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The shallow axial crust

In the upper oceanic crust, conduction occurs predominantly within seawater filled cracks. Drury & Hyndman (1979) observed a decrease in resistivity of about two orders of magnitude between dry and seawater saturated basalt samples. The overall resistivity of the medium therefore depends strongly on the resistivity of seawater, which itself varies with temperature. At ambient deep ocean temperatures (approximately 2° C), seawater has a resistivity of 0.3 . This falls to a minimum of about 0.04 at 350 ° C and then rises slightly for higher temperatures (Nesbitt, 1993). Up to temperatures of about 350 ° C the resistivity of seawater,sw , at a temperature T, to a good approximation is given by (e.g. Becker 1985)

There is an ambiguity in the porosity required to explain a given measurement of resistivity, with a high porosity and ambient seafloor water temperature giving the same resistivity as a much lower porosity but higher seawater temperature (Evans etal, 1994). Although conduction in seawater filled cracks is the predominant mechanism, the presence of alteration products precipitated in cracks also affects the conductivity (Drury & Hyndman, 1979; Pezard, 1990). Such alteration products in general have a greater resistivity than seawater, therefore as cracks are in-filled there is an increase in the resistivity of the crust (Becker, 1985; Pezard, 1990).

The shallow resistivity structure of the AVR is fairly well constrained around Quail by the short range data collected during the first source tow. The upper 700 m to 1 km of the structure are constrained primarily by the 11 Hz data, which are only slightly affected by the 2-dimensionality of the ridge. Examination of the simple 1-dimensional model is therefore valid providing the study is limited to the upper part of the crust. The steep resistivity gradient in the upper 500 m of the structure is the best constrained feature of the shallow structure, and is consistent with the steep seismic velocity gradient in the upper few hundred metres of the crust (Navin etal , this issue) equated with seismic layer 2A.

The upper HS bound can be used to estimate the porosity, taking the resistivity of the solid phase to be 10,000 , much larger than that of seawater, so that conduction within the solid is negligible. This parameterisation gives a good estimate of the conducting volume, but may underestimate the total porosity if the medium contains isolated pores. The resistivity is approximately 1  close to the seafloor. Assuming ambient ocean floor temperatures (around 2°C) the porosity inferred from this measurement is approximately 50% in the upper 100 m of the crust. Values of around 40% are inferred from seismic P-wave velocities (Navin etal, this issue). Purdy (1987) obtained slightly lower seafloor porosities of around 30% using seismic data from the Mid-Atlantic Ridge at 23°N. Similar values were obtained by Evans etal (1994) using CSEM data from the crest of the East Pacific Rise at 13°N. Submersible surveys reveal significant fracturing and fissuring of the neovolcanic zone, with fissure widths on the scale of centimetres to metres (Ballard & Van Andel, 1977). Such fissuring could account for the high porosities observed in the upper crust.

The results from the Reykjanes Ridge can be compared directly to the CSEM results of Evans (1994) from 13° N on the East Pacific Rise. At 1 km below the seafloor the resistivity at the Reykjanes Ridge is 15, five times less than the resistivity at equivalent depths on the East Pacific Rise at 13°N. Temperature/porosity trade off curves are shown in Figure. 9 for these two bulk resistivities. If the porosity were 0.5% at both ridges, a temperature difference of approximately 200 could explain the observed difference in resistivity. Such a temperature difference would be consistent with the lack of evidence for a large crustal melt body at 13° N on the East Pacific Rise, which is inferred to be in a state of relative magmatic quiescence (Evans etal, 1994), compared to the Reykjanes Ridge, where the RAMESSES experiment has detected a large crustal magma chamber. It is probable that the difference results from a combination of temperature and porosity effects. The seismic results (Navin etal, this issue) show a region of depressed P-wave velocity in the upper crust on the AVR axis, which is not observed at the East Pacific Rise and could indicate increased fracture porosity at the Reykjanes Ridge. Results from Deep Sea Drilling Project hole 409, drilled in crust estimated to be 2.2-3.2 Ma old on the western flank of the Reykjanes Ridge, indicate that the layer 2 basalts have a high vesicularity, averaging 27%, caused by the low confining pressure during eruption at this shallow ridge (Duffield, 1979). Since a connected porosity of at most 3% in layer 2 is inferred from the CSEM measurements (Figure. 9), such vesicles must be predominantly isolated or in-filled so that their contribution to conduction in the basalt is small.


Next: The mid-crustal low resistivity Up: Implications for the fluid Previous: Implications for the fluid

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Lucy MacGregor
Fri Aug 15 08:48:04 PDT 1997