  The correlation functions of two or more Euclidean Wilson loops of various
shapes in Euclidean anti-de Sitter space are computed by considering the
minimal area surfaces connecting the loops. The surfaces are parametrized by
Riemann theta functions associated with genus three hyperelliptic Riemann
surfaces. In the case of two loops, the distance $L$ by which they are
separated can be adjusted by continuously varying a specific branch point of
the auxiliary Riemann surface. When $L$ is much larger than the characteristic
size of the loops, then the loops are approximately regarded as local operators
and their correlator as the correlator of two local operators. Similarly, when
a loop is very small compared to the size of another loop, the small loop is
considered as a local operator corresponding to a light supergravity mode.
