Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0668481
Funder
Australian Research Council
Funding Amount
$140,385.00
Summary
Time-resolved observation of highly transient events by a novel digital high-speed camera. Highly transient, that is, rapidly changing, events occur in nature and in almost every field of science and engineering. Knowledge and understanding of these processes is vital for the design of better and innovative machines, materials and instruments. Valuable insight into these processes can be gained if one can visualise them by means of high-speed photography. This application seeks the acquisition o ....Time-resolved observation of highly transient events by a novel digital high-speed camera. Highly transient, that is, rapidly changing, events occur in nature and in almost every field of science and engineering. Knowledge and understanding of these processes is vital for the design of better and innovative machines, materials and instruments. Valuable insight into these processes can be gained if one can visualise them by means of high-speed photography. This application seeks the acquisition of a novel and unique digital camera system that would allow one to observe rapidly occurring processes with unprecedented clarity. The availability of such a system would significantly strengthen cutting-edge research activities in various disciplines that would ultimately lead to the development of original and innovative products.Read moreRead less
Interstellar Gas Dynamics. The conversion of interstellar gas into stars is a key process in the life-history of galaxies and the formation of planetary systems. Star formation takes place within a heterogeneous, dynamic cloud, and entails a million-fold contraction controlled by a complex interplay between gravity, magnetic forces, ionisation balance, chemical reactions and particles of interstellar dust. Previous modelling has adopted inappropriate approximations for the evolution of the mag ....Interstellar Gas Dynamics. The conversion of interstellar gas into stars is a key process in the life-history of galaxies and the formation of planetary systems. Star formation takes place within a heterogeneous, dynamic cloud, and entails a million-fold contraction controlled by a complex interplay between gravity, magnetic forces, ionisation balance, chemical reactions and particles of interstellar dust. Previous modelling has adopted inappropriate approximations for the evolution of the magnetic field. This research will bring a rigorous treatment of magnetic diffusion to bear on the theory of cloud evolution, shock waves, star formation and protoplanetary discs.
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Discovery Early Career Researcher Award - Grant ID: DE200100168
Funder
Australian Research Council
Funding Amount
$312,566.00
Summary
Fast predictive tools for suspensions of slender fibres in viscous fluids. This project aims to develop an effective toolbox for modelling suspensions of slender fibres in viscous fluids. Though little is understood about the interactions of fibres in viscous fluids, such configurations occur frequently in nature and industry: e.g. sperm gather together and swim by waving slender filaments, and collections of carbon fibres are injection molded to manufacture machine parts. Current models are qua ....Fast predictive tools for suspensions of slender fibres in viscous fluids. This project aims to develop an effective toolbox for modelling suspensions of slender fibres in viscous fluids. Though little is understood about the interactions of fibres in viscous fluids, such configurations occur frequently in nature and industry: e.g. sperm gather together and swim by waving slender filaments, and collections of carbon fibres are injection molded to manufacture machine parts. Current models are qualitative or require large computations. This project will use ideas from colloidal suspensions and state-of-the-art asymptotic techniques to develop a refined toolbox for collections of slender fibres in viscous flow. These methods could help understand infertility, develop new technologies and optimise manufacturing.Read moreRead less
Feedback Processes in Galaxy Formation. We have an opportunity to combine the best Australian theory with the best local and international telescopes, to probe the murky story of how galaxies form and why they look they way they do today. By looking back to a time when the Universe was only 1 billion years old, and comparing what we see with cutting edge supercomputer simulations plus pure theory, we will gain insight into the birth of entire galaxies. The results will form part of the study o ....Feedback Processes in Galaxy Formation. We have an opportunity to combine the best Australian theory with the best local and international telescopes, to probe the murky story of how galaxies form and why they look they way they do today. By looking back to a time when the Universe was only 1 billion years old, and comparing what we see with cutting edge supercomputer simulations plus pure theory, we will gain insight into the birth of entire galaxies. The results will form part of the study of how the universe works - that is driving astrophysics today, and represents pure research for the sake of advancing knowledge and showing us where we fit into the Universe. In doing so we will also advance Australia's base of theoretical and computational expertise.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE160100194
Funder
Australian Research Council
Funding Amount
$250,000.00
Summary
Optical diagnostics for the investigation of high-speed energetic processes. Optical diagnostics for the investigation of high-speed energetic processes:
The project seeks to establish equipment to enable the investigation of high-speed energetic processes. Such processes, where large amounts of energy are released over a short time frame, occur in nature and almost every field of science and engineering, and their investigation is a formidable challenge. This challenge is designed to be met th ....Optical diagnostics for the investigation of high-speed energetic processes. Optical diagnostics for the investigation of high-speed energetic processes:
The project seeks to establish equipment to enable the investigation of high-speed energetic processes. Such processes, where large amounts of energy are released over a short time frame, occur in nature and almost every field of science and engineering, and their investigation is a formidable challenge. This challenge is designed to be met through the combined use of state-of-the-art flow visualisation, thermography and spectrometry equipment. These diagnostics would open avenues into so far impossible or difficult to conduct research on highly transient phenomena in various research fields, which include various aspects of fluid mechanics, combustion, and fracture mechanics. The equipment would be instrumental in the design of better and innovative machines, materials, instruments and processes.Read moreRead less
Turbulent mixing of a passive scalar. Turbulence is the usual state of fluid motion. This proposal will increase Australia's expertise in fundamental turbulence research, especially in the area of turbulent mixing, which is of major importance in many natural and engineering problems involving combustion, chemical reactions and pollution. A better knowledge of mixing at small scales will lead to more efficient combustion, savings in energy expenditure as well as a reduction in pollutant emiss ....Turbulent mixing of a passive scalar. Turbulence is the usual state of fluid motion. This proposal will increase Australia's expertise in fundamental turbulence research, especially in the area of turbulent mixing, which is of major importance in many natural and engineering problems involving combustion, chemical reactions and pollution. A better knowledge of mixing at small scales will lead to more efficient combustion, savings in energy expenditure as well as a reduction in pollutant emissions. Read moreRead less
Forces on Particles in Flows Traversing a Magnetic Field. The influence of magnetic fields on the motion of particles near surfaces will be examined using quiescent and shear flow fields at low Reynolds numbers. This theoretical and experimental study will produce a precise theoretical understanding of the motion, including the shear induced lift-force, and hence a basis for controlling the interaction of the particle with the adjacent surface. This fundamental study will provide the foundations ....Forces on Particles in Flows Traversing a Magnetic Field. The influence of magnetic fields on the motion of particles near surfaces will be examined using quiescent and shear flow fields at low Reynolds numbers. This theoretical and experimental study will produce a precise theoretical understanding of the motion, including the shear induced lift-force, and hence a basis for controlling the interaction of the particle with the adjacent surface. This fundamental study will provide the foundations needed to apply magnetic fields to a broad range of emerging problems in nano-technology and biotechnology, and help train and educate a student at the PhD level in the area.Read moreRead less
Effect of forcing on the turbulent mixing of a passive scalar. This project will increase Australia’s expertise in the area of turbulence, which is the usual state of fluid motion . A better knowledge of turbulent mixing will lead to more efficient combustion, savings in energy expenditure as well as a reduction in pollutant emissions.
Rarefied hypervelocity separated flow in the transitional to continuum regimes. The transition regime for low-density flows is a no-man's-land between free-molecular and continuum flow, where the flow behaves differently to the assumptions typically used for modelling either flow type. Bird's direct Simulation Monte Carlo (DSMC) method is typically thought to be the best way of modelling these flows, but has not produced excellent agreement with previous experiments on low-density separated flow ....Rarefied hypervelocity separated flow in the transitional to continuum regimes. The transition regime for low-density flows is a no-man's-land between free-molecular and continuum flow, where the flow behaves differently to the assumptions typically used for modelling either flow type. Bird's direct Simulation Monte Carlo (DSMC) method is typically thought to be the best way of modelling these flows, but has not produced excellent agreement with previous experiments on low-density separated flows, due to computational limitations and lack of knowledge of the flow's internal energy. This proposal is a blind test of the best current DSMC codes against our experiments and a hypersonic continuum code, with the full internal energy state of the flow experimentally quantified for the first time.Read moreRead less
Nanorheology: Hydrodynamic Slip in Newtonian Fluids. Understanding fluid flow across a surface is essential to a great number of technologies. For over one hundred years it has been assumed that the layer of fluid adjacent to the solid moves with the solid, this is known as the no-slip boundary condition. Recently direct force balance measurements of aqueous Newtonian solutions have indicated the presence of boundary slip. Using a newly developed nanorheology technique we will systematically inv ....Nanorheology: Hydrodynamic Slip in Newtonian Fluids. Understanding fluid flow across a surface is essential to a great number of technologies. For over one hundred years it has been assumed that the layer of fluid adjacent to the solid moves with the solid, this is known as the no-slip boundary condition. Recently direct force balance measurements of aqueous Newtonian solutions have indicated the presence of boundary slip. Using a newly developed nanorheology technique we will systematically investigate the conditions that control boundary slip. This information will be used to quantify, model and control boundary slip, progressing the fields of microfluidics, particle deposition, and colloid stability.Read moreRead less