ProfessorAdrian Muxworthy

Professor of Earth and Planetary Magnetism

Department of Earth Science & Engineering - Faculty of Engineering

RESEARCH

Overview
Geomagnetic Field Variation
The 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. With several colleagues, I am working on several new methods of determining accurate ancient geomagnetic field intensity (palaeointensity) determination.

Magnetotactic bacteria
Magnetotactic bacteria contain chains of magnetic crystals (usually magnetite), which are termed magnetosomes. The bacteria use these chains of magnetosomes as magnetic compasses to help navigate towards their optimal environment, which is in the oxic-anoxic transition zone. This affect is termed magnetotaxis. To maximize magnetotaxis the magnetosomes should be large to increase the magnetic signal, but not so large that the magnetization in the individual magnetosomes becomes non-uniform and less efficient. With Wyn Williams at the University of Edinburgh, we have used numerical micromagnetic models to determine optimal grain and spatial geometries for chains of magnetotactic bacteria.

Unravelling complex magnetic signals
The magnetic signature of most natural magnetic materials is highly complex. To interpret such signals in geological or environmental terms requires a good understanding of fundamental magnetic processes, such as magnetic hysteresis, and a knowledge of chemical effects such as diagenesis, which can strongly alter mineralogy. With a number of colleagues, I examine a range of fundamental mineral magnetic properties and develop new methods of extracting meaningful information from rocks. We employ several of approaches from examining well-characterized rocks, to synthesizing magnetic mineralss to constructing numerical models.

Evolution of Volcanic Processes
Violent pyroclastic volcanic eruptions such as the famous "Pompeii" eruption of Mt. Vesuvius in 79 AD, can be highly destructive . To assess the risk for the today's local inhabitants it is important to have a knowledge of the historical behaviour of such geohazards. Pyroclastic density currents generated during eruptions can move at high speeds in excess of 100 km per hour, but more importantly can vary in temperature from ambient up to 1000 C. Obviously the temperature strongly affects the danger to local inhabitants and livestock. The only method of estimating the emplacement temperature of past pyroclastic deposits, is through examination of the magnetic signature acquired by lithic clasts during the eruption. With colleagues, I employ palaeomagnetic techniques to study the evolution of volcanic processes

GRANTS

  • GRANT
    Planetary Origins and Evolution at Imperial
    Science and Technology Facilities Council (STFC)1 Apr 2016 - 31 Mar 2019
    Science and Technology Facilities Council (STFC): Planetary Origins and Evolution at Imperial (2016-2019)
  • GRANT
    Origin of the Magnetic Signature of Hydrocarbons
    Natural Environment Research Council (NERC)12 Jun 2012 - 11 Jun 2014
    Natural Environment Research Council (NERC): Origin of the Magnetic Signature of Hydrocarbons (2012-2014)