The Australian Research Data Commons (ARDC) invites you to participate in a short survey about your
interaction with the ARDC and use of our national research infrastructure and services. The survey will take
approximately 5 minutes and is anonymous. It’s open to anyone who uses our digital research infrastructure
services including Reasearch Link Australia.
We will use the information you provide to improve the national research infrastructure and services we
deliver and to report on user satisfaction to the Australian Government’s National Collaborative Research
Infrastructure Strategy (NCRIS) program.
Please take a few minutes to provide your input. The survey closes COB Friday 29 May 2026.
Complete the 5 min survey now by clicking on the link below.
The mathematics of novel magnetic memory materials. Magnetic memories are the world’s principal device for storing information. The next generation will have greatly increased access speed and data-storage capacity. This project will develop the mathematical theory of these new magnetic memory materials, a crucial first step in understanding and being able to fine-tune their properties.
Numerical modelling of the solar atmosphere. This project will develop a complete and realistic model of the magnetic solar activity using computer simulations of the interconnected solar interior and atmosphere. The results of this project will provide a deeper insight into the physical processes behind solar activity phenomena and will help in the development of methods of solar activity prediction.
Discovery Early Career Researcher Award - Grant ID: DE130100333
Funder
Australian Research Council
Funding Amount
$315,640.00
Summary
A new class of fast and reliable spectral methods for partial differential equations. The project will develop novel fast and reliable spectral methods for computing solutions to general partial differential equations. These methods will be applied to solve important equations that arise in mathematical physics and other areas where high accuracy is essential.
Discovery Early Career Researcher Award - Grant ID: DE140101960
Funder
Australian Research Council
Funding Amount
$332,820.00
Summary
Computational geophysical and astrophysical fluid dynamics at the petascale. The rise of petascale computing provides great potential for new insight, provided one can harness the resources. This project will develop a state-of-the-art computational framework for solving general partial differential equations relevant to many contemporary applications in astrophysics and the geosciences. This project will design a toolkit for maximum extensibility by a large community of scientists and applied m ....Computational geophysical and astrophysical fluid dynamics at the petascale. The rise of petascale computing provides great potential for new insight, provided one can harness the resources. This project will develop a state-of-the-art computational framework for solving general partial differential equations relevant to many contemporary applications in astrophysics and the geosciences. This project will design a toolkit for maximum extensibility by a large community of scientists and applied mathematicians. Building a highly flexible framework allows the agile design and side-by-side comparison of new mathematical models and computational algorithms. This project will employ the new framework on a number of key science areas such as the dynamics of solar magnetism, and tidal interactions in stars and planetary interiors.Read moreRead less
Asymptotics of the exponentially small. Asymptotic analysis plays a vital role in studying the complex interfacial dynamics that are fundamental for practical problems in fluid mechanics such as the withdrawal of oil and gas from underground reservoirs and the optimal design of ship hulls to minimise wave drag. These applications exhibit extremely small physical effects that may be crucially important but cannot be described using classical asymptotic analysis. This project will develop state of ....Asymptotics of the exponentially small. Asymptotic analysis plays a vital role in studying the complex interfacial dynamics that are fundamental for practical problems in fluid mechanics such as the withdrawal of oil and gas from underground reservoirs and the optimal design of ship hulls to minimise wave drag. These applications exhibit extremely small physical effects that may be crucially important but cannot be described using classical asymptotic analysis. This project will develop state of the art mathematical techniques in exponential asymptotics to address this deficiency in the classical theory, and provide a deeper understanding of pattern formation, instabilities and wave propagation on the interface between two fluids.Read moreRead less
Advanced simulation methods for the coupled solar interior and atmosphere. This project aims to develop numerical methods for complex magnetohydrodynamic simulations able to handle sharp and dynamically evolving inhomogeneities, spherical geometries, and dramatic variations in density and wave speed across the simulation domain. The project plans to develop these methods within the context of solar wave processes, which are fundamental to the transfer of energy from the sun’s interior to its out ....Advanced simulation methods for the coupled solar interior and atmosphere. This project aims to develop numerical methods for complex magnetohydrodynamic simulations able to handle sharp and dynamically evolving inhomogeneities, spherical geometries, and dramatic variations in density and wave speed across the simulation domain. The project plans to develop these methods within the context of solar wave processes, which are fundamental to the transfer of energy from the sun’s interior to its outer atmosphere, to the acceleration of the solar wind that rushes past the Earth continually, and to solar activity in general. This would provide the best available modelling of how the sun's atmosphere works, with direct implications for how the Earth's space environment is determined by solar storms and eruptions.Read moreRead less
A semiclassical approach to spectral theory. Spectral theory is the branch of mathematics dealing with natural frequencies (eigenvalues) and modes of vibration (eigenfunctions) of systems arising in geometry, quantum physics and engineering. As such, they have important applications in seismic and medical imaging, nanotechnology, and optical communications. This project aims to use recently developed mathematical tools to advance our understanding of high energy eigenvalues and eigenfunctions, a ....A semiclassical approach to spectral theory. Spectral theory is the branch of mathematics dealing with natural frequencies (eigenvalues) and modes of vibration (eigenfunctions) of systems arising in geometry, quantum physics and engineering. As such, they have important applications in seismic and medical imaging, nanotechnology, and optical communications. This project aims to use recently developed mathematical tools to advance our understanding of high energy eigenvalues and eigenfunctions, as well as new algorithms for numerically computing them.Read moreRead less
Anisotropy and flow in fast-particle dominated and burning tokamak plasmas: stability of ITER and the coming demonstration fusion power plant. This project will identify how beam injected and fusion born alphas affect the magnetic ?eld and excite wave modes in spherical tokamaks, where these particles have the most impact. Understanding these effects is critical to long pulse operation of high performance tokamaks with burning plasmas. In the UK spherical tokamak MAST for instance, fast ion driv ....Anisotropy and flow in fast-particle dominated and burning tokamak plasmas: stability of ITER and the coming demonstration fusion power plant. This project will identify how beam injected and fusion born alphas affect the magnetic ?eld and excite wave modes in spherical tokamaks, where these particles have the most impact. Understanding these effects is critical to long pulse operation of high performance tokamaks with burning plasmas. In the UK spherical tokamak MAST for instance, fast ion driven bursty “chirping modes” and “?shbone” modes evolve into "long-lived" modes damaging plasma performance. This project will resolve the physics of the seed fast ion driven mode, its linear threshold and fully nonlinear evolution. Wider outcomes include scoping the impact of beams and alphas in next step burning plasma experiments, such as a nuclear facility for materials development, ITER, and a fusion power plant.Read moreRead less
Emergence and control of self-organisation in fusion plasmas: through the International Thermonuclear Experimental Reactor (ITER) and beyond. Fusion is a carbon free technology, which promises millions of years of base-load power. The promise has led to massive support for the proof-of-principle experiment, ITER. A challenge facing ITER is minimising edge instabilities, which can destroy the plasma facing wall. The project will explore if a new model can describe and control these instabilities.
Robust numerical solution of partial differential equations on petascale computer systems with applications to tsunami modelling and plasma physics. The project will apply new mathematical ideas to exploit the unprecedented computational resources provided by the next generation of high performance computers. The resulting techniques and software will form a key component for the science needed to understand the workings of complex dynamical systems, such as tsunamis and fusion reactors.