10.5 Evaluation of the significance of lateral variation 157
An example of such a simulation will be treated in Chapter 13. In brief, geologi-
cal and structural controls, together with requirements for conservation of material,
enable one to make a reasonable approximation of the past and present mode of
deformation of many deformed and denuded regions. Numerical models based on
such kinematic frameworks can be used to solve for the evolving thermal structure
of the deforming region (Koons, 1987; Beaumont et al., 1996; Batt and Braun,
1997). The physical and thermal coupling of these models enables the tracking
of selected material points through the model domain, and the assessment of how
a given exhumation path interacts with the evolving thermal structure, enabling
thermal histories, and their implications for different thermochronometers, to be
calculated for individual particles.
The multi-variate models needed to incorporate the dynamic interplay of heat
flow, kinematics and sample mineralogy that goes into producing a thermochrono-
logical age cannot usually provide a unique interpretation for specific age data
(e.g., Quidelleur et al., 1997). Rather, such models are used to provide insights into
how various aspects of tectonic deformation and accompanying denudation are
ultimately integrated into the thermochronological record, thus helping to choose
between competing hypotheses, and guiding interpretation of the physical causes
behind observed regional patterns in thermochronological data (Shi et al., 1996;
Beaumont et al., 1996; Batt and Braun, 1999; Batt et al., 2001; Ehlers et al., 2001).
Case study: the Olympic Mountains
The Olympic Mountains (Figure 10.3) are the topographically highest and most
deeply exhumed segment of the Cascadia forearc high of western North America.
The Olympics were the earliest part of the forearc to become emergent, c. 12 Myr
ago (Brandon and Calderwood, 1990), and the mountainous topography of the
range has been sustained since that time by continued accretion of material
from the subducting Juan de Fuca Plate and within-wedge deformation (Brandon
and Calderwood, 1990; Brandon et al., 1998). The Cascadia accretionary wedge
(Figure 10.3) is composed predominantly of sedimentary material built up by this
progressive accretion (Clowes et al., 1987; Brandon and Calderwood, 1990). This
sedimentary wedge underlies most of the offshore continental margin, reaching
thicknesses of 30 km, but is sub-aerially exposed only in the Olympic Mountains
(Stewart, 1970; Rau, 1973; Tabor and Cady, 1978).
In common with many accretionary complexes, there is a general paucity of
age-diagnostic fossils within the sandstones of the Cascadia accretionary wedge.
In the absence of reliable paleontological age control, thermochronological data
have long been the prime means applied to constraining the tectonic evolution