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Assistant Professor of Mathematics
PhD, McMaster
Computational Fluid Dynamics
Office: HH-3035
Phone: (709) 737-8071
Fax: (709) 737-3010
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Objectives
Improving our knowledge of turbulence implies a better
understanding of fluid flows that are important in
environmental, aeronautical, or industrial
applications. For example, accurate modelling of the
turbulent
atmosphere is critical for such varied purposes as weather
forecasting, projecting climate change, and
mitigating air pollution.
The development and the verification of high performance
adaptive multiresolution models are key objectives of my
current research. Following are some specific on-going
research topics.
Multi-scale, space-time adaptive
algorithms for turbulent flows
Turbulence is difficult to approximate mathematically,
and to calculate numerically, because it is active
over a large and continuous range of length scales
(e.g. from less than a millimeter to hundreds of
kilometers in the atmosphere). The range of active scales
increases with an increase of the Reynolds number, which means flows are
increasingly
difficult to calculate at large Reynolds numbers of
practical interest. However, it has been conjectured
that a turbulent flow is spotty - only a fraction of the
flow is active and this active proportion of the flow
decreases as the Reynolds number increases. This means
that high Reynolds number flows are highly intermittent in
both space and time. A numerical model that exploits such
space-time intermittency would use only a fraction of
computational time compared to classical high performance
numerical models.
A better understanding for the space-time intermittency of turbulence is related to many environmental or industrial applications, but classical theories or models of turbulence fail to explain properly such intermittency. In particular, a scaling of the
intermittent space-time degrees of freedom
with respect to increasing turbulence intensity would help us in designing high performance computer models. In my PhD thesis, a scaling of the number of space-time
intermittent modes with the Reynolds number for
2D homogeneous isotropic decaying turbulence was estimated
numerically. This study further reported
that temporal intermittency is much stronger than the
spatial intermittency for 2D decaying turbulence.
Currently, I am involved in extending these results to 3D
models of turbulence. I am also investigating for
a scaling of intermittent space-time modes in the case of
forced homogeneous isotropic turbulence.
Coherent structures in the atmosphere
Our current knowledge of coherent motion in the
atmosphere relies on adhoc approximation of the average
motion, which is an
accumulated empirical or statistical information. An
improved understanding of the coherent atmosphere is
essential for projecting climate change or improving
global climate models. State-of-the-art computer models
for the atmosphere
attempt to resolve a flow up to a certain scale,
expressing unresolved scales in terms of resolved
motion. In such subgrid scale approaches, the
intermittency of coherent structures are ignored. However,
it is evident from both numerical simulation and
observation that only a
fraction of the turbulent atmospheric scales are needed to be
resolved to exploit intermittency. Therefore, exploiting
intermittency is an optimal alternative to classical
subgrid scale modelling. Until recently, it is not yet clear how does one
extract intermittently active atmospheric scales. I study
the space-time intermittency of highly turbulent flows
i.e. flows with high Reynolds number.
Figure: The vorticity fields after many eddy turn
over times are presented, showing intermittency of
two-dimensional turbulence at moderate Reynolds number. Left: decaying turbulence, right: forced turbulence.
This work aims to develop multiresolution approaches for
investigating intermittency of coherent structures in the
atmosphere. A multiresolution atmospheric modelling system
has been proposed and verified using
a coastal circulation system of a dry atmosphere. Further
extension to understand an appropriate parameterization
for moisture effect and turbulence are in progress.
Fully-Lagrangian adevection schemes for
industrial, environmental, or geoscience applications
Figure: Numerical simulation of a moving front in a
channel. Top:
Fully-Lagrangian, bottom: Eulerian.
A computer model of the
atmosphere or ocean concerns advection dominated flows.
The realization that numerical
treatment of advection on a conventional Eulerian mesh is
plagued with instabilities and unrealistic negative
constituent values has inspired continuous efforts in
finding more elegant tools for improving state-of-the-art
atmospheric
transport and chemistry models.
A fully-Lagrangian advection scheme has been developed for
accurate simulation of advection dominated flow
problems. The model has been compared with standard Eulerian finite different approaches. We found that the fully-Lagrangian model provieded significant improvements in terms of both CPU time and accuracy. Two types of problems were considered: a
two-dimensional flow, where a fluid is injected into a
domain confined in one direction and containing
a resident fluid, and a two-dimensional sea-breeze circulation of a dry atmosphere in the coastal region.
A computer model for the geological storage of greenhouse gasses, and for oil/gas reservoir simulation are potential application of this method. In addition, I am also interested in extending this work towards a fully-Lagrangian 3D simulation of the atmosphere, and in comparing the result with classical approaches - for example - semi-Lagrangian and flux-form Eulerial schemes.
Energy-conserving Computational Fluid
Dynamics (CFD) techniques in complex geometry
In aerodynamics, off-shore drilling, or wind engineering
of buildings, one needs simulate moderate to high Reynolds
number incompressible flows around arbitrary solid
structures. For an adaptive mesh simulation of such flows, a potential challenge is to resolve the coupling between the velocity and pressure such that the incompressibility of the flow is satisfied.
I study the development of novel energy-conserving
algorithms for flow around arbitrary obstacles. In this
approach a penalization method is used to model both the
pressure gradient force and the force exerted by solid obstacles. I am interested to examine this algorithm for complex geometry flows and to compare the result with that of classical projection algorithms.
Figure: Vortex shedding at the wake behind a cylinder. Left:
Adaptive wavelet solution, right: Adapted grid
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