Supporting early science from the Murchison Widefield Array - a Square Kilometre Array (SKA) pathfinder telescope. The Murchison Widefield Array (MWA) is likely to be the first operational pathfinder for the $2.5 billion Square Kilometre Array (SKA) on one of the two candidate SKA sites - the Murchison Radioastronomy Observatory (MRO) in Western Australia. The MWA will therefore generate large volumes of scientific data before 2012, the expected date of the international decision that will dete ....Supporting early science from the Murchison Widefield Array - a Square Kilometre Array (SKA) pathfinder telescope. The Murchison Widefield Array (MWA) is likely to be the first operational pathfinder for the $2.5 billion Square Kilometre Array (SKA) on one of the two candidate SKA sites - the Murchison Radioastronomy Observatory (MRO) in Western Australia. The MWA will therefore generate large volumes of scientific data before 2012, the expected date of the international decision that will determine whether Australia or South Africa is to host the SKA. The early science results from the MWA will showcase the excellence of the Australian site for radio astronomy and play a significant strategic role in Australia's bid to attract the SKA, as an international mega-science project to Australia, with its benefits to Australian science, industry and society.Read moreRead less
Supporting early science from the Murchison Widefield Array - a Square Kilometre Array (SKA) pathfinder telescope. The Murchison Widefield Array (MWA) is likely to be the first operational pathfinder for the $2.5 billion Square Kilometre Array (SKA) on one of the two candidate SKA sites - the Murchison Radioastronomy Observatory (MRO) in Western Australia. The MWA will therefore generate large volumes of scientific data before 2012, the expected date of the international decision that will dete ....Supporting early science from the Murchison Widefield Array - a Square Kilometre Array (SKA) pathfinder telescope. The Murchison Widefield Array (MWA) is likely to be the first operational pathfinder for the $2.5 billion Square Kilometre Array (SKA) on one of the two candidate SKA sites - the Murchison Radioastronomy Observatory (MRO) in Western Australia. The MWA will therefore generate large volumes of scientific data before 2012, the expected date of the international decision that will determine whether Australia or South Africa is to host the SKA. The early science results from the MWA will showcase the excellence of the Australian site for radio astronomy and play a significant strategic role in Australia's bid to attract the SKA, as an international mega-science project to Australia, with its benefits to Australian science, industry and society.Read moreRead less
Technologies for space based interferometry. This project aims to develop a new method for laser displacement measurements that will be uniquely suited for use in space. These measurements will enable gravitational measurements of unprecedented accuracy. Missions such as GRACE utilise gravitational observations to provide the distribution of melting polar ice, changes in sea levels, and quantitative estimates of ground water in the world’s food bowls. The technique will also allow space-based gr ....Technologies for space based interferometry. This project aims to develop a new method for laser displacement measurements that will be uniquely suited for use in space. These measurements will enable gravitational measurements of unprecedented accuracy. Missions such as GRACE utilise gravitational observations to provide the distribution of melting polar ice, changes in sea levels, and quantitative estimates of ground water in the world’s food bowls. The technique will also allow space-based gravitational wave detectors far simpler than previous proposals. The improved performance, inherent robustness and drastically reduced complexity will enable new classes of missions that would not otherwise be possible. Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100004
Funder
Australian Research Council
Funding Amount
$502,453.00
Summary
Semiconductor laser for adaptive optics in astronomy and space awareness. This project aims to create a laser system for use as a laser guide star. Semiconductor laser technology is a cost effective, highly reliable and compact alternative to expensive, inefficient, bulky laser systems. This laser has wide scientific appeal for research with telescopes in astronomy, and for satellite tracking and mitigation of the threat of space debris. Producing a sodium laser guide star in Australia is expect ....Semiconductor laser for adaptive optics in astronomy and space awareness. This project aims to create a laser system for use as a laser guide star. Semiconductor laser technology is a cost effective, highly reliable and compact alternative to expensive, inefficient, bulky laser systems. This laser has wide scientific appeal for research with telescopes in astronomy, and for satellite tracking and mitigation of the threat of space debris. Producing a sodium laser guide star in Australia is expected to secure the country's position as the premier provider of commercial-grade laser guide star adaptive optics systems for civil and defence telescopes around the world.Read moreRead less
High-cadence near-infrared imaging. This project aims to deploy a cryogenic camera system to improve the outputs of astronomical telescopes. The system is equipped with an emerging detector technology, a near-infrared Avalanche Photo-Diode array, capable of high cadence imaging with frame rates of 10 - 1,000 Hz at a wavelength of around 2.2 microns. This new technology is a key component to the future of adaptive optics systems for astronomical telescopes as it allows the rapid measurements nece ....High-cadence near-infrared imaging. This project aims to deploy a cryogenic camera system to improve the outputs of astronomical telescopes. The system is equipped with an emerging detector technology, a near-infrared Avalanche Photo-Diode array, capable of high cadence imaging with frame rates of 10 - 1,000 Hz at a wavelength of around 2.2 microns. This new technology is a key component to the future of adaptive optics systems for astronomical telescopes as it allows the rapid measurements necessary to correct the image blurring introduced by the Earth's atmosphere. No expertise currently exists in Australia with this new technology. Capitalising on previous investment, the camera system is intended to fill a capability gap in local expertise and to ensure the potential of the next generation of telescopes is realised and strengthen our competitive edge for frontier instrumentation across the wider Australian imaging community.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100008
Funder
Australian Research Council
Funding Amount
$700,000.00
Summary
Australian Seismic Imaging Array. The project aims to create a facility for developing techniques for imaging the deep earth and the surface motion in ambient seismic waves created by wind, waves and human activity. The techniques will enable sources of seismic vibrations to be identified and suppressed, and will allow mapping techniques to be developed for monitoring and discovery of resources such as ground water. Gravitational wave researchers will benefit from the ability to suppress seismic ....Australian Seismic Imaging Array. The project aims to create a facility for developing techniques for imaging the deep earth and the surface motion in ambient seismic waves created by wind, waves and human activity. The techniques will enable sources of seismic vibrations to be identified and suppressed, and will allow mapping techniques to be developed for monitoring and discovery of resources such as ground water. Gravitational wave researchers will benefit from the ability to suppress seismic vibrations, while geophysicists will benefit from new techniques and training. Read moreRead less
Probing the limits of Gravitational Force Sensing. This project will develop innovative laser measurement topologies for probing the limits of gravitational force sensing. Of particular interest is the detection of gravitational waves from astrophysical sources. Technology developed in this project will be able to see gravitational forces from slow moving mass at great distances away. Implementation of this technology will enhance the terrestrial gravitational wave detectors to observe at lower ....Probing the limits of Gravitational Force Sensing. This project will develop innovative laser measurement topologies for probing the limits of gravitational force sensing. Of particular interest is the detection of gravitational waves from astrophysical sources. Technology developed in this project will be able to see gravitational forces from slow moving mass at great distances away. Implementation of this technology will enhance the terrestrial gravitational wave detectors to observe at lower frequencies. This project will ensure Australia's continued involvement in the international Advanced LIGO (Laser Interferometer Gravitational Observatory) project and guarantee Australian participation in the first direct detection of gravitational waves.Read moreRead less