WAVES IN THE MIDDLE ATMOSPHERE. Atmospheric waves have a profound influence in the atmosphere. A unique network of radars in the southern hemisphere will be used to study wave processes in the upper atmosphere. The project will investigate causes of wave variability, wave sources and wave-wave interactions and will involve satellite measurements and international collaboration. Results will guide the development and testing of schemes that incorporate the effects of small-scale waves in numerica ....WAVES IN THE MIDDLE ATMOSPHERE. Atmospheric waves have a profound influence in the atmosphere. A unique network of radars in the southern hemisphere will be used to study wave processes in the upper atmosphere. The project will investigate causes of wave variability, wave sources and wave-wave interactions and will involve satellite measurements and international collaboration. Results will guide the development and testing of schemes that incorporate the effects of small-scale waves in numerical weather and climate models. Outcomes from the project will have application in modelling climate change.Read moreRead less
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
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0989093
Funder
Australian Research Council
Funding Amount
$1,800,000.00
Summary
Australian Partnership in Advanced LIGO. Advanced Interferometer Gravitational-Wave Observatory (LIGO) (AdvLIGO) will be the first gravitational wave observatory capable of frequent observation of known sources of gravitational waves leading to the birth of gravitational wave astronomy. The development of instruments capable of doing this is driving technology in fields such as lasers , optics, photonics and data analysis. By playing a key role in this facility, Australia will reap the scienti ....Australian Partnership in Advanced LIGO. Advanced Interferometer Gravitational-Wave Observatory (LIGO) (AdvLIGO) will be the first gravitational wave observatory capable of frequent observation of known sources of gravitational waves leading to the birth of gravitational wave astronomy. The development of instruments capable of doing this is driving technology in fields such as lasers , optics, photonics and data analysis. By playing a key role in this facility, Australia will reap the scientific and technical rewards of being part of the most exciting frontier of physics in the 21st Century whilst training scientists and technologists for tomorrow.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0453743
Funder
Australian Research Council
Funding Amount
$237,654.00
Summary
Advanced Materials Laser Characterisation Facility. A networked laser facility spanning the University of Melbourne, Monash University, the University of Adelaide, and Flinders University, will be created by integrating new laser instrumentation with existing specialised infrastructure. The facility will provide chemists at the four institutions with the necessary equipment to collaboratively investigate and optimise the properties of a diverse array of advanced materials, including nanoparticle ....Advanced Materials Laser Characterisation Facility. A networked laser facility spanning the University of Melbourne, Monash University, the University of Adelaide, and Flinders University, will be created by integrating new laser instrumentation with existing specialised infrastructure. The facility will provide chemists at the four institutions with the necessary equipment to collaboratively investigate and optimise the properties of a diverse array of advanced materials, including nanoparticles, polymers, biomaterials, and artificial photosynthetic systems. The outcome will be a world-class research network, outfitted with a suite of sophisticated techniques that are not currently available at any single university, or through any other Australian institution or consortium.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0883111
Funder
Australian Research Council
Funding Amount
$570,000.00
Summary
A Laser Facility for Imaging the Time Evolution of Scalars in Turbulent Flows. Establishing this facility will maintain Australia's position at the international leading edge of research in energy, the environment, combustion, and fluid mechanics. The new diagnostics capabilities will advance science through projects that serve the first National Research Priority and assist industry in the design and development of clean combustion devices and energy efficient technologies. The new facility wil ....A Laser Facility for Imaging the Time Evolution of Scalars in Turbulent Flows. Establishing this facility will maintain Australia's position at the international leading edge of research in energy, the environment, combustion, and fluid mechanics. The new diagnostics capabilities will advance science through projects that serve the first National Research Priority and assist industry in the design and development of clean combustion devices and energy efficient technologies. The new facility will also be made available to researchers from non-participating institutions at operating costs and will provide the training platform for graduates from all Australian Universities. This will ensure the continuity of future research and developments in these and related fields in Australia.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0882792
Funder
Australian Research Council
Funding Amount
$600,000.00
Summary
High Power Laser, Test Masses, Digital Control System and Vacuum System for High Optical Power Interferometry Experiments. Gravitational waves are expected to offer humanity a completely new spectrum with which to study the Universe. Australia has been a pioneer in the quest to open up this new spectrum. This project will allow Australia to play a key role in a world-wide project which aims for the first time to enable gravitational waves to be detected from black holes and neutron stars through ....High Power Laser, Test Masses, Digital Control System and Vacuum System for High Optical Power Interferometry Experiments. Gravitational waves are expected to offer humanity a completely new spectrum with which to study the Universe. Australia has been a pioneer in the quest to open up this new spectrum. This project will allow Australia to play a key role in a world-wide project which aims for the first time to enable gravitational waves to be detected from black holes and neutron stars throughout the universe. It will give Australia access to developed technologies, and will be a major boost to physical science research and education.Read moreRead less
Novel Mass Spectrometric Approaches to the Study of Protein-Protein Interactions. Protein-protein interactions mediate all fundamental cellular processes, yet the structural complexity of protein assemblies mean they are often difficult to characterise using traditional analytical methods. This project will develop and demonstrate novel mass spectrometric approaches towards a molecular level description of the structure and interactions of biological protein complexes, which in turn may underpi ....Novel Mass Spectrometric Approaches to the Study of Protein-Protein Interactions. Protein-protein interactions mediate all fundamental cellular processes, yet the structural complexity of protein assemblies mean they are often difficult to characterise using traditional analytical methods. This project will develop and demonstrate novel mass spectrometric approaches towards a molecular level description of the structure and interactions of biological protein complexes, which in turn may underpin the rational design of drugs for the treatment of a range of human health conditions. This project will also provide training of young researchers to the highest international standards in mass spectrometry and protein science, for benefit to Australian industry and research.Read moreRead less
Non-Covalent Interactions Probed by Velocity Map Imaging. Our research program concerns non-covalent interactions, which are of fundamental importance in a range of areas including condensed phase chemistry, the folding of large molecules, biomolecule shape, host-guest chemistry and molecular self-assembly. We probe non-covalent interactions through studies of van der Waals molecules, which involve two or more molecules or atoms held together by non-covalent forces. Our group has developed new ....Non-Covalent Interactions Probed by Velocity Map Imaging. Our research program concerns non-covalent interactions, which are of fundamental importance in a range of areas including condensed phase chemistry, the folding of large molecules, biomolecule shape, host-guest chemistry and molecular self-assembly. We probe non-covalent interactions through studies of van der Waals molecules, which involve two or more molecules or atoms held together by non-covalent forces. Our group has developed new experimental methodologies for determining the strength of intermolecular interactions and these will be used to study the effect of 3-body interactions. Because of their role in chemical reaction, we will also undertake detailed studies of complexes involving radical species.Read moreRead less
Particle astrophysics with the Pierre Auger observatory. Australia's scientific reputation is enhanced through participation in international collaborations that aim to solve long-standing mysteries in science. The Pierre Auger Observatory covers a huge 3000 square km in western Argentina, where we are attempting to solve one of the biggest puzzles in modern astrophysics - the origin of the highest energy cosmic rays, particles 100 million times more energetic than we can produce on Earth. Ade ....Particle astrophysics with the Pierre Auger observatory. Australia's scientific reputation is enhanced through participation in international collaborations that aim to solve long-standing mysteries in science. The Pierre Auger Observatory covers a huge 3000 square km in western Argentina, where we are attempting to solve one of the biggest puzzles in modern astrophysics - the origin of the highest energy cosmic rays, particles 100 million times more energetic than we can produce on Earth. Adelaide scientists were founding members of the Auger project, and now have leading roles within the experiment. This is providing our students with access to world-class facilities and researchers in a field which has moved to the mainstream of astrophysics research.Read moreRead less
Searches for the Origin of Ultra-High Energy Cosmic Rays. The highest energy cosmic rays are the most energetic particles known in the Universe, but we do not know their origin. The ARC-supported Pierre Auger Project is now beginning data acquistion, and will be fully constructed in 2005, with a collecting power 10 times larger than previous experiments. The proposed fellow will collaborate with the Adelaide group in searching for clusters of arrival directions, with an aim of discovering astro ....Searches for the Origin of Ultra-High Energy Cosmic Rays. The highest energy cosmic rays are the most energetic particles known in the Universe, but we do not know their origin. The ARC-supported Pierre Auger Project is now beginning data acquistion, and will be fully constructed in 2005, with a collecting power 10 times larger than previous experiments. The proposed fellow will collaborate with the Adelaide group in searching for clusters of arrival directions, with an aim of discovering astrophysical sources. This project will involve sophisticated event reconstruction and analysis techniques, which take advantage of Auger's unique combination of huge collecting power and good control of systematic uncertainties.Read moreRead less