Mohsen Bazargan

and 4 more

Pressure and temperature change simultaneously in the Earth’s crust from surface to depth. Joint pressure and temperature changes influence many different physical properties. There are many studies on samples at elevated pressure, where the influence of open cracks, fractures, voids and pores have been studied. Applying confining pressure has a direct influence on crack closure, and this influence on dynamic properties (density and elastic modulus, bulk, shear and young’s) of rocks above 200 MPa is assumed linear with the linear increase in wave speed. This is because it is generally assumed that most cracks are closed above 200 MPa, which in nature would correspond to a depth of ~7-8 km. However, from the KTB deep drilling well in Germany, it is known that fluid-filled fractures and pores can remain open until 8 to 9 km depth. Applying temperature can affect the dynamic properties of rock by thermal expansion, possibly reopening cracks that were closed at pressures >200 MPa, and thermally expanding grains. This influence is also assumed to be linear at a temperature below partial melting, and in the absence of phase transitions. A similar effect has been observed by a number of research groups during laboratory experiments and calculating seismic velocity results under 600 MPa confining pressure and 600oC temperature. In this work, an effort has been made to mathematically investigate the influence of temperature and pressure on the seismic properties (velocity of pressure and shear waves, density and Poisson’s ratio) of crystalline rocks, measured during laboratory experiments. Elastic wave speeds, moduli and density are increasing as a function of pressure and decreasing as a function of temperature. However, these pressure and temperature-related changes are shown to be nonlinear from room conditions up to 600oC and 600 MPa. In this presentation, we focus on non-linear changes mainly in the high-pressure portion of the velocity as a function of pressure (>200 MPa). When confining pressure is applied, measured P- and S- waves show an increase in velocity and decrease in anisotropy. However, the effect of temperature on measured P- and S- waves show a decrease in velocity and increases in anisotropy. These changes are not very different from linear, but it is not possible to fit velocity as a function of pressure or temperature with linear mathematical functions. The implications of non-linear relationships between pressure, temperature and elastic wave speeds are discussed in this presentation.

Thorben Schöfisch

and 2 more

In this study, we report results from three analogue models with similar initial setup and different amounts of bulk shortening, to simulate a development of a pop-up structure in fold-and-thrust belts at different stages. Samples are taken in different places of the deformed models for analysis using anisotropy of magnetic susceptibility. Shortening of the models resulted in the formation of a pop-up structure, which is bounded by backthrust(s) and complex forekink zone(s). Several forethrusts at different degrees of maturity developed in front of the pop-up structure. Three distinct types of magnetic fabric can be identified throughout the models: (i) a compactional oblate fabric that changes as function of distance towards a localized deformation zone (e.g., thrust or kinkzone), (ii) a thrust-induced fabric with magnetic foliation parallel to the thrust surface, and (iii) a complex forekink zone fabric with broad girdle distributions of principal axes and magnetic lineation perpendicular to shortening direction. The latter indicate interplay between folding and thrusting of the shortened sand layers. Additionally, a decrease in degree of anisotropy with appearance of a quantitatively more prolate fabric can be observed towards the thrusts and kinkzones. Additionally at thrusts, a variation in strain is reflected by the magnetic fabric and can be inherited in a thrust-induced fabric. In conclusion, strain is changing as function of distance towards localized deformation zones with characteristic fabric, and differences in magnetic fabric are distinct between data away and within deformation zones as deformation zones mature.