§3.3 Interpolation
Contents
- §3.3(i) Lagrange Interpolation
- §3.3(ii) Lagrange Interpolation with Equally-Spaced Nodes
- §3.3(iii) Divided Differences
- §3.3(iv) Newton’s Interpolation Formula
- §3.3(v) Inverse Interpolation
- §3.3(vi) Other Interpolation Methods
§3.3(i) Lagrange Interpolation
The nodes or abscissas
are real or complex; function values
are
. Given
distinct points
and
corresponding
function values
, the Lagrange interpolation polynomial is the
unique polynomial
of degree not exceeding
such that
,
. It is given by
where
Here the prime signifies that the factor for
is to be omitted,
is the Kronecker symbol, and
is the nodal
polynomial
With an error term the Lagrange interpolation formula for
is given
by
If
,
(
), and the nodes
are real, and
is
continuous on the smallest closed interval
containing
, then the error can be expressed
for some
. If
is analytic in a simply-connected domain
(§1.13(i)), then for
,
where
is a simple closed contour in
described in the positive
rotational sense and enclosing the points
.
§3.3(ii) Lagrange Interpolation with Equally-Spaced Nodes
The
-point formula (3.3.4) can be written in the
form

where the nodes
(
) and function
are real,
and
are the Lagrangian interpolation coefficients defined by
Let
be defined by
where the maximum is taken over
-intervals given in the formulas below. Then
for these
-intervals,
¶ Linear Interpolation
¶ Three-Point Formula

¶ Four-Point Formula

¶ Five-Point Formula

¶ Six-Point Formula

¶ Seven-Point Formula

¶ Eight-Point Formula

§3.3(iii) Divided Differences
The divided differences of
relative to a sequence of distinct points
are defined by
and so on. Explicitly, the divided difference of order
is given by
If
and the
(
) are real, and
is
times continuously
differentiable on a closed interval containing the
, then
and again
is as in §3.3(i).
If
is analytic in a simply-connected domain
, then for
,
where
is given by (3.3.3), and
is a
simple closed contour in
described in the positive
rotational sense and enclosing
.
§3.3(iv) Newton’s Interpolation Formula
This represents the Lagrange interpolation polynomial in terms of divided differences:
The interpolation error
is as in §3.3(i). Newton’s
formula has the advantage of allowing easy updating: incorporation of a new
point
requires only addition of the term with
to (3.3.38), plus the computation
of this divided difference. Another advantage is its robustness with respect to
confluence of the set of points
. For example, for
coincident points the limiting form is given by
.
§3.3(v) Inverse Interpolation
In this method we interchange the roles of the points
and the function
values
. It can be used for solving a nonlinear scalar equation
approximately. Another approach is to combine the methods of §3.8
with direct interpolation and §3.4.
¶ Example
To compute the first negative zero
of the Airy
function
(§9.2). The inverse interpolation
polynomial is given by
compare (3.3.38). With
,
,
, we obtain
and with
we find that
, with 4 correct digits. By
using this approximation to
as a new point,
, and evaluating
, we find that
, with
9 correct digits.
For comparison, we use Newton’s interpolation formula (3.3.38)
with the derivative
and compute an approximation to
by using Newton’s rule
(§3.8(ii))
with starting value
. This gives the new point
. Then by using
in Newton’s interpolation
formula, evaluating
and
recomputing
, another
application of Newton’s rule with starting value
gives the
approximation
, with 8 correct digits.
§3.3(vi) Other Interpolation Methods
For Hermite interpolation, trigonometric interpolation, spline interpolation, rational interpolation (by using continued fractions), interpolation based on Chebyshev points, and bivariate interpolation, see Bulirsch and Rutishauser (1968), Davis (1975, pp. 27–31), and Mason and Handscomb (2003, Chapter 6). These references also describe convergence properties of the interpolation formulas.
For interpolation of a bounded function
on
the cardinal
function of
is defined by
where
is called the Sinc function. For theory and applications see Stenger (1993, Chapter 3).


