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.Read moreRead less
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.Read moreRead less
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.Read moreRead less
Electromagnetic Ion Cyclotron Waves and Magnetosphere Plasma Dynamics. Space weather, manifest as magnetic storms in the Earth's magnetosphere, can severely disrupt and damage advanced technological systems operating in space and on the ground. Spacecraft may experience operational anomalies, pipeline corrosion may eventuate in the long term, and the performance of GPS navigation systems, HF communication systems, mobile phone networks, and surveillance radars, may be degraded. Knowledge of the ....Electromagnetic Ion Cyclotron Waves and Magnetosphere Plasma Dynamics. Space weather, manifest as magnetic storms in the Earth's magnetosphere, can severely disrupt and damage advanced technological systems operating in space and on the ground. Spacecraft may experience operational anomalies, pipeline corrosion may eventuate in the long term, and the performance of GPS navigation systems, HF communication systems, mobile phone networks, and surveillance radars, may be degraded. Knowledge of the near-Earth space environment under which these problems occur is extremely important. This project identifies relevant mechanisms. The research consolidates Australia's international space profile, provides excellent postgraduate training in the field, and contributes to Australia's future technological development.Read moreRead less
Physics of extreme brightness temperatures in radioastronomical sources. Pulsars and some quasars are so very bright that the conventional explanation for radioastronomical emission from other sources either does not apply to them, or presents unsolved problems. We see (in radio waves) these sources through the interstellar medium which acts like a wrinkled pane of glass in distorting the image. New scientific ideas and methodologies are proposed here and will be explored in the project, with th ....Physics of extreme brightness temperatures in radioastronomical sources. Pulsars and some quasars are so very bright that the conventional explanation for radioastronomical emission from other sources either does not apply to them, or presents unsolved problems. We see (in radio waves) these sources through the interstellar medium which acts like a wrinkled pane of glass in distorting the image. New scientific ideas and methodologies are proposed here and will be explored in the project, with the objective to understand these sources and to extract information on their propreties and those of the interstellar medium. Read moreRead less
Interstellar Gas Dynamics. The conversion of interstellar gas into stars is a key process in the life-history of galaxies and the formation of planetary systems. Star formation takes place within a heterogeneous, dynamic cloud, and entails a million-fold contraction controlled by a complex interplay between gravity, magnetic forces, ionisation balance, chemical reactions and particles of interstellar dust. Previous modelling has adopted inappropriate approximations for the evolution of the mag ....Interstellar Gas Dynamics. The conversion of interstellar gas into stars is a key process in the life-history of galaxies and the formation of planetary systems. Star formation takes place within a heterogeneous, dynamic cloud, and entails a million-fold contraction controlled by a complex interplay between gravity, magnetic forces, ionisation balance, chemical reactions and particles of interstellar dust. Previous modelling has adopted inappropriate approximations for the evolution of the magnetic field. This research will bring a rigorous treatment of magnetic diffusion to bear on the theory of cloud evolution, shock waves, star formation and protoplanetary discs.
Read moreRead less
Scanning Probe Microscopy for Fabrication and Analysis of Polymer Photovoltaics. Australian economic growth will depend increasingly on the provision of devices using materials designed at the molecular level. Scanning probe microscopy, which uses tips placed very close to surfaces to analyse or modify the surfaces with molecular precision, is an indispensible tool in designing such materials. In this project, scanning probe microscopy will be used to analyse and build structures on polymer sola ....Scanning Probe Microscopy for Fabrication and Analysis of Polymer Photovoltaics. Australian economic growth will depend increasingly on the provision of devices using materials designed at the molecular level. Scanning probe microscopy, which uses tips placed very close to surfaces to analyse or modify the surfaces with molecular precision, is an indispensible tool in designing such materials. In this project, scanning probe microscopy will be used to analyse and build structures on polymer solar cells in order to maximise the efficiency of the cells and build prototype nanoscale polymer devices. This will lead to the improvement in devices delivering sustainable energy production - a technology which has the promise of producing energy cheaply from sunlight.Read moreRead less
The application of Markov Chain Monte Carlo methods to the search for space-time variations of fundamental constants. This work will establish Australia as the world leader in one of the most vibrant topics in current physics research. The results obtained could reveal extra dimensions in our universe and provide the first experimental evidence for string theories. The proposed research will also fundamental new information about dark matter and dark energy, the two most pressing problems in c ....The application of Markov Chain Monte Carlo methods to the search for space-time variations of fundamental constants. This work will establish Australia as the world leader in one of the most vibrant topics in current physics research. The results obtained could reveal extra dimensions in our universe and provide the first experimental evidence for string theories. The proposed research will also fundamental new information about dark matter and dark energy, the two most pressing problems in cosmology. The solutions of these problems will revolutionise our understanding of the universe. This program involves collaborations with major international institutes and provides a superb training-ground for Australian postgraduate students.Read moreRead less
Building the future of theoretical astrophysics: Views of the virtual Universe. The virtual observatory (VO) is a major international initiative to
maximise scientific returns from astrophysical databases by providing
enhanced network access to data and analysis procedures, but it
lacks a vital theoretical complement. This project presents a unified
forward modelling approach to three key problems in: 1. gravitational
lens reconstruction; 2. solar coronal magnetic fields; and 3.
interpreta ....Building the future of theoretical astrophysics: Views of the virtual Universe. The virtual observatory (VO) is a major international initiative to
maximise scientific returns from astrophysical databases by providing
enhanced network access to data and analysis procedures, but it
lacks a vital theoretical complement. This project presents a unified
forward modelling approach to three key problems in: 1. gravitational
lens reconstruction; 2. solar coronal magnetic fields; and 3.
interpretation of stellar oscillations. The goal is the development of
a `virtual telescope' for visualising synthetic datasets, designed to
provide the necessary theoretical complement to the VO.
Read moreRead less
Relativistic Plasma Astrophysics: Pulsars, IDVs and transients. We will tackle four fundamental problems in theoretical astrophysics. How do small, dead stars known as pulsars produce radio emission? Why do quasars, the most distant objects in the universe, twinkle at radio wavelengths? What is the relationship between violent bursts of gamma-ray emission and other astrophysical explosions? Why are strongly magnetized pulsars so efficient at radiating high energy photons? We will attack these qu ....Relativistic Plasma Astrophysics: Pulsars, IDVs and transients. We will tackle four fundamental problems in theoretical astrophysics. How do small, dead stars known as pulsars produce radio emission? Why do quasars, the most distant objects in the universe, twinkle at radio wavelengths? What is the relationship between violent bursts of gamma-ray emission and other astrophysical explosions? Why are strongly magnetized pulsars so efficient at radiating high energy photons? We will attack these questions by developing new theories for coherent emission, scintillation, particle acceleration and processes in superstrong magnetic fields, and testing them against observationsRead moreRead less