Earth Science and Engineering, Imperial College London
Doi
Abstract
Consideration of stabilisation techniques is essential in the development of physical models if
they are to faithfully represent processes over a wide range of scales. Careful application of
these techniques can significantly increase
flexibility of models, allowing the computational
meshes used to discretise the underlying partial differential equations to become highly nonuniform
and anisotropic, for example. This
exibility enables a model to capture a wider
range of phenomena and thus reduce the number of parameterisations required, bringing a
physically more realistic solution.
The next generation of
fluid
flow and radiation transport models employ unstructured
meshes and anisotropic adaptive methods to gain a greater degree of
flexibility. However
these can introduce erroneous artefacts into the solution when, for example, a process becomes
unresolvable due to an adaptive mesh change or advection into a coarser region of mesh in
the domain. The suppression of these effects, caused by spatial and temporal variations in
mesh size, is one of the key roles stabilisation can play.
This thesis introduces new explicit and implicit stabilisation methods that have been
developed for application in
fluid and radiation transport modelling. With a focus on
a consistent residual-free approach, two new frameworks for the development of implicit
methods are presented. The first generates a family of higher-order Petrov-Galerkin methods,
and the example developed is compared to standard schemes such as streamline upwind
Petrov-Galerkin and Galerkin least squares in accurate modelling of tracer transport. The
dissipation generated by this method forms the basis for a new explicit fourth-order subfilter
scale eddy viscosity model for large eddy simulation. Dissipation focused more sharply on
unresolved scales is shown to give improved results over standard turbulence models. The
second, the inner element method, is derived from subgrid scale modelling concepts and,
like the variational multiscale method and bubble enrichment techniques, explicitly aims to
capture the important under-resolved fine scale information. It brings key advantages to
the solution of the Navier-Stokes equations including the use of usually unstable velocity-pressure
element pairs, a fully consistent mass matrix without the increase in degrees of
freedom associated with discontinuous Galerkin methods and also avoids pressure filtering.
All of which act to increase the
flexibility and accuracy of a model.
Supporting results are presented from an application of the methods to a wide range
of problems, from simple one-dimensional examples to tracer and momentum transport in
simulations such as the idealised Stommel gyre, the lid-driven cavity, lock-exchange, gravity
current and backward-facing step. Significant accuracy improvements are demonstrated
in challenging radiation transport benchmarks, such as advection across void regions, the scattering Maynard problem and demanding source-absorption cases. Evolution of a free
surface is also investigated in the sloshing tank, transport of an equatorial Rossby soliton,
wave propagation on an aquaplanet and tidal simulation of the Mediterranean Sea and global
ocean.
In combination with adaptive methods, stabilising techniques are key to the development
of next generation models. In particular these ideas are critical in achieving the aim of
extending models, such as the Imperial College Ocean Model, to the global scale