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
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
Optical phased array for space debris tracking and manoeuvring. Space junk in low Earth orbit is increasing at an alarming rate, jeopardising our access to critical navigation, communications, weather and natural disaster warning services. This project will prevent collisions of debris with satellites by developing a new laser system called an optical phased array to track and remotely manoeuvre space debris.
Removing the blur: Guidestar lasers for the space industry . The speed and quality of transferring information between earth and space can be greatly enhanced by adaptive optical systems that provide correction for atmospheric aberrations. The laser-generated guidestars that lie at the heart of these systems must be bright, preferably multi-coloured and with low background. By taking advantage of the unique optical properties of diamond, this project aims to develop lasers that produce these adv ....Removing the blur: Guidestar lasers for the space industry . The speed and quality of transferring information between earth and space can be greatly enhanced by adaptive optical systems that provide correction for atmospheric aberrations. The laser-generated guidestars that lie at the heart of these systems must be bright, preferably multi-coloured and with low background. By taking advantage of the unique optical properties of diamond, this project aims to develop lasers that produce these advanced features to fulfil the needs of the space industry sector. These outcomes are expected to create new services and products in the areas of space situational awareness, space debris management and satellite communications, and have major spin-off benefits to astronomy and defence.Read moreRead less
Space development of the HDLT Australian Plasma Thruster. The collaboration between the ANU research group and ASTRIUM/EADS, the largest European aerospace company, is a unique opportunity for Australia to capitalize on the new discovery of the Helicon Double Layer Thruster made at the ANU. This will allow the Australian space community to stay abreast of international developments in space propulsion and to be with the for-runners of this new technology.
ANU will have direct access to ASTRIUM ....Space development of the HDLT Australian Plasma Thruster. The collaboration between the ANU research group and ASTRIUM/EADS, the largest European aerospace company, is a unique opportunity for Australia to capitalize on the new discovery of the Helicon Double Layer Thruster made at the ANU. This will allow the Australian space community to stay abreast of international developments in space propulsion and to be with the for-runners of this new technology.
ANU will have direct access to ASTRIUM/EADS via the relationships developed in this project putting Australia in the enviable position of being an insider in future space developments concerning plasma thrusters and space technology in general.Read moreRead less
Creating a national time and frequency network for Australia. This project will develop the means to distribute accurate time and frequency across the Australian continent via an optical fibre network. This network will meet the needs of future telecommunications, science and astronomy projects including the Australian bid for the Square Kilometre Array radio-astronomy project.
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
Mapping the dark matter with early type galaxies. Unidentified dark matter outweighs luminous matter (stars, gas, and galaxies) by several times and is detected by its gravitational effects in the Universe. The Six Degree Field Galaxy Survey is now complete and this project will prepare a larger survey, which will put the team clearly in the lead in understanding the distribution of dark matter.
Electron Transpiration Cooling of Hypersonic Vehicles. Future aircraft for flight at hypersonic speeds require sharp leading edges for the best aerodynamic performance. Sharp leading edges incur high heat loads and cannot be adequately cooled with current technologies. The project aim is to investigate novel surface materials that emit electrons when heated. This emission of electrons from the surface can significantly contribute to the cooling of the sharp leading edges. This project is expecte ....Electron Transpiration Cooling of Hypersonic Vehicles. Future aircraft for flight at hypersonic speeds require sharp leading edges for the best aerodynamic performance. Sharp leading edges incur high heat loads and cannot be adequately cooled with current technologies. The project aim is to investigate novel surface materials that emit electrons when heated. This emission of electrons from the surface can significantly contribute to the cooling of the sharp leading edges. This project is expected to deliver new experimental data on novel surface materials exposed to a hypersonic flow environment and computer models that can simulate their cooling effect. This investigation will contribute towards enabling technologies for sustained hypersonic flight by overcoming critical head load limitations.Read moreRead less
Technologies for advanced optical fibre sensors. This project is to create a significantly better technology for exploration of oil and gas reserves under the ocean. Based on lasers and fibre optics, it leverages Australia's prodigious photonics expertise and couples it with Australia's established and well-regarded resource industry. Successful completion will enable better utilization of this country's natural resources, in particular oil and gas reserves, whilst also creating a high technolog ....Technologies for advanced optical fibre sensors. This project is to create a significantly better technology for exploration of oil and gas reserves under the ocean. Based on lasers and fibre optics, it leverages Australia's prodigious photonics expertise and couples it with Australia's established and well-regarded resource industry. Successful completion will enable better utilization of this country's natural resources, in particular oil and gas reserves, whilst also creating a high technology export, given the size of the world marine survey market (US$4 billion). Better energy exploration technologies are vital to Australia and, indeed the world, as energy supply dwindles and the increased energy costs begin to impact negatively on economic growth.Read moreRead less