The main aim of processing GHMT data is to derive the polarity of the remanent magnetization (Jr) of the sediment surrounding the borehole from the magnetic field intensity measured inside the borehole (B0) (Fig. F3). (Strictly speaking, B is an induction, and the NMRS measures the induction by the field.)
The remanent magnetization of sediments is typically acquired during deposition by preferential alignment of the magnetic grains along the magnetic field direction. The sediment also carries an induced magnetization (Ji) along the direction of the present-day field. Both these magnetizations contribute to the field anomaly in the borehole (Bfr and Bfi), according to the following equations (Pozzi et al., 1988):
and
(similarly for Bfi) where Bfrx and Bfrz are the components of Bfr in the x- (~north) and z- (down) directions.
The total field B0 is much larger than the field anomaly caused by the remanent magnetization (in the example in Fig. F3; 44,000 nT compared to 114 nT), so B0 and the Earth's field, Br, are subparallel (to 0.104° in the Fig. F3 example). Therefore, to a very close approximation, it is the projection of the remanent anomaly Bfr along B0 that contributes to the measured B0. In the rest of this paper below this point, Bfr refers to the projection of the remanent anomaly along B0. Bfr is calculated by (Pozzi et al., 1988):
(similarly for Bfi) where I is the magnetic inclination. The field anomaly in the borehole Bfi caused by the induced magnetization Ji can be calculated from the above Equation 3. Ji itself can be calculated from the magnetic susceptibility , which is measured by the SUMS:
where
In the above equations (see, for example, Parkinson, 1983),