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Research Topic : Space Transport
Scheme : Discovery Projects
Australian State/Territory : TAS
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  • Funded Activity

    Discovery Projects - Grant ID: DP0342478

    Funder
    Australian Research Council
    Funding Amount
    $180,000.00
    Summary
    Masers: high resolution probes of star formation. The largest stars in the Galaxy play a vital role in the formation of the atoms which make life on Earth possible. The birth of these stars is shrouded in gas and dust through which only radiowaves penetrate. In this project we will make observations of interstellar masers from the hydroxyl and methanol molecules and through mathematical modelling of molecular excitation and radiative transfer probe the physical, chemical and evolution .... Masers: high resolution probes of star formation. The largest stars in the Galaxy play a vital role in the formation of the atoms which make life on Earth possible. The birth of these stars is shrouded in gas and dust through which only radiowaves penetrate. In this project we will make observations of interstellar masers from the hydroxyl and methanol molecules and through mathematical modelling of molecular excitation and radiative transfer probe the physical, chemical and evolutionary status of the high-mass stars associated with the masers.
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    Funded Activity

    Discovery Projects - Grant ID: DP0770157

    Funder
    Australian Research Council
    Funding Amount
    $356,292.00
    Summary
    Radio Interferometer Studies of Compact Astronomical Sources. The giant black holes in the centres of distant galaxies that are the topic of this study are used to set the reference frame for geodesy on the earth. Remote and exotic as they are, they have real-world applications such as improving the positions available from GPS receivers and measuring continental drift. The signal processing equipment being developed for this new telescope is based on FPGA (field programmable gate array) chips .... Radio Interferometer Studies of Compact Astronomical Sources. The giant black holes in the centres of distant galaxies that are the topic of this study are used to set the reference frame for geodesy on the earth. Remote and exotic as they are, they have real-world applications such as improving the positions available from GPS receivers and measuring continental drift. The signal processing equipment being developed for this new telescope is based on FPGA (field programmable gate array) chips, that promise to revolutionize the data processing industry, from radar to cellular telephones to computer networks. The young scientists who are working on this project will go on to lead the commercial and industrial applications of this new technology.
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    Funded Activity

    Discovery Projects - Grant ID: DP180101061

    Funder
    Australian Research Council
    Funding Amount
    $416,584.00
    Summary
    The scale and structure of the Milky Way. This project aims to use new Australian infrastructure to make the most accurate distance measurements to date in the southern Milky Way, completing the three-dimensional picture of our Galaxy. Australia's international standing in astronomy has led to it being one of the host countries for the square kilometre array project, which will bring significant economic and technological benefits to the country. This project builds upon Australia's astronomical .... The scale and structure of the Milky Way. This project aims to use new Australian infrastructure to make the most accurate distance measurements to date in the southern Milky Way, completing the three-dimensional picture of our Galaxy. Australia's international standing in astronomy has led to it being one of the host countries for the square kilometre array project, which will bring significant economic and technological benefits to the country. This project builds upon Australia's astronomical expertise and will provide the most accurate picture to date of the Milky Way. Astronomy provides unique opportunities for engaging the community in discussions of science and society and inspires students to study STEM subjects.
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    Funded Activity

    Discovery Projects - Grant ID: DP110104101

    Funder
    Australian Research Council
    Funding Amount
    $230,000.00
    Summary
    A survey of the interstellar medium in the Milky Way and Magellanic Clouds using the Australian Square Kilometre Array Pathfinder. Between the stars in the Milky Way there are clouds of gas and dust; old stars eject heavy elements into this interstellar medium, and new stars form when interstellar clouds collapse under their own gravity. This survey is making maps of the interstellar gas using spectral lines at radio wavelengths to trace the cycle of star formation.
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    Funded Activity

    Discovery Projects - Grant ID: DP0559613

    Funder
    Australian Research Council
    Funding Amount
    $317,882.00
    Summary
    Transient Astronomical Sources at Radio Frequencies. Australian radio telescopes are among the finest and most modern anywhere in the world, and they are the only such instruments that can study the Southern Hemisphere sky. The University of Tasmania operates two radio observatories, at Hobart, Tas, and Ceduna, SA, that are used together to detect astronomical pulses arriving simultaneously at the two sites. The techniques of interference suppression, dispersion searching, fast sampling over b .... Transient Astronomical Sources at Radio Frequencies. Australian radio telescopes are among the finest and most modern anywhere in the world, and they are the only such instruments that can study the Southern Hemisphere sky. The University of Tasmania operates two radio observatories, at Hobart, Tas, and Ceduna, SA, that are used together to detect astronomical pulses arriving simultaneously at the two sites. The techniques of interference suppression, dispersion searching, fast sampling over broad bandwidths, and high speed data transmission between Ceduna and Hobart that will be implemented in this project have direct applications in science and the communications industry. The students who will develop this equipment will carry over their expertise to the private sector.
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    Active Funded Activity

    Discovery Projects - Grant ID: DP180103260

    Funder
    Australian Research Council
    Funding Amount
    $317,288.00
    Summary
    Mathematical and computational analysis of ship wakes. This project aims to develop mathematical and computational tools to compute the energy in a given ship wake and to determine a range of properties of a ship by taking simple measurements of the water height as the ship travels past. The expected outcomes of this project include a suite of algorithms that back-calculate the hull shape and operating conditions of a moving ship given only the surface height data measured at a single point. The .... Mathematical and computational analysis of ship wakes. This project aims to develop mathematical and computational tools to compute the energy in a given ship wake and to determine a range of properties of a ship by taking simple measurements of the water height as the ship travels past. The expected outcomes of this project include a suite of algorithms that back-calculate the hull shape and operating conditions of a moving ship given only the surface height data measured at a single point. These results should have direct implications for measuring damage to coastal zones by ship wakes and for surveillance of shipping channels.
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    Funded Activity

    Discovery Projects - Grant ID: DP0342500

    Funder
    Australian Research Council
    Funding Amount
    $330,000.00
    Summary
    Structure and Evolution of High Brightness Temperature Cores of Quasars and Galaxies. Interstellar scintillation, ISS, is a revolutionary new and powerful technique which we will use to study the highest brightness temperature cores of radio quasars with unprecedented angular resolution, and probe the interstellar medium of our Galaxy in a way not previously possible. The combination of scintillation and conventional VLBI allows imaging with light-month to light-year resolution across the known .... Structure and Evolution of High Brightness Temperature Cores of Quasars and Galaxies. Interstellar scintillation, ISS, is a revolutionary new and powerful technique which we will use to study the highest brightness temperature cores of radio quasars with unprecedented angular resolution, and probe the interstellar medium of our Galaxy in a way not previously possible. The combination of scintillation and conventional VLBI allows imaging with light-month to light-year resolution across the known Universe. Scintillation observations are challenging basic synchrotron physics by uncovering quasar cores with temperatures possibly as high as 10^15 K, and lifetimes many times longer than theory. The Ceduna and Hobart telescopes are cornerstones of our scintillation and VLBI proposals.
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    Active Funded Activity

    Discovery Projects - Grant ID: DP200101909

    Funder
    Australian Research Council
    Funding Amount
    $465,000.00
    Summary
    The Occurrence of Cold Planets in the Galaxy. The project aims to explore a unique niche in exoplanet detection: searches for cold planets down to Earth mass, including ice giants and rogue free-floating planets. Infrared cameras and adaptive optics on large telescopes will be used to make accurate measurements of cold planets in diverse galactic environments. These are significant because they are completely different from most known exoplanets, being far from their host stars and unique probes .... The Occurrence of Cold Planets in the Galaxy. The project aims to explore a unique niche in exoplanet detection: searches for cold planets down to Earth mass, including ice giants and rogue free-floating planets. Infrared cameras and adaptive optics on large telescopes will be used to make accurate measurements of cold planets in diverse galactic environments. These are significant because they are completely different from most known exoplanets, being far from their host stars and unique probes of planet formation theory. Expected outcomes are a greatly improved understanding of planet formation, and improved techniques for cold planet detection with gravitational microlensing. The project will strongly benefit the next generation space-based programs planned for the next decade.
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    Active Funded Activity

    Discovery Projects - Grant ID: DP210100313

    Funder
    Australian Research Council
    Funding Amount
    $366,000.00
    Summary
    Quantitative psychological theories for a dynamic world. . The dynamic world around us means we need to constantly adjust our decisions in light of ever-changing influences, both external (weather, traffic ...) and internal (fatigue, learning ...). This project aims to understand how these changes affect performance. This will have significance for basic science, and also practical benefits for applied psychology. This project will examine the dynamic nature of psychological processes in a range .... Quantitative psychological theories for a dynamic world. . The dynamic world around us means we need to constantly adjust our decisions in light of ever-changing influences, both external (weather, traffic ...) and internal (fatigue, learning ...). This project aims to understand how these changes affect performance. This will have significance for basic science, and also practical benefits for applied psychology. This project will examine the dynamic nature of psychological processes in a range of settings: simple decisions, consumer decisions, human-machine interactions, and team performance. Theory development will lead to improved understanding of underlying cognitive processes, and transforms the measurement of decisions, which is important for applied psychological investigations.
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