Long term geomagnetic
evolution and links with Earth history
Palaeomagnetic records may be unique
in the Earth sciences in giving us direct
observational evidence regarding deep internal
processes occurring back into deep geological
time. The Earth's magnetic field exhibits clear
variations on timescales of millions and even
billions of years that are probably caused by
changing conditions in the planet's core and
mantle. I am interested to try and explain these
variations in terms of mantle dynamics and core
evolution. I hope to develop palaeomagnetism
into a reliable tool for telling us, not only
about fluid flow in the outer core, but also
about mantle convection from the bottom-up
through documenting and interpreting its influence on the geodynamo.
Selected publications:
Biggin, A.J., Piispa, E, Pesonen, L.J., Holme,
R., Paterson, G.A., Veikkolainen, T.,, Tauxe, L.
2015. Palaeomagnetic field strength variations
suggest Mesoproterozoic inner core nucleation.
Nature. 526, 245-248.
Biggin, A.J. , Steinberger, B., bert, J.,
Suttie, N., Holme, R., Torsvik, T., van der
Meer, D., vanHinsbergen, 2012. Possible links
between long term geomagnetic variations and
whole-mantle convection processes. Nature
Geosci. 8, 526-533.
Biggin, A.J., Strik, H.M.A., & Langereis, C.G.,
2008. Evidence for a very-long-term trend
ingeomagnetic secular variation. Nature Geosci.
1, 395-398. |
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A plot of the strength
of the main component of the geomagnetic field
versus time for the last few thousands of years.
Taken from Ertepinar et al. (2012). |
Variations in the Earth's magnetic
field through the Holocene
The geomagnetic field's strength and
morphology has varied considerably even on the
timescales of human history. The field is
presently weakening at a rate of a few percent
per century leaving our technology increasingly
vulnerable to harsh space weather events. Studies of
recent variations can tell us
about the dynamics of the geodynamo processes
operating the Earth's core and additionally warn us
about how the field may change in the near
future. I am
particularly interested in studying very strong
fluctuations in the
strength of the field that are increasingly
evident in archaeomagnetic records from the last
few thousands of years.
Selected publications:
Ertepinar, P., Langereis, C.G., Biggin, A.J., de
Groot, L.V., Kulakoglu, F., Omura, S., Süel, S.
2016. Full vector archaeomagnetic records from
Anatolia between 2400 and 1350 BCE: Implications
for geomagnetic field models and the dating of
fires in antiquity. Earth Planet. Sci. Lett.
434, 171-186.
Ertepinar P, Langereis CG, Biggin AJ, Frangipane M, Matney T, Okse T, Engin A
(2012) Archaeomagnetic study of five mounds from Upper Mesopotamia between 2500
and 700 BCE: Further evidence for an extremely strong geomagnetic field ca.3000
years ago'. Earth Planet. Sci. Lett. 357-358, 84-98.
de Groot L, Biggin A, Dekkers M, Langereis C, Herrero-Bervera E (2013). Rapid
regional perturbations to the recent global geomagnetic decay revealed by a new
Hawaiian record. Nature Communications 4: 2727. |
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The Earth's
earliest magnetic field
Some of the oldest rocks on Earth retain a
palaeomagnetic signal that can be demonstrated
to be as old as they are. The Earth was a very
different place 3.5 billion years ago, when the
rocks we are working with from the Barberton
Greenstone Belt in southern Africa acquired
their magnetisations. We know very little but
the mantle was much hotter and the core was
probably still entirely liquid. Palaeomagnetic
studies of these rock provide a unique
opportunity to constrain conditions deep in
Earth's interior in the Archaean Aeon and
thereby to document our planet's evolution.
Selected publications:
Biggin, A.J., de Wit, M.K., Langereis, C.G.,
Zegers, T.E., Voûte, S., Dekkers, M.J., Drost,
K., 2011. Palaeomagnetism of Archaean rocks of
the Onverwacht Group, Barberton Greenstone Belt
(southern Africa): Evidence for a stable and
potentially reversing geomagnetic field at ca.
3.5 Ga. Earth Planet. Sci. Lett. 302, 314-328.
Biggin, A.J., Strik, G.H.M.A. & Langereis, C.G.,
2009. The intensity of the geomagnetic field in
the late-Archaean: new measurements and an
analysis of the updated IAGA palaeointensity
database. Earth, Planets & Space 61, 9-22.
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The Barberton
Greenstone Belt - home to some of the oldest
palaeomagnetic recorders on the planet. |
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Outputs of a numerical
model of thermoremanent magnetisation applied to
predict the outcome of different palaeointensity
experiments performed on non-ideal samples
(Biggin et al., 2010). |
Acquisition of thermoremanent magnetisation
in natural materials and implications for palaeointensity records
Measurements of the ancient geomagnetic strength are crucial for documenting
and understanding geomagnetic field behaviour on
all timescales. It is possible to make these
"palaeointensity" measurements only from things
that have cooled down from high temperature in
the presence of the geomagnetic field and
acquired a "thermoremanent magnetisation". The
process by which rocks acquire this
magnetisation is not fully understood however
and this, plus the fact that
many rocks do not contain ideal magnetic
recorders, makes measuring the palaeointensity
accurately difficult. I am interested to
understand the thermoremanent magnetisation
acquisition process and the different problems
that can bias palaeointensity estimates so they
can be mitigated against.
Selected publications:
Paterson, G.A., Biggin, A.J., Hodgson, E.,
Hill, M.J., 2015. Thellier-type paleointensity
data from multidomain specimens. Phys. Earth
Planet. Int. 245, 117-133.
Biggin AJ, Badejo S, Hodgson E, Muxworthy A, Shaw J, Dekkers M, 2013. The effect
of cooling rate on the intensity of thermoremanent magnetisation (TRM) acquired
by assemblages of pseudo-single domain, multi domain, and interacting single
domain grains. Geophysical Journal International 193, 1239-1249
Biggin, A.J., 2010. Are systematic differences
between thermal and microwave Thellier-type
palaeointensity estimates a consequence of multidomain bias in the thermal results? Physics
of the Earth and Planetary Interiors, 180:
16-40.
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Geomagnetic Palaeosecular Variation
Secular variation refers to the changes in the
Earth's magnetic field that require you to
change your compass's north arrow every year or
two. It is also thought to be responsible for
causing the magnetic field to reverse its
polarity every few hundreds of thousands of
years. Palaeosecular variation is the study of
this variability as recorded in ancient lavas
and sedimentary rocks and it has the potential
to provide fundamental insights into the
stability state of the geodynamo in the past as well as provide a tool for
constraining volcanic eruption rates.
Selected publications:
Suttie, N., Biggin, A.J., Holme, R., 2015.
Robust estimators of palaeosecular variation.
Geophys. J. Int. 200, 1046-1051.
Suttie, N., Biggin, A.J., Holme, R., 2014. Correlation of palaeomagnetic
directions constrains eruption rate of large igneous provinces. Earth Planet.
Sci. Lett. 387, 4-9.
Biggin, A.J., Van Hinsbergen, D.J.J., Langereis,
C.G., Straathof, G.B. and Deenen, M.H.L., 2008.
Geomagnetic secular variation in the Cretaceous
Normal Superchron and in the Jurassic. Phys.
Earth Planet. Inter. 169, 3-19.
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Palaeosecular variation
represented in terms of scatter of virtual
geomagnetic poles in the Cretaceous Normal
Superchron (Biggin et al., 2008; PEPI). |