The acquisition of post-depositional detrital remanent magnetization in a variety of natural sediments

Summary. Post-depositional detrital remanent magnetization (pDRM) is the primary means whereby many sediments acquire their palaeomagnetic signal. We have studied the acquisition of this magnetization in a variety of natural sediments. Our technique involves determining the magnetic direction recorded by a sediment as a function of the water content present in the sediment when the sediment experiences a change in the direction of the applied magnetic field. Most of the sediments used in this study were collected wet from natural environments and were preserved in their original state until they were used in the experiments. Grain sizes were measured by the settling tube method which led to the determination of the clay, silt and sand fractions in each sediment. Isothermal remanent magnetization acquisition studies indicated that the predominant magnetic carriers were magnetite. In the pDRM acquisition studies two distinct modes of behaviour were found. For sediments with a sand content less than 60 per cent, the original direction of magnetization was preserved regardless of the water content. Such behaviour is not consistent with a theoretical model which assumes that at high water contents the magnetic carriers remain mobile within fluid-filled voids and hence are able to realign along a new magnetic field direction. For sediments with a sand content in excess of 60%, remagnetization along a new magnetic field direction occurred as expected, provided the sediments were sufficiently wet. Studies of natural sediments and corresponding samples of dried and reconstituted sediments have demonstrated that the magnetic characterization of a sediment can be reliably determined even for older, desiccated sediments.     

Decay of a post-depositional remanent magnetization in wet sediments due to the effect of drying

Summary. The decay of the post-depositional remanent magnetization (post-DRM) during desiccation in magnetic field free space is measured as a function of the loss of water. The decay is ascribed to the drying effect and the time decay of viscous remanent magnetization (VRM). The VRM forms only 10 per cent of the total of loss of remanent magnetization. The decay due to the drying effects depends both on the loss of water and on either the evaporation rate or the period of storage. The percentage of loss of magnetization is independent of its intensity.
A critical drying stage appears (about 60 per cent in water content on a dry basis) which is characterized as a vanishing point of mobile particles or particle units. The mobile particles or units play an important role both in acquisition and demagnetization through physical rotational motion within wet sediments before the critical drying stage. More than 80 per cent of the total loss of the post-DRM is destroyed before the desiccation proceeds to the critical drying stage. The decay of post-DRh4 is concluded to be mainly due to the physically random rotation of the magnetic particles trapped in shallow energy wells which are overcome by the torques caused by the application of the alternating magnetic field less than 200 Oe.     

Directional errors in remanent magnetization of non-cubic soft sediment specimens measured with spinner magnetometers

Summary. This paper assesses theoretically and experimentally the errors in palaeomagnetic directions introduced by measuring rectangular but non-cubic blocks of soft sediments in slow speed spinner magnetometers. Plastic boxes commonly used for this purpose hold samples 21 × 21 × 15 mm. This study models the response of Schonstedt and Molspin spinners to such specimens and presents the results of experiments in which the remanent magnetization (RM) of obsidian blocks, both as cubes and after subsequent cutting to fit within the boxes, was measured to determine actual instrument behaviour. These experiments indicate that the error introduced by use of specimens of the above dimensions may be as much as 8.5° for the smallest specimen-sensor separation in the Schonstedt spinner. For the Molspin spinner and for the next smallest specimen-sensor separation in the Schonstedt instrument, the error is smaller but nevertheless non-negligible.     

Effect of compaction on the acquisition of a detrital remanent magnetization in fine-grained sediments

Summary. Measurements of the detrital remanent magnetization (DRM) of redeposited deep-sea sediment of the silty clay grade are described. Variations in the magnitude of an observed remanence inclination error are related to conditions of sediment accumulation, contrasted here as grain-by-grain settling from a dilute dispersion or by settling from a concentrated slurry. For these artificial redepositions post-depositional compaction is shown to be a major factor in shallowing the observed inclination from the ambient field inclination. The term compactive DRM is tentatively assigned to describe such behaviour.     

An investigation of the scattered remanent magnetization of the Dunnet Head sandstone

Summary. The directions of remanent magnetism of samples of the Dunnet Head sandstone from Scotland are very scattered on a scale down to a few millimetres, although an overall mean direction is reasonably well defined. The scattered directions show considerable stability against thermal demagnetization and there is evidence that haematite pigment is an important carrier of the remanence. It is concluded that the origin of the inhomogeneous magnetization is a disturbed ambient field during acquisition of chemical remanence by the pigment.     

Compaction-induced subsidence in the margin of a carbonate platform

Abstract The Late Carnian Raibl Formation of the Sella Group (Dolomites, N Italy) forms a sedimentary wedge which thins progressively toward the core of a stratigraphically underlying Middle Carnian carbonate platform (Cassian Dolomite). The platform is composed largely of megabreccia clinoforms displaying progradation above the coeval basinal sequence (San Cassiano Formation). These basinal sediments thin from a maximum in a basinward direction to a pinchout towards the central core of the Sella buildup. The progradational foreslopes thin in an antithetic fashion, from a maximum immediately adjacent to the central core of the Sella to a minimum in a basinward direction. The wedge geometry and onlap of the Raibl Formation atop the Sella platform margin is interpreted as the result of compaction-induced differential subsidence and tilting of the platform top. Basinward increase in subsidence of the platform top resulted from a basinward increase in compaction of basinal San Cassiano sediments. Decompaction calculations and stratigraphic/geometric restoration of Carnian strata support this conclusion.     

Rotational remanent magnetization and the torque exerted on a rotating rock in an alternating magnetic field

Summary. Using an air turbine at rotation frequencies of between 1.5 and 275 revolutions per second (rps), the dependence of rotational remanent magnetization (RRM) on rotation frequency has been investigated for two igneous samples in and alternating field of 51 mT peak at 50 Hz. The same experimental arrangement has also been used to measure the dependence on rotation frequency of the torque exerted by the alternating field on the rock samples. The dependence of torque and RRM on peak field has also been measured at a rotation frequency of 112 rps and a linear relationship between RRM and torque has been demonstrated.
In an attempt to elucidate the way in which RRM arises, analytical and numerical models of the rock have been developed in order to calculate the torque curves and these agree quite closely with those observed experimentally. While the precise factor responsible for RRM has not yet been identified from the numerical model it is suggested that RRM may arise as a result of particle moments suddenly flipping into the field direction, and thus by virtue of their intrinsic angular momentum acquiring a transient component of magnetic moment antiparallel to the rotation vector describing the flip. This component, due to the hysteresis of the assembly of particles, will not then entirely disappear when the alternating field is removed. An estimate of the transient axial field which can be considered to deflect each moment towards the rotation axis during the flip yields a value of the order of 1 mT.