We combine a stabilized reduction-to-the-pole and an upward continuati
on filter to produce meaningful reduced-to-the-pole fields at low magn
etic latitudes. The stabilizing procedure is based on the development,
in Taylor's series, of the theoretical expression for the reduction-t
o-the-pole filter in the wavenumber domain. The filter instability is
caused by the huge filter amplitudes along the magnetization azimuth,
which are expressed by the infinite sum of terms close to unity. The s
tabilizing procedure reduces to simply truncating the infinite series.
The upward continuation filter attenuates the high wavenumber compone
nt of the noise and allows us to design a stabilized filter closer to
the theoretical one, Besides, quantitative interpretations of source d
epth based on the filtered field are more reliable when using upward c
ontinuation as compared with arbitrary low-pass filters. The proposed
filter was applied to synthetic data of a single prism uniformly magne
tized along a supposedly known direction, and it produced a reduced-to
-the-pole field very close to the theoretical field at pole. We also a
pplied the filter to magnetic data from Dixon Seamount assuming induce
d magnetization only. We obtained, within the central part of the anom
aly, roughly circular contours of the reduced-to-the-pole anomaly due
to the nearly circular shape of the Seamount (evidenced by topographic
data).