minor rewording, no fixes

[unix-history] / usr / src / usr.bin / spline / spline.1

.\" Copyright (c) 1990 The Regents of the University of California.
.\" All rights reserved.
.\"
.\" %sccs.include.proprietary.roff%
.\"
.\"	@(#)spline.1	6.3 (Berkeley) %G%
.\"
.TH SPLINE 1 "%Q"
.AT 3
.SH NAME
spline \- interpolate smooth curve
.SH SYNOPSIS
.B spline
[ option ] ...
.SH DESCRIPTION
.I Spline
takes pairs of numbers from the standard input as abcissas and ordinates
of a function.
It produces a similar set, which
is approximately equally spaced and
includes the input set, on the standard output.
The cubic spline output
(R. W. Hamming,
.ft I
Numerical Methods for Scientists and Engineers,
.ft R
2nd ed., 349ff)
has two continuous derivatives,
and sufficiently many points to look smooth when plotted, for
example by
.IR  graph (1G).
.PP
The following options are recognized,
each as a separate argument.
.TP 5
.B  \-a
Supply abscissas automatically (they are missing from
the input); spacing is given by the next
argument, or is assumed to be 1 if next argument is not a number.
.TP 5
.B  \-k
The constant
.IR k ""
used in the boundary value computation
.IP
.if n .ig
.ti +1.5i
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.EN
..
.if t .ig
.ce
(2nd deriv. at end) = k*(2nd deriv. next to end)
..
.IP
.br
is set by the next argument.
By default
.IR k ""
= 0.
.TP 5
.B  \-n
Space output points
so that approximately
.I n
intervals occur between the lower and upper
.I x
limits.
(Default
.I n
= 100.)
.TP 5
.B  \-p
Make output periodic, i.e. match
derivatives at ends.
First and last input values should normally agree.
.TP 5
.B  \-x
Next 
1 (or 2) arguments are lower (and upper) 
.I x
limits.
Normally these limits are calculated from the data.
Automatic abcissas start at lower limit
(default 0).
.SH "SEE ALSO"
graph(1), plot(1)
.SH DIAGNOSTICS
When data is not strictly monotone in
.I x,
.I spline
reproduces the input without interpolating extra points.
.SH BUGS
A limit of 1000 input points is enforced silently.