Controlled-source, frequency-domain, and time-domain electromagnetic m
ethods require accurate, fast, and reliable methods of computing the e
lectric and magnetic fields from the source configurations used. Excep
t for small magnetic dipole sources, all electric and magnetic sources
are composed of lengths of straight wire, which may be grounded. If t
he source-receiver separation is large enough, the composite electrica
l dipoles may be considered to be infinitely small, and in a 1-D earth
model the fields are expressed as Hankel transforms of an input funct
ion, which depends only on the model parameters. The Hankel transforms
can be evaluated using the digital filter theory of fast Hankel trans
forms. However, the approximation of the infinitely small dipole is no
t always valid, and fields from a finite electrical dipole must be cal
culated. Traditionally, this is done by numerical integration of the f
ields from an infinitesimal dipole, thus increasing computation time c
onsiderably. The fields from the finite electrical dipole are expresse
d as Hankel transforms and as integrals of Hankel transforms. The theo
ry of fast Hankel transforms is extended to include integrals of Hanke
l transforms, and a method is devised for calculating the filter coeff
icients. Unlike the fast Hankel transform, the computation involved in
the integrated Hankel transforms is not a true convolution, and so a
set of filter coefficients must be calculated for each source-receiver
configuration. Furthermore, the method is extended to include the cal
culation of potential differences where one more integration is involv
ed, which is what is actually measured in the field. The computation o
f filter coefficients is very fast, and for standard configurations, t
he coefficients need be computed only once. The method is as fast, acc
urate, and reliable as the fast Hankel transforms method, and is up to
an order of magnitude faster than the usual numerical integration.