Innovative solutions to enhance space situational awareness. This project seeks to significantly advance Australia's space situational awareness by researching advanced orbit prediction techniques. The development of novel space object orbit prediction techniques will greatly improve collision warnings for satellite operators that provide essential space-based services to Australian Government and industries.
Stellar chemical signatures of planet formation. Through demanding observations with the largest telescopes and extremely accurate analyses, the project will search for the characteristic fingerprints of planet formation imprinted in the chemical compositions of the sun and stars that we have discovered. The work will shed light on the origin of the solar system and identify stars harbouring planets.
Understanding the sources of the slow solar wind. This project aims to reveal the origins of the slow solar wind, a continuous stream of plasma emanating from the Sun that fills the solar system and impacts the Earth. This project expects to enhance our understanding of how this solar wind is accelerated and structured using a suite of state-of-the-art computational simulations. In doing this, the project expects to provide critical physical understanding to allow interpretation of data from NA ....Understanding the sources of the slow solar wind. This project aims to reveal the origins of the slow solar wind, a continuous stream of plasma emanating from the Sun that fills the solar system and impacts the Earth. This project expects to enhance our understanding of how this solar wind is accelerated and structured using a suite of state-of-the-art computational simulations. In doing this, the project expects to provide critical physical understanding to allow interpretation of data from NASA and ESA's flagship space missions Parker Solar Probe and Solar Orbiter. Benefits should include enhanced physical understanding that will contribute to the international effort to develop reliable space-weather forecasting systems, critical for space exploration and space-based technology.Read moreRead less
Next generation space weather forecasts. Next generation space weather forecasts. This project aims to improve Australia's space weather prediction capabilities by developing space weather forecasts that use ground- and space-based GPS data. The Earth's ionosphere is temporally and spatially variable and the small number of observations limits understanding of its dynamics and effects on radio waves. Using ground- and space-based GPS to remotely sound the ionosphere increases this coverage and c ....Next generation space weather forecasts. Next generation space weather forecasts. This project aims to improve Australia's space weather prediction capabilities by developing space weather forecasts that use ground- and space-based GPS data. The Earth's ionosphere is temporally and spatially variable and the small number of observations limits understanding of its dynamics and effects on radio waves. Using ground- and space-based GPS to remotely sound the ionosphere increases this coverage and can be used to develop space weather forecasts tailored to industries that heavily rely on GPS and satellite communications. An expected direct outcome of this research is modernised space weather forecasts, with economic benefits for several industries.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
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
Prediction of coronal mass ejections and their radio emissions. This project aims to explain in detail the motion and properties of coronal mass ejections (CMEs) leaving the sun, the radio emissions they generate, and space weather triggers for the sun and other stars. The project expects to create new knowledge in the fields of space, plasma, and astro-physics and space weather research. Expected outcomes include capabilities to accurately predict CMEs and space weather triggers from the sun to ....Prediction of coronal mass ejections and their radio emissions. This project aims to explain in detail the motion and properties of coronal mass ejections (CMEs) leaving the sun, the radio emissions they generate, and space weather triggers for the sun and other stars. The project expects to create new knowledge in the fields of space, plasma, and astro-physics and space weather research. Expected outcomes include capabilities to accurately predict CMEs and space weather triggers from the sun to Earth and theories for type II and IV solar radio bursts. Benefits include high-level training and enhanced human capital and scientific prominence for Australia.Read moreRead less
Integrated Observation, Theory, and Simulation of Type II Solar Radio Bursts. Type II solar radio bursts are associated with solar flares, coronal mass ejections (CMEs), and space weather events at Earth. They are the archetype of collective radio emission associated with shocks. This project aims to: answer longstanding fundamental scientific questions about type IIs using the new Murchison Widefield Array (MWA) and NASA spacecraft, while developing a new Australian capability in solar radio ph ....Integrated Observation, Theory, and Simulation of Type II Solar Radio Bursts. Type II solar radio bursts are associated with solar flares, coronal mass ejections (CMEs), and space weather events at Earth. They are the archetype of collective radio emission associated with shocks. This project aims to: answer longstanding fundamental scientific questions about type IIs using the new Murchison Widefield Array (MWA) and NASA spacecraft, while developing a new Australian capability in solar radio physics; perform new observations and theoretical calculations of relevant emission mechanisms, and, develop a new integrated data-tested theory and simulation capability for type II bursts that explains the emissions quantitatively, and positions us to predict the arrival of CMEs and related space weather at Earth. Read moreRead less
Integrated data-tested theory and modelling of type three solar radio emissions. Type three solar radio emissions, the Sun's most powerful and common, are the archetypal collective radio phenomenon in space physics and astrophysics. The project will integrate new theoretical work and simulations into a first integrated data-tested theory that can explain type three bursts, resolve long standing issues, and constrain solar physics.
Prediction of solar activity and space weather by automated analyses of solar radio and magnetic field observations and simulations. This project will build world-recognised capabilities to forecast space weather events at Earth in time to take protective measures. It involves around the clock automated identification and analysis of specific solar radio bursts, forecasting solar activity that results in transients moving Earth-ward, and simulations to predict when these will reach Earth.