Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0560716
Funder
Australian Research Council
Funding Amount
$864,610.00
Summary
A National T-ray Facility. T-rays are between microwaves and infrared on the electromagnetic spectrum. Recently, advances in femtosecond lasers enabled access to T-ray frequencies, producing an important new imaging modality for non-invasive sensing of materials and structures. Internationally, T-rays represent a rich new science leading to advanced forms of biophotonics, biomedical imaging and spectroscopy. Non-invasive T-ray diagnostics of nano- and bio-materials are being hotly pursued. The o ....A National T-ray Facility. T-rays are between microwaves and infrared on the electromagnetic spectrum. Recently, advances in femtosecond lasers enabled access to T-ray frequencies, producing an important new imaging modality for non-invasive sensing of materials and structures. Internationally, T-rays represent a rich new science leading to advanced forms of biophotonics, biomedical imaging and spectroscopy. Non-invasive T-ray diagnostics of nano- and bio-materials are being hotly pursued. The outcome will be a strategically important Australian T-ray facility that will provide immediate and transparent nationwide access. Historically, industry is transformed every time a new part of the electromagnetic spectrum becomes accessible - T-rays are the next frontier.Read moreRead less
High-temperature Elastic Wave Speeds of Mantle Minerals and their Seismological Implications. Laboratory measurements of elastic wave speeds are critical for the interpretation of seismological models for the Earth's deep interior. During the past several years, research groups at ANU and Stony Brook University have separately been proving novel experimental techniques for measurement of the temperature dependence of elastic wave speeds. Now a timely collaboration is proposed in which we would ....High-temperature Elastic Wave Speeds of Mantle Minerals and their Seismological Implications. Laboratory measurements of elastic wave speeds are critical for the interpretation of seismological models for the Earth's deep interior. During the past several years, research groups at ANU and Stony Brook University have separately been proving novel experimental techniques for measurement of the temperature dependence of elastic wave speeds. Now a timely collaboration is proposed in which we would exploit access to similar temperature ranges under two very different pressure regimes to examine the mixed pressure-temperature dependence of wave speeds that is so critical for the inference of chemical composition, mineralogical make-up, and temperature variations within the Earth's mantle.Read moreRead less
DROP DEFORMATION IN CONFINED MICROFLUIDIC GEOMETRIES. Increasingly, high technology applications in biotechnology and microtechnology industries need to process complex (non-Newtonian) fluids with dispersed particles/droplets in channels as small as several microns (microfluidics). A computational fluid dynamic model of non-Newtonian droplet deformation in microfluidic geometries will be developed, and validated using experimental measurements of the flow field in this project. The aim is to und ....DROP DEFORMATION IN CONFINED MICROFLUIDIC GEOMETRIES. Increasingly, high technology applications in biotechnology and microtechnology industries need to process complex (non-Newtonian) fluids with dispersed particles/droplets in channels as small as several microns (microfluidics). A computational fluid dynamic model of non-Newtonian droplet deformation in microfluidic geometries will be developed, and validated using experimental measurements of the flow field in this project. The aim is to understand and quantify factors influencing droplet deformation. Coupling non-Newtonian characteristics with microfluidic geometries will allow the continuous manufacture of micro-particles of specified size and shape for existing and new applications, and will provide guidance for further extending the process to nano-particle manufacture.Read moreRead less
Special Research Initiatives - Grant ID: SR0354517
Funder
Australian Research Council
Funding Amount
$20,000.00
Summary
Adaptive Optics for Australian Astronomy, Medicine, Industry, and Defence. Adaptive optics is a technique for correcting wavefront distortions in light beams to improve optical imaging performance. The Research Network for Adaptive Optics aims to draw together isolated Australian and New Zealand research groups working on adaptive optics applications in disparate areas to achieve a critical mass of researchers in this burgeoning field. Adaptive optics has wide application in areas as diverse as ....Adaptive Optics for Australian Astronomy, Medicine, Industry, and Defence. Adaptive optics is a technique for correcting wavefront distortions in light beams to improve optical imaging performance. The Research Network for Adaptive Optics aims to draw together isolated Australian and New Zealand research groups working on adaptive optics applications in disparate areas to achieve a critical mass of researchers in this burgeoning field. Adaptive optics has wide application in areas as diverse as astronomy, vision science, ophthalmology, microscopy, optical communications, laser radar, and laser beam shaping. The Research Network will coordinate and expand Australian involvement in these areas and inform industry, as have similar networks in the USA and Europe.Read moreRead less
The Evolution of Gas in Galaxy Groups. The evolution of gas in galaxy groups is poorly understood, but is crucial to understanding galaxy evolution. This project provides a training opportunity for a talented postdoc to conduct the first `multiwavelength census' of southern galaxy groups, perform simulations and make predictions of group properties at early times. We will better understand the evolutionary processes in groups and provide a `local anchor' for future surveys. The knowledge gained ....The Evolution of Gas in Galaxy Groups. The evolution of gas in galaxy groups is poorly understood, but is crucial to understanding galaxy evolution. This project provides a training opportunity for a talented postdoc to conduct the first `multiwavelength census' of southern galaxy groups, perform simulations and make predictions of group properties at early times. We will better understand the evolutionary processes in groups and provide a `local anchor' for future surveys. The knowledge gained will feed directly into the design of the future Square Kilometre Array, and raise Australia's profile in this $1B project. We exploit Australia's best astronomical facilities, and establish a new University-CSIRO collaboration.
Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0236657
Funder
Australian Research Council
Funding Amount
$210,000.00
Summary
Renewed Great Melbourne Telescope: Opening a Window on the Universe. We propose to refurbish the Great Melbourne Telescope (GMT) located at Mount Stromlo Observatory with a new state-of-the-art imager. This instrument will be available to the entire Australian Astronomical community, and will allow Australian researchers to undertake cutting edge research with this world leading two colour wide field imager. A fully automated observing and data reduction pipeline, a world first for a telescope o ....Renewed Great Melbourne Telescope: Opening a Window on the Universe. We propose to refurbish the Great Melbourne Telescope (GMT) located at Mount Stromlo Observatory with a new state-of-the-art imager. This instrument will be available to the entire Australian Astronomical community, and will allow Australian researchers to undertake cutting edge research with this world leading two colour wide field imager. A fully automated observing and data reduction pipeline, a world first for a telescope of this size, means astronomers can work on their data, analyzing everything from the Solar System, to the most distant objects in the Universe, rather than spending night after night at the telescope.Read moreRead less
Illuminating the Universe with Exploding Stars. We are using Exploding Stars (Supernovae and Gamma Ray Bursts) to measure fundamental properties of the Universe. We use Type Ia Supernovaeto trace the Expansion History of the Universe and learn about the nature of the Dark Energy which currently dominates the Universe. We use Gamma Ray Bursts to illuminate the gas in and around galaxies to measure the chemical composition and structure of the Early Universe.
Advanced Atomic Sources for Precision Measurement. Many advances in our technology-driven society rely on the precision measurement of quantities such as accelerations, magnetic and electric fields. A higher level of measurement precision leads to a clear economic or strategic advantage. We expect to provide the Australian industrial and government sectors with new and better methods for making precise measurements with accelerometers, gyroscopes and gravity gradiometers. This proposal will pla ....Advanced Atomic Sources for Precision Measurement. Many advances in our technology-driven society rely on the precision measurement of quantities such as accelerations, magnetic and electric fields. A higher level of measurement precision leads to a clear economic or strategic advantage. We expect to provide the Australian industrial and government sectors with new and better methods for making precise measurements with accelerometers, gyroscopes and gravity gradiometers. This proposal will place Australia with only a handful of other countries as an international leader in the new technology of coherent atom interferometry. It is expected that this proposal will lead to innovative prototype devices as well as significant patentable technology. Read moreRead less
Noise-free Cryogenic Wavefront Sensing. This project aims to optimise the prototype adaptive optics technology for the Giant Magellan Telescope (GMT) by leveraging past investment in adaptive optics instrumentation and shortwave infrared detector systems. This project expects to generate significant improvements in GMT performance, with ten times greater image resolution than the Hubble Space Telescope and current estimates of >90% sky coverage, compared with ~50% coverage for current technology ....Noise-free Cryogenic Wavefront Sensing. This project aims to optimise the prototype adaptive optics technology for the Giant Magellan Telescope (GMT) by leveraging past investment in adaptive optics instrumentation and shortwave infrared detector systems. This project expects to generate significant improvements in GMT performance, with ten times greater image resolution than the Hubble Space Telescope and current estimates of >90% sky coverage, compared with ~50% coverage for current technology. Expected outcomes of this project include the development of a highly trained workforce and continued international collaboration in the field of high-technology sensor systems. This contribution to the GMT will provide significant benefits—it will change the way we view the Universe.Read moreRead less
A Laser Guide Star using a High Power, Synchronously Pumped Optical Parametric Oscillators. We will develop a novel high power source of 589nm coherent (laser) light to be used to create a laser guide star by exciting sodium atoms in the earth's upper atmosphere (the mesosphere). This is needed to determine the distortion caused by the atmosphere on an optical beam propagating through it and generate the information needed to correct those distortions using an adaptive optics telescope. This pr ....A Laser Guide Star using a High Power, Synchronously Pumped Optical Parametric Oscillators. We will develop a novel high power source of 589nm coherent (laser) light to be used to create a laser guide star by exciting sodium atoms in the earth's upper atmosphere (the mesosphere). This is needed to determine the distortion caused by the atmosphere on an optical beam propagating through it and generate the information needed to correct those distortions using an adaptive optics telescope. This project focuses on the development of a novel high power 589nm source based on a synchronously pumped optical parametric oscillator.Read moreRead less