.html
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91 Copyright (C) 2000
92 University Corporation for Atmospheric Research
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94 This documentation is free software; you can redistribute it and/or
95 modify it under the terms of the GNU General Public License as pub‐
96 lished by the Free Software Foundation; either version 2 of the
97 License, or (at your option) any later version.
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99 This software is distributed in the hope that it will be useful, but
100 WITHOUT ANY WARRANTY; without even the implied warranty of MER‐
101 CHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General
102 Public License for more details.
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104 You should have received a copy of the GNU General Public License along
105 with this software; if not, write to the Free Software Foundation,
106 Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307 USA.
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111UNIX January 1999 c_csa3ls(3NCARG)