Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0346515
Funder
Australian Research Council
Funding Amount
$507,000.00
Summary
Fluorescence Detector for the Australian National Beamline Facility. X-ray absorption spectroscopy (XAS) is an extremely important synchrotron radiation tool for determining the local structure around an X-ray absorbing atom. This has many applications in the study of materials, minerals, metal complexes, and metalloproteins and can often be used to obtain information that is not available by other techniques, because structural information can be obtained in the solid or solution state and in ....Fluorescence Detector for the Australian National Beamline Facility. X-ray absorption spectroscopy (XAS) is an extremely important synchrotron radiation tool for determining the local structure around an X-ray absorbing atom. This has many applications in the study of materials, minerals, metal complexes, and metalloproteins and can often be used to obtain information that is not available by other techniques, because structural information can be obtained in the solid or solution state and in mixtures. The current proposal is aimed at introducing new technology into the Australian National Beamline Facility that will greatly improve the quality and quantity of experiments that can be performed and extend studies into dilute solutions and protein samples.Read moreRead less
Eddy-resolving global ocean-sea ice modelling. Eddy-resolving global ocean-sea ice modelling. This project aims to develop a world-class global ocean-sea ice model framework through a nationwide consortium. The resulting high resolution models are expected to provide the foundation for the next decade of Australian ocean-sea ice modelling capacity. This research should lead to improved ocean and sea ice prediction, ocean reanalyses, and climate projections, enhancing Australia's capacity to pred ....Eddy-resolving global ocean-sea ice modelling. Eddy-resolving global ocean-sea ice modelling. This project aims to develop a world-class global ocean-sea ice model framework through a nationwide consortium. The resulting high resolution models are expected to provide the foundation for the next decade of Australian ocean-sea ice modelling capacity. This research should lead to improved ocean and sea ice prediction, ocean reanalyses, and climate projections, enhancing Australia's capacity to predict the ocean state on timescales of days to decades. This is expected to yield efficiencies in shipping, marine search and rescue and naval operations, and increase the accuracy of projected future changes in climate, sea level, ocean ecosystems and the cryosphere.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0989747
Funder
Australian Research Council
Funding Amount
$400,000.00
Summary
Ultrafast Dynamics Measurement Facility for the Physical, Biochemical, and Materials Sciences. The term "ultrafast revolution" describes the transformations in science due to ultrafast laser technology. Today, ultrafast lasers are used in surgery, nanomaterial fabrication, biomedical imaging, spectroscopic investigations, and new applications are still emerging. This facility will draw together leading chemists, physicists, and engineers to investigate key ultrafast processes and phenomena in th ....Ultrafast Dynamics Measurement Facility for the Physical, Biochemical, and Materials Sciences. The term "ultrafast revolution" describes the transformations in science due to ultrafast laser technology. Today, ultrafast lasers are used in surgery, nanomaterial fabrication, biomedical imaging, spectroscopic investigations, and new applications are still emerging. This facility will draw together leading chemists, physicists, and engineers to investigate key ultrafast processes and phenomena in the physical, biochemical and material sciences. This is of strategic importance to keep Australia at the global forefront for scientific endeavours, supporting new research and commercial opportunities. This facility will also produce highly trained graduates, who will find employment in industry throughout Australia and globally.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0347797
Funder
Australian Research Council
Funding Amount
$263,000.00
Summary
A Versatile High-resolution X-ray Diffractometer for Materials Research. The aim of this project is to establish a state-of-the-art triple-axis x-ray diffraction facility capable of non-destructively analysing complex semiconductor materials and structures investigated by all Australian semiconductor-growing groups. Growers and device engineers will be able to control growth processes accurately and correlate device performance with structural analysis. Modern triple-axis instruments can also b ....A Versatile High-resolution X-ray Diffractometer for Materials Research. The aim of this project is to establish a state-of-the-art triple-axis x-ray diffraction facility capable of non-destructively analysing complex semiconductor materials and structures investigated by all Australian semiconductor-growing groups. Growers and device engineers will be able to control growth processes accurately and correlate device performance with structural analysis. Modern triple-axis instruments can also be used for high-resolution texture analysis and surface reflectivity measurements on numerous types of materials. Thus chemists, geologists, and materials scientists with interests outside of the semiconductor growth community will gain substantial benefit from this instrument for the investigation of materials of technological and economic importance.Read moreRead less
Galactic Archaeology: A Radial Velocity Experiment to Unveil the History of the Milky Way. The ambitious RAdial Velocity Experiment (RAVE) will measure velocities and chemical properties of 50 million stars in the period 2006-2010 - 2000 times the number measured throughout history. RAVE will use a new-technology Australian fiber spectrometer at the Siding Spring UK Schmidt Telescope. A key demonstrator for RAVE is our proposed pilot survey using existing instruments to measure 100,000 stars - a ....Galactic Archaeology: A Radial Velocity Experiment to Unveil the History of the Milky Way. The ambitious RAdial Velocity Experiment (RAVE) will measure velocities and chemical properties of 50 million stars in the period 2006-2010 - 2000 times the number measured throughout history. RAVE will use a new-technology Australian fiber spectrometer at the Siding Spring UK Schmidt Telescope. A key demonstrator for RAVE is our proposed pilot survey using existing instruments to measure 100,000 stars - already 20 times larger than any previous survey - providing unique chemical and kinematical fingerprints of our Galaxy's formation. This is critical for determining the optimum observing strategy, data management, and software pipeline, before embarking on the full survey in 2006.Read moreRead less
The Last 8 Billion Years of Cosmic Evolution. A key factor in Australia's international prominence in astronomy has been the development and use of innovative instrumentation on its telescopes to undertake major leading-edge surveys. This project will enhance this reputation by using the new AAOmega facility on the 3.9m Anglo-Australian Telescope to make the largest ever survey of galaxies in the distant universe. This will allow us to address the two most important issues in cosmology today - ....The Last 8 Billion Years of Cosmic Evolution. A key factor in Australia's international prominence in astronomy has been the development and use of innovative instrumentation on its telescopes to undertake major leading-edge surveys. This project will enhance this reputation by using the new AAOmega facility on the 3.9m Anglo-Australian Telescope to make the largest ever survey of galaxies in the distant universe. This will allow us to address the two most important issues in cosmology today - the nature of the "dark energy" that is causing the universe's expansion to accelerate, and the detailed role of dark matter in galaxy formation and evolution. Read moreRead less
The fundamental physics governing the formation of cosmic structure. This project will investigate the physics that underlie three of the most fundamental processes within the universe - its accelerated expansion, the formation of cosmic structure, and galaxy formation - thereby contributing to the Priority Goal of Breakthrough Science under National Research Priority 3. It will involve world-leading research in these areas, enabled by innovative instrumentation on Australia's national telescope ....The fundamental physics governing the formation of cosmic structure. This project will investigate the physics that underlie three of the most fundamental processes within the universe - its accelerated expansion, the formation of cosmic structure, and galaxy formation - thereby contributing to the Priority Goal of Breakthrough Science under National Research Priority 3. It will involve world-leading research in these areas, enabled by innovative instrumentation on Australia's national telescope facilities. National benefit will also come via the collaborations it will involve with prestigious North American institutions. These collaborations will lead to new research capability being built within Australia, through knowledge and expertise being vested in young postgraduate and postdoctoral researchers.Read moreRead less
Special Research Initiatives - Grant ID: SR120200004
Funder
Australian Research Council
Funding Amount
$30,000,000.00
Summary
Australian Synchrotron Access Program. The Australian Synchrotron epitomises scientific research excellence in Australian and New Zealand. Its impact spans nearly every research sector. This proposal brings together over 30 Australian universities working together to ensure that world-class peer-reviewed science continues to be performed at the Australian Synchrotron.
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
ARC Complex Open Systems Research Network. Complexity is the common frontier in the physical, biological and social sciences. This Network will link specialists in all three sciences through five generic conceptual and mathematical theme activities. It will promote research into how subsystems self-organise into new emergent structures when assembled into an open, non-equilibrium system. Outcomes will include new technologies and software tools and deeper understanding of fundamental questions i ....ARC Complex Open Systems Research Network. Complexity is the common frontier in the physical, biological and social sciences. This Network will link specialists in all three sciences through five generic conceptual and mathematical theme activities. It will promote research into how subsystems self-organise into new emergent structures when assembled into an open, non-equilibrium system. Outcomes will include new technologies and software tools and deeper understanding of fundamental questions in science. An essential function of the network will be introducing researchers end users to new tools and broadening the horizons of graduate students.Read moreRead less