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are such linear functionals of T ; here, x, y, z denotes a local coordinate sys-
tem in which the z -axis is vertical upwards and the x -and y -axes are directed
towards north and east, and R = 6371 km is a mean radius of the earth.
Equation (10-9) is a consequence of equations such as (2-377), with ∂s = ∂x
or ∂y ;normalgravity γ may be considered constant with respect to horizon-
tal derivation. Equation (10-10) is the well-known fundamental equation of
physical geodesy in spherical approximation (2-263). Equations (10-9) and
(10-10) refer to the earth's surface.
To repeat, by saying that deflections of the vertical and gravity distur-
bances and anomalies are linear functionals of T , we simply indicate the fact
that ξ, η, δg, g depend on T by the expressions (10-9) and (10-10), which
clearly are linear; they are the linear terms of a Taylor expansion, neglect-
ing quadratic and higher terms. In the above notation L i T ,thesymbol L i
denotes, for instance, the operation
1
γ
∂x
L i =
(10-12)
applied to T at some point.
Putting
L i f = L i T = i
(10-13)
and substituting (10-2), we get
q
B ik b k = i
with B ik = L i ϕ k ,
(10-14)
i =1
where L i ϕ k denotes the number obtained by applying the operation L i to the
base function ϕ k ; the coecient B ik obtained in this way does not depend
on the measured values. Equation (10-14) is a linear system of q equations
for q unknowns, which is quite similar to (10-6). This method of fitting an
analytical approximating function to a number of given linear functionals is
called collocation and is frequently used in numerical mathematics.
It is clear that interpolation is a simple special case of collocation in
which
L i f = f ( P i )
(10-15)
is the “evaluation functional”, giving the value of f at a point P i .Thus
we see that in both interpolation and collocation the coecients b k require
the solution of a linear system of equations (which in general will not be
symmetric).
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