
Once below the Curie Point, the material retains the
same field when it is moved or the magnetic field
changes around it. A rock may contain a number of
different magnetic minerals that each have their own
Curie Point temperature, and alteration of the rock may
occur to create new minerals that will record the ambi-
ent magnetic field at the time of their formation. The
preserved magnetisation or remnant magnetism in a
rock may therefore be a complex mixture of different
field orientations resident in different minerals.
The remnant magnetism in a rock sample is mea-
sured to determine the orientation of the Earth’s mag-
netic field relative to the sample at the time of the
formation of the rock (Hailwood 1989). In extrusive
igneous rocks this will be recorded by the remnant
magnetism in minerals such as magnetite and hae-
matite as they cool below their Curie Point. This
strong signal is relatively easily detected by a magnet-
ometer, but of more use to the stratigrapher is a much
weaker remnant magnetism preserved in sedimentary
rocks. As fine magnetised particles (grains containing
iron minerals such as haematite) settle out of water
they tend to orient themselves parallel to the Earth’s
magnetic field. Clearly not all of these particles will
line up perfectly parallel to the ambient field, but there
will be a statistically significant pattern in their orien-
tation that will give the sediment a remnant polarity.
The effect is strongest in fine-grained sediments depos-
ited from suspension with a high proportion of iron
minerals. In coarser grained sediment the particles
will be oriented by the flow that deposited them and
the remnant magnetism in sediments that have a low
iron content may not be detectable. The remnant
magnetism in a rock will be reset when the minerals
are heated above their Curie Point during meta-
morphism or when the minerals are altered by dia-
genesis or weathering.
21.4.2 Practical magnetostratigraphy
The objective of a magnetostratigraphic study will
usually be to identify periods of normal and reversed
magnetic polarity recorded in a succession of strata.
Field sampling is normally carried out by drilling out
small cores of rock from beds in the outcrop. The
orientation of the cores in three dimensions and the
attitude of the bedding are measured and multiple
cores are normally taken from a single bed in order
to provide enough samples for a statistically signifi-
cant analysis of the remnant magnetism at that single
site. The vertical interval between sampling sites in
the succession will depend on the rates of accumula-
tion of the sediments and the time interval between
field reversals during that period of Earth history. In
successions deposited at slow rates, samples may need
to be taken every few metres up the succession in
order to be sure of detecting all the polarity reversals,
whereas higher rates of accumulation allow a wider
spacing of sample sites. Once a reversal is identified,
the precise location in the succession may be deter-
mined by resampling at closer intervals between the
sites that show opposite field directions.
The remnant magnetism in the samples is deter-
mined in the laboratory by a magnetometer. Modern
instruments are capable of detecting and measuring
magnetic fields in the samples that are several orders
of magnitude weaker than the Earth’s magnetic field.
The effects of the present-day magnetic field are
removed by putting the sample in a space shielded
from the present-day field and either heating it up or
subjecting it to the field of an alternating current. The
orientation of the remaining remnant magnetism will
be relict from an earlier stage in its history, hopefully
the time at which the rock was formed. The remnant
magnetism recorded in separate samples at the same
site is compared to ensure statistical significance of
the result.
21.4.3 Magnetostratigraphic correlation
By making measurements of the remnant palaeomag-
netism through a succession of beds it is possible to
construct a record of the periods of normal and
reversed stratigraphy. These are conventionally
shown as intervals marked in black for normal polar-
ity and white for reversed polarity (Fig. 21.4). The
pattern of reversals in the Earth’s magnetic field
through time has been established for much of the
Phanerozoic and many reversal events are well dated.
In order to tie the pattern measured in an individual
succession to the established polarity stratigraphy it is
essential to have some sort of tie-point to the geologi-
cal time scale. This may be provided by absolute dat-
ing of a unit, such as a lava, within the successions, or
biostratigraphic information that can be used to relate
a point in the succession to the time scale (Fig. 21.5).
An important proviso is that any time gaps in the
record provided by the succession are recognised
Magnetostratigraphy 331