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Socio-Economic Objective : Physical sciences
Field of Research : Ionospheric And Magnetospheric Physics
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  • Funded Activity

    Discovery Projects - Grant ID: DP0344361

    Funder
    Australian Research Council
    Funding Amount
    $162,000.00
    Summary
    Localised instabilities in magnetically confined plasmas heated by radio waves. The H-1 Heliac Major National Facility will be used for experiments to search for localised plasma "ballooning" instabilities. These instabilities, studied theoretically but not yet identified in experiments, are thought to limit the pressure achievable in plasmas of interest for production of renewable, low-greenhouse gas emission, fusion power, and are also invoked to explain magnetospheric phenomena like auroral s .... Localised instabilities in magnetically confined plasmas heated by radio waves. The H-1 Heliac Major National Facility will be used for experiments to search for localised plasma "ballooning" instabilities. These instabilities, studied theoretically but not yet identified in experiments, are thought to limit the pressure achievable in plasmas of interest for production of renewable, low-greenhouse gas emission, fusion power, and are also invoked to explain magnetospheric phenomena like auroral substorms. The flexible magnetic configuration, radio frequency (rf) and microwave plasma heating systems, and diagnostic set of H-1 are uniquely suited to this program. Advances in rf plasma techniques and diagnostics will also benefit the development of novel communications and instrumentation technologies.
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    Funded Activity

    Discovery Projects - Grant ID: DP1096901

    Funder
    Australian Research Council
    Funding Amount
    $440,000.00
    Summary
    The Response of the Middle Atmosphere to Solar and Dynamical Forcing. The region of the atmosphere and ionosphere between 50 and 100 km is difficult to measure directly. We will use a unique array of instruments deployed across Australia to study how this region responds to waves generated in the lower atmosphere and to changes in electromagnetic energy from the sun and particle precipitation from the magnetosphere. Outcomes will help our understanding of how the region is responding to rising l .... The Response of the Middle Atmosphere to Solar and Dynamical Forcing. The region of the atmosphere and ionosphere between 50 and 100 km is difficult to measure directly. We will use a unique array of instruments deployed across Australia to study how this region responds to waves generated in the lower atmosphere and to changes in electromagnetic energy from the sun and particle precipitation from the magnetosphere. Outcomes will help our understanding of how the region is responding to rising levels of greenhouse gas concentrations. Cooling effects are already apparent and our research will look for additional evidence of change.
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    Funded Activity

    Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0775621

    Funder
    Australian Research Council
    Funding Amount
    $494,000.00
    Summary
    Mileura Widefield Array: A New Low Frequency Telescope. A new radio-quiet site for international radio astronomy is being developed at Mileura in Western Australia. We have constructed a low frequency test array on the site, and established that the site is excellent for radio astronomy. We plan to build a telescope which will observe the early universe, when stars and galaxies where first born. This will be the first telescope capable of this type of measurement of the early universe. In addi .... Mileura Widefield Array: A New Low Frequency Telescope. A new radio-quiet site for international radio astronomy is being developed at Mileura in Western Australia. We have constructed a low frequency test array on the site, and established that the site is excellent for radio astronomy. We plan to build a telescope which will observe the early universe, when stars and galaxies where first born. This will be the first telescope capable of this type of measurement of the early universe. In addition, the telescope will measure the solar wind, and its potential interactions with the earth.
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    Funded Activity

    Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0451713

    Funder
    Australian Research Council
    Funding Amount
    $583,605.00
    Summary
    Completion of the Tasman International Geospace Environment Radar (TIGER). TIGER is part of an international high frequency radar consortium (SuperDARN) studying the coupling of space weather processes to the ionosphere. This is critical for radio, navigation and surveillance networks. TIGER provides important new information because it extends the global radar coverage significantly equatorward, and it can be combined with other radars in Antarctica and Alaska. However, only one of the two T .... Completion of the Tasman International Geospace Environment Radar (TIGER). TIGER is part of an international high frequency radar consortium (SuperDARN) studying the coupling of space weather processes to the ionosphere. This is critical for radio, navigation and surveillance networks. TIGER provides important new information because it extends the global radar coverage significantly equatorward, and it can be combined with other radars in Antarctica and Alaska. However, only one of the two TIGER radars necessary to carry out these studies has been built. This proposal is for completion of the second radar, to be located in New Zealand. The US Air Force has already granted A$443k toward this project.
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    Funded Activity

    Discovery Projects - Grant ID: DP0559544

    Funder
    Australian Research Council
    Funding Amount
    $260,000.00
    Summary
    DYNAMICS OF EARTH'S RADIATION BELTS. Space weather is produced by rapid variations in wave fields and particle populations in near-Earth space, and has many effects. These include damage to spacecraft (causing operational anomalies and loss of service), degrading the performance of GPS, space-ground, HF radio and cable-based networks, and affecting surveillance radars. The core aim of this project is to improve knowledge of the waves and particles causing these effects. While being important to .... DYNAMICS OF EARTH'S RADIATION BELTS. Space weather is produced by rapid variations in wave fields and particle populations in near-Earth space, and has many effects. These include damage to spacecraft (causing operational anomalies and loss of service), degrading the performance of GPS, space-ground, HF radio and cable-based networks, and affecting surveillance radars. The core aim of this project is to improve knowledge of the waves and particles causing these effects. While being important to aerospace engineers, this work also consolidates Australia's international space profile and provides excellent training in this field. Since space weather causes significant radiation exposure to aircraft crew and passengers this work also has broader ramifications.
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    Funded Activity

    Discovery Projects - Grant ID: DP0664424

    Funder
    Australian Research Council
    Funding Amount
    $383,000.00
    Summary
    Dual Radar Studies of Sub-Auroral Magnetosphere-Ionosphere Coupling. Benefits include: - improved ability to observe, understand and predict space weather impacts on Australia's communications, navigation, and surveillance capabilities; - support for specific Australian programs such as: the JORN the over-the-horizon radar coastal surveillance system; IPS Radio and Space Services space weather monitoring activities (TIGER is a key component of the Australian Space Weather Plan - Strategic Plan .... Dual Radar Studies of Sub-Auroral Magnetosphere-Ionosphere Coupling. Benefits include: - improved ability to observe, understand and predict space weather impacts on Australia's communications, navigation, and surveillance capabilities; - support for specific Australian programs such as: the JORN the over-the-horizon radar coastal surveillance system; IPS Radio and Space Services space weather monitoring activities (TIGER is a key component of the Australian Space Weather Plan - Strategic Planning to 2010 and Beyond); - continue to provide Australia with a central role in the multi-nation SuperDARN project that continues to pioneer new initiatives in successful network operations for scientific studies and for the development of space weather data products for monitoring agencies and other scientists.
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    Funded Activity

    Discovery Projects - Grant ID: DP0663643

    Funder
    Australian Research Council
    Funding Amount
    $239,000.00
    Summary
    Polar Cap Region Boundary Dynamics. Geomagnetic storms have the potential to severely impair critical technology infrastructure. Consequences of strong geomagnetic activity can include power failures, pipeline corrosion, satellite failures, inaccurate GPS positioning and radio navigation. Knowledge of how, where and under which conditions this activity occurs is therefore crucial. The primary aim of this project is to extend our knowledge of the mechanisms by which this activity occurs. This wor .... Polar Cap Region Boundary Dynamics. Geomagnetic storms have the potential to severely impair critical technology infrastructure. Consequences of strong geomagnetic activity can include power failures, pipeline corrosion, satellite failures, inaccurate GPS positioning and radio navigation. Knowledge of how, where and under which conditions this activity occurs is therefore crucial. The primary aim of this project is to extend our knowledge of the mechanisms by which this activity occurs. This work will consolidate Australia's international space profile and provide excellent training in this field, helping Australia's future technology development.
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    Funded Activity

    Linkage - International - Grant ID: LX0239962

    Funder
    Australian Research Council
    Funding Amount
    $28,600.00
    Summary
    Ground based monitoring of plasma dynamics in the magnetosphere. We will use a new technique to study the plasmapause, a fundamental and highly dynamic boundary in geospace. This is usually examined using spacecraft and ground-based VLF measurements, but these suffer several limitations. We have developed the ability to monitor plasma density in geospace, by measuring the resonant frequency of geomagnetic field line oscillations. This project will use data from extensive ground magnetometer a .... Ground based monitoring of plasma dynamics in the magnetosphere. We will use a new technique to study the plasmapause, a fundamental and highly dynamic boundary in geospace. This is usually examined using spacecraft and ground-based VLF measurements, but these suffer several limitations. We have developed the ability to monitor plasma density in geospace, by measuring the resonant frequency of geomagnetic field line oscillations. This project will use data from extensive ground magnetometer arrays to thus study the spatial and temporal variation in particle density near the plasmapause. Comparison with VLF and spacecraft measurements will provide new information on the plasma composition and dynamics in this important region.
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    Funded Activity

    Discovery Projects - Grant ID: DP1096653

    Funder
    Australian Research Council
    Funding Amount
    $185,000.00
    Summary
    Current-free double layers applied to astrophysical objects and space propulsion. The collaboration between the ANU research group and European Aeronautic Defence and Space Company (EADS) ASTRIUM, 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 fore .... Current-free double layers applied to astrophysical objects and space propulsion. The collaboration between the ANU research group and European Aeronautic Defence and Space Company (EADS) ASTRIUM, 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 forerunners of this new technology. ANU will have direct access to EADS-ASTRIUM 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.
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    Funded Activity

    Linkage - International - Grant ID: LX0882515

    Funder
    Australian Research Council
    Funding Amount
    $10,800.00
    Summary
    Ring Current and Radiation Belt Dynamics. Outbursts of energy from the Sun manifest themselves as geomagnetic storms in the Earth's magnetosphere. These storms can severely disrupt and damage advanced technological systems operating on the ground and in space. Operational spacecraft may experience anomalies, pipelines in the long term may corrode and the performance of GPS navigational systems, HF (High Frequency) communications systems, mobile/cell telephone networks and defence surveillance ra .... Ring Current and Radiation Belt Dynamics. Outbursts of energy from the Sun manifest themselves as geomagnetic storms in the Earth's magnetosphere. These storms can severely disrupt and damage advanced technological systems operating on the ground and in space. Operational spacecraft may experience anomalies, pipelines in the long term may corrode and the performance of GPS navigational systems, HF (High Frequency) communications systems, mobile/cell telephone networks and defence surveillance radars may be degraded. It is important to understand the magnetospheric conditions contributing to these problems. This research identifies relevant mechanisms. It also enhances Australia's international space research profile, contributes to Australia's future and supports excellent postgraduate training.
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