1CSA3LS(3NCARG) NCAR GRAPHICS CSA3LS(3NCARG)
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6 CSA3LS - cubic spline approximation, simple entry for three-dimensional
7 input, list output
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10 CALL CSA3LS (NI, XI, UI, KNOTS, NO, XO, YO, ZO, UO,
11 NWRK, WORK, IER)
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14 NI (integer,input) The number of input data points. It must be
15 that NI .gt. 3 and, depending on the size of KNOTS below,
16 NI may have to be larger.
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18 XI (real, input) An array containing the X - Y - Z coordinates
19 of the input data points. XI is dimensioned for 3 x NI.
20 XI(1,L) is the X coordinate, XI(2,L) is the Y coordinate,
21 and XI(3,L) is the Z coordinate for the input domain for
22 L=1,NI.
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24 UI (real, input) An array dimensioned for NI containing func‐
25 tion values at the input XI values, that is, UI(L) is the
26 value of the input function at XI(L) for L=1,NI.
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28 KNOTS (integer, input) An array dimensioned for 3 containing the
29 number of knots to be used in each coordinate direction for
30 constructing the approximation spline. KNOTS(I) must be at
31 least 4 for I=1,3. The larger the value for KNOTS, the
32 closer the approximated curve will come to passing through
33 the input function values.
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35 NO (integer, input) The number of coordinate values in the
36 output list. NO can be any positive number.
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38 XO (real, input) An array dimensioned for NO containing the X
39 coordinates of the output list.
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41 YO (real, input) An array dimensioned for NO containing the Y
42 coordinates of the output list.
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44 ZO (real, input) An array dimensioned for NO containing the Z
45 coordinates of the output list.
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47 UO (real, output) An array dimensioned for NO containing the
48 calculated function values for the output spline. UO(I) is
49 the calculated functional value at (XO(I),YO(I),ZO(I)) for
50 I=1,NO.
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52 NWRK (integer, input) The size of the WORK array. NWRK must be
53 at least NK * (NK+3) where NK = KNOTS(1) * KNOTS(2) *
54 KNOTS(3).
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56 WORK (real, input) A work array dimensioned for NWRK.
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58 IER (integer, output) An error return value. If IER is
59 returned as 0, then no errors were detected. If IER is non-
60 zero, then refer to the man page for csagrid_errors for
61 details.
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64 CSA3LS is called to find an approximating cubic spline for three-dimen‐
65 sional input data. If you want to weight the input data values, calcu‐
66 late derivatives, or handle data sparse areas specially, then you will
67 need to use CSA3LXS.
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70 To use CSA3LS, load the NCAR Graphics library ngmath.
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73 csagrid, csa3s, csa3xs, csa3lxs
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75 Complete documentation for Csagrid is available at URL
76 http://ngwww.ucar.edu/ngdoc/ng/ngmath/csagrid/csahome.html
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79 Copyright (C) 2000
80 University Corporation for Atmospheric Research
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82 The use of this Software is governed by a License Agreement.
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86UNIX January 1999 CSA3LS(3NCARG)