Vibration Isolation Technology and Instrumentaion for Geophysical Surveys. Many geophysical exploration instruments are limited in sensitivity by vibration induced noise. New techniques of vibration isolation have been shown to eliminate vibration induced noise in a vibrating wire magnetic gradiometer. This project will create fully integrated sensor ?isolation packages for airborne and underwater applications, both for gradiometers and for ground penetrating radars. The project will signific ....Vibration Isolation Technology and Instrumentaion for Geophysical Surveys. Many geophysical exploration instruments are limited in sensitivity by vibration induced noise. New techniques of vibration isolation have been shown to eliminate vibration induced noise in a vibrating wire magnetic gradiometer. This project will create fully integrated sensor ?isolation packages for airborne and underwater applications, both for gradiometers and for ground penetrating radars. The project will significantly benefit the mineral exploration industry as well as underwater detection of cables and ship wrecks.Read moreRead less
Advanced Electromagnetic Sensors and Magnetic Gradiometers for Natural Resources Exploration and Future Space Missions. Australia will benefit from the long-standing world-class mining exploration industry. The new magnetic gradiometer system would greatly enhance their arsenal of geophysical exploration tools, especially for the detection of both magnetically and/or conductive minerals like nickel sulphide. Due to the inherent skin depth issues of conductive cover, a unique condition in Austral ....Advanced Electromagnetic Sensors and Magnetic Gradiometers for Natural Resources Exploration and Future Space Missions. Australia will benefit from the long-standing world-class mining exploration industry. The new magnetic gradiometer system would greatly enhance their arsenal of geophysical exploration tools, especially for the detection of both magnetically and/or conductive minerals like nickel sulphide. Due to the inherent skin depth issues of conductive cover, a unique condition in Australia, a low frequency electromagnetic survey system is one of the best methods to penetrate the cover and investigate deeper geological structures. The low frequency isolation system developed in this project will improve the survey instrument performance down to 4Hz, providing capability to explore resources about 50-100% deeper than existing instrumentation allows.Read moreRead less
Novel High-Q Resonant Structures for Space and Telecommunications. High-Q microwave resonators with low spurious mode density have important applications in telecommunications, radar, navigation, precision metrology and time standards. We will develop high-Q resonators by constructing a dielectric Bragg resonators using monocrystalline sapphire loaded in a copper cavity with new cylindrical and spherical geometries. Based on these devices, compact and economical state-of-the-art ultra-low noise ....Novel High-Q Resonant Structures for Space and Telecommunications. High-Q microwave resonators with low spurious mode density have important applications in telecommunications, radar, navigation, precision metrology and time standards. We will develop high-Q resonators by constructing a dielectric Bragg resonators using monocrystalline sapphire loaded in a copper cavity with new cylindrical and spherical geometries. Based on these devices, compact and economical state-of-the-art ultra-low noise microwave oscillators and hydrogen masers will be built for the telecommunications market and space applications.Read moreRead less
Experiments with Advanced Isolation Systems, Suspension and Test Masses Using ACIGA's High Optical Power Test Facility. This proposal will allow experimental verification of the performcane of of sapphire test masses and their associated isolation and suspension system in ACIGA's high optical power test facility at Gingin. The work will contribute to the worldwide effort to increase the sensitivity of laser interferometers to the level where known sources of gravitational waves can be detected ....Experiments with Advanced Isolation Systems, Suspension and Test Masses Using ACIGA's High Optical Power Test Facility. This proposal will allow experimental verification of the performcane of of sapphire test masses and their associated isolation and suspension system in ACIGA's high optical power test facility at Gingin. The work will contribute to the worldwide effort to increase the sensitivity of laser interferometers to the level where known sources of gravitational waves can be detected at a reasonable rate.Read moreRead less
High Performance Microwave Oscillators for Radars, Comminication Systems and Precision Noise Measurements. The aim of the project is to develop a new class of microwave oscillators with unique combination of properties including low-noise, high frequency stability and reduced sensitivity to vibration. Such oscillators are essential for expanding fields of radar, fiber optics, optical frequency synthesis and metrology.
The industrial partner's focus will be on demands for reduced cost and impro ....High Performance Microwave Oscillators for Radars, Comminication Systems and Precision Noise Measurements. The aim of the project is to develop a new class of microwave oscillators with unique combination of properties including low-noise, high frequency stability and reduced sensitivity to vibration. Such oscillators are essential for expanding fields of radar, fiber optics, optical frequency synthesis and metrology.
The industrial partner's focus will be on demands for reduced cost and improved environmental performance, the university team will focus on improved frequency stability, optimal tuning and novel vibration immunity techniques.
Achieving the project goals will broaden the international markets for the industry partner's products and lead to increased export income for Australia.
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Development of Optical Clocks and Their Applications to Precision Frequency Measurements and Time Keeping. The goal of the proposed international researcher exchange program is to enhance the ongoing collaboration between the Frequency Standards and Metrology (FSM) Group at the University of Western Australia and leading US research institutions, including National Institute of Standards and Technology (NIST) in the field of (i) laser cooled atomic frequency standards, (ii) methods of optical ....Development of Optical Clocks and Their Applications to Precision Frequency Measurements and Time Keeping. The goal of the proposed international researcher exchange program is to enhance the ongoing collaboration between the Frequency Standards and Metrology (FSM) Group at the University of Western Australia and leading US research institutions, including National Institute of Standards and Technology (NIST) in the field of (i) laser cooled atomic frequency standards, (ii) methods of optical frequency synthesis and coherent time transfer between widely separated parts of electromagnetic spectrum and (iii) generation of low noise microwave signals directly from frequency stabilised ultra-fast pulsed lasers.Read moreRead less
Application of ultra-high stability cryogenic sapphire oscillators to Very Long Baseline Interferometry. This project will develop a state-of-the-art commercial prototype of the cryogenic sapphire oscillator (CSO) optimised for use at remote sites. Proof of operation will be applied to the important niche market of Very-Long Baseline Interferometry (VLBI) radio astronomy, with improvements in image quality. The research will also significantly benefit the Australian bid for the SKA project, as ....Application of ultra-high stability cryogenic sapphire oscillators to Very Long Baseline Interferometry. This project will develop a state-of-the-art commercial prototype of the cryogenic sapphire oscillator (CSO) optimised for use at remote sites. Proof of operation will be applied to the important niche market of Very-Long Baseline Interferometry (VLBI) radio astronomy, with improvements in image quality. The research will also significantly benefit the Australian bid for the SKA project, as the CSO is the only technology capable of synchronising the outputs of the telescopes arrays to the required signal to noise to attain the required image quality. The project will further Australia's status in radio astronomy as a world leader and add to our exports of precision scientific instruments.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
Application of Femtosecond Light Sources to Generation of Low Noise Microwave Signals. The main goal of the research project is to develop prototypes of photonic oscillators capable of generating spectrally pure signals both at optical and microwave frequencies. The project is also aimed at understanding noise mechanisms affecting frequency stability of classical microwave oscillators based on sapphire loaded cavity resonators. By cryogenically cooling such resonators we plan to create a new fam ....Application of Femtosecond Light Sources to Generation of Low Noise Microwave Signals. The main goal of the research project is to develop prototypes of photonic oscillators capable of generating spectrally pure signals both at optical and microwave frequencies. The project is also aimed at understanding noise mechanisms affecting frequency stability of classical microwave oscillators based on sapphire loaded cavity resonators. By cryogenically cooling such resonators we plan to create a new family of extremely low noise and economically viable microwave signal sources. The research proposed will enrich the field of oscillator frequency control, give rise to new techniques for precision noise measurements and reinforce Australia's position at the forefront of microwave and photonic science.Read moreRead less
Micro-engineered Optical Fibre Clocks. Clocks and oscillators are crucial components of all communication, navigation and computing technologies. Improvements in the performance of these internal clocks results in improvement in the performance of the dependent system, and are thus of high economic and technological value. A great need presently exists for compact and high performance clocks for improving optical fibre communication systems. The goal of this project is join the expertise of t ....Micro-engineered Optical Fibre Clocks. Clocks and oscillators are crucial components of all communication, navigation and computing technologies. Improvements in the performance of these internal clocks results in improvement in the performance of the dependent system, and are thus of high economic and technological value. A great need presently exists for compact and high performance clocks for improving optical fibre communication systems. The goal of this project is join the expertise of the University of Western Australia group with that of the University of Bath team to develop a new type of clock to fulfil this need.Read moreRead less