For PhD projects for 2015 view here:  look under geophysics  and computer modelling.

We conduct research on a wide range of topics. Here are a few vignettes:

Hydrocarbon identification and magnetic minerals

Hydrocarbon identification and magnetic mineralsAeromagnetic surveys and magnetic susceptibility measurements in drill cuttings, soils and sediments have been proposed as alternative and/or complementary methods of assessment and exploration of hydrocarbon reservoirs. Some magnetic anomalies have been attributed to the existence of authigenic magnetite and/or Fe-sulphides at shallow dep ths. These magnetic minerals have been hypothesized to be a chemical byproduct of primary Fe-oxides exposed to a reducing environment induced by the underlying reservoir. The formation of seconda ry magnetite as spherical aggregates (framboids) has been linked to the presence of hydrocarbons or oil biodegradation but a mechanism for such formations has not been established.

Nano-scale recording in rocks

Nano-scale recording in rocksFor reliable interpretation of palaeo-magnetic data, the mechanisms that induce and alter magnetic remanence, like thermoremanent magnetisation (TRM) and acquisition chemical remanent magnetisation (CRM) must be fully understood. Magnetic signals from rocks are often dominated by grains that contain non-uniform pseudo-single domain (PSD) magnetisation states. However, there is very little understanding of their CRM and TRM properties. Environmental transmission electron microscopy (ETEM) enables the detailed investigation of localised chemical reactions under gas atmospheres with an interpretable spatial resolution. Off-axis electron holography permits nanometre-scale imaging of magnetic induction within and around materials as a function of applied field and temperature. The complementary use of these TEM techniques can be used to reveal local changes in magnetisation in minerals as they alter during in situ heating in controlled atmospheres.

Dating of cataclysmic events

Dating of cataclysmic eventsKey to understanding of cataclysmic events such as mega-floods and palaeo-tsunamis is the ability to accurately date them. This can prove problematic, as the record of rapid erosion retained by the geological record leaves little identifiable material that can be easily dated. For example, large boulders (erratics) are common features of both glacial retreat and cataclysmic events, but as most of their intrinsic properties are not associated with the event we need to examine physical effects or properties that were re-set or initiated at the time of the event. Two measureable effects are the degree of exposure to cosmogenic rays on an erratic’s freshly exposed surfaces and the new magnetisation (a viscous remanent magnetisation (VRM)) recorded by the magnetic minerals within the rock due to its re-orientation in the geomagnetic. The acquisition of VRM is time dependent. We are currently testing this method using erratics from Iceland.


MeteoritesMicrometeorites are extraterrestrial particles 10 µm to 2 mm in size which represent the most important part of the flux of extraterrestrial material to accrete onto Earth’s surface. Magnetite is present in most micrometeorites and is formed by oxidation of iron bearing mineralogical phases during atmospheric entry. Magnetite grains account for the very strong magnetic signal of micrometeorites. Size distribution of neoformed magnetite crystals can be determined using their magnetic properties and is a good indicator of the melting and/or cooling rate during melting of micrometeorites in the atmosphere. Another part of this project is to observe the evolution of magnetic signal with increasing chemical weathering in micrometeorites extracted from moraine collected in the Transantarctic Mountains.

Geomagnetic field variation

Geomagnetic field variationThe Earth's magnetic is constantly changing. To understand variations on long geological timescales, we need to examine the magnetic signal recorded by rocks during their formation. Extracting directional magnetic recording from rocks is relatively straightforward, but extracting the intensity of the ancient field is much more problematic. Reliable intensity data is required if we are to construct accurate geomagnetic field models and understand the long-term behaviour of the fluid motions deep within the earth where the field originates. We are working on a number of topics, including field evolution (fieldwork in Botswana) and field variation (fieldwork in Iceland).



Magnetostratigraphy uses known changes in the polarity of the Earth’s magnetic field over time for correlation of rocks from one place to another. The geomagnetic polarity time scale can be used to date rocks or particular events preserved in the rock record, if a particular polarity reversal can be identified. We are currently using magnetostratigraphy to produce a chronostratigraphic framework for the Morrison Formation, a suite of rocks deposited by rivers and on flood plains 150 million years ago in the Upper Jurassic Period. The Morrison Formation is famous for its iconic and diverse dinosaurian fauna, including Stegosaurus and Diplodocus. Attempts to understand the evolution and palaeoecology of the dinosaurs are currently hampered by a lack of long-range correlation across the Formation.