Summary. In order to urlderstand the relative importance of the various phenomena which contribute to marine magnetic anomalies, an analysis was performed on magnetic profiles measured simultaneously at the sea surface and near the sea floor. The data come from three long geophysical surveys made over spreading centres in the eastern Pacific with the Deep Tow instrument package. At low spatial frequencies the two sets of observations agree very closely when related by the mathematical model of upward continuation from magnetic sources below, which are assumed to be perfectly heated, i.e. ‘two-dimensional’. However, spectral analysis reveals the presence of a discrepancy at high spatial frequencies. In all three surveys at wavelengths shorter than about 4km the observed surface field power exceeds the upward continued power by several orders of magnitude. Several causes for this discrepancy are examined, including deviations from twodimensionality , numerical problems, and the noise background of the ocean environment, and the most likely candidate is shown to be ionospheric activity. Spectra of magnetograms from the nearest land observatories intersect the upward continued spectra at about 4-km wavelength, and exhibit power at high spatial frequency which agrees with the extra power in the surface data in each survey. For the observed surface data, the regime of valid geological interpretation is limited by ionospheric noise to wavelengths longer than about 4km. The near-bottom data do not suffer from such a limitation primarily because they were obtained near the geological sources, not just because of the attenuation of the ionospheric noise by the conducting sea water above. The interpretation regime of the near-bottom data is much wider, extending to wavelengths of a few hundred metres where the observed power nears the quantization noise level and where the validity of the assumption of perfectly heated sources probably breaks down. The behaviour of the observed spectra suggests an analytical model which portrays how the bandwidth of the interpretation regime of the surface field depends on the towing speed, source depth and ionospheric activity level. It is shown that a faster towing speed reduces the effect of the ionospheric noise.
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