William Fleetwood Sheppard

Summary

William Fleetwood Sheppard 1911 Encyclopædia Britannica (1911)

If we represent the corresponding value of u by an ordinate drawn from the line, the extremities of all such ordinates will lie on a curve which will be the graph of u with regard to x. Interpolation therefore consists in determining the length of the ordinate of a curve occupying a particular position, when the lengths of ordinates occupying certain specified positions are known. If u is a function of two variables, x and y, we may similarly represent it by the ordinate of a surface, the position of the ordinate being determined by the values of x and of y jointly.
Source: Wikisource

William Fleetwood Sheppard 1911 Encyclopædia Britannica (1911)

Similarly in using differences of a higher order we replace the graph by a curve whose equation is of the form u = A + Bx + Cx2 + Dx3 + . . . The various forms that interpolation-formulae take are due to the various principles on which ordinates are selected for determining the values of A, B, C . . .
B. Inverse Interpolation.
5. To find the value of x when u is given, i.e. to find the value of θ when uθ is given, we use the same formula as for direct interpolation, but proceed (if differences beyond the first are involved) by successive approximation.
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