We performed spectral analysis of the record of relative geomagnetic paleoi
ntensity obtained at ODP Site 983, covering the time interval 0-1.1 Ma. The
results confirm the presence of significant power at frequencies correspon
ding to the earth orbital parameters (eccentricity, obliquity, precession).
The construction of the evolutionary spectrum allowed us to establish the
non-stationarity of the signal at those frequencies. The subsequent use of
wavelet techniques made it possible to demarcate the time intervals over wh
ich orbital frequencies are present in the record. For those intervals, the
paleointensity record shows some coherency with the isothermal remanent ma
gnetization, normalizer of the natural remanent magnetization, and the rati
o anhysteretic remanent magnetization/k. These results suggest that the orb
ital frequencies embedded in the paleointensity record are the expression o
f lithologic variations, and probably not a characteristic of the geodynamo
itself. Extracting (filtering) these wavelet components from the Site 983
paleointensity record indicates, however, that this secondary overprint is
of sufficiently low level that it has a minor effect on the overall charact
er of the record. (C) 2000 Elsevier Science B.V. All rights reserved.