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The CSEM method

The decay of electromagnetic fields in a medium is governed by both the resistivity of the medium and the frequency of the signal. The electromagnetic skin depth defines the distance over which the amplitude of an electromagnetic field decays by a factor 1/e and the phase of the signal is shifted by radians:

where is the skin depth in metres, is the resistivity of the homogeneous medium through which the electromagnetic field is diffusing, is the angular frequency of the signal and µ is magnetic permeability, usually assumed to take its free space value everywhere. Although this expression is derived assuming simple plane wave fields, it provides a useful guide to the attenuation of more complicated dipole fields in the crust. The diffusive nature of the fields means that sharp boundaries and anomalies with a scale length less than a skin depth are not well resolved.

Our experiment involves the transmission of an electromagnetic signal at discrete frequencies (in contrast to the time domain system of Edwards & Chave, 1986) from a horizontal electric dipole (HED) source to an array of remote sea bottom receivers which detect the horizontal electric field. The frequency at which signals are transmitted must be carefully chosen, taking into account the possible resistivity and scale of structures which might be encountered. If the frequency is too low, the skin depth in the seafloor is very long so the signal is not inductively attenuated between the source and the receiver and cannot resolve crustal scale structure. If the transmission frequency is too high, the skin depth is very small and signals only penetrate the shallow part of the crust. All but the very shortest range signals are attenuated to such an extent that they can no longer be detected above the noise (e.g. Flossadottir & Constable, 1996). Another consideration is the noise spectrum. At frequencies below approximately 0.3 Hz, microseism noise is significant (Webb & Cox, 1986), and at lower frequencies still, ionospheric noise starts to leak through the conductive ocean. The range of frequencies which can be usefully employed for probing crustal structure to depths of a few kilometres or more is therefore between a few tenths and a few tens of Hertz.



Next: The experiment Up: The RAMESSES Experiment III: Previous: Introduction

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