A Major Upgrade of the Pierre Auger Cosmic Ray Observatory. A major upgrade is under-way to enhance the sensitivity of the 3000 square kilometre Pierre Auger Observatory in its search for the origin of the highest energy cosmic rays, the most energetic particles known in the Universe. This follows an unexpected Auger result that indicates a significant fraction of these cosmic rays are heavy nuclei. This project, assisting the upgrade, is expected to significantly improve the observatory's abil ....A Major Upgrade of the Pierre Auger Cosmic Ray Observatory. A major upgrade is under-way to enhance the sensitivity of the 3000 square kilometre Pierre Auger Observatory in its search for the origin of the highest energy cosmic rays, the most energetic particles known in the Universe. This follows an unexpected Auger result that indicates a significant fraction of these cosmic rays are heavy nuclei. This project, assisting the upgrade, is expected to significantly improve the observatory's ability to identify the mass, and hence the electric charge, of the incoming cosmic rays, allowing astrophysical source directions to be identified for the low charge particles less affected by cosmic magnetic fields. The project will also contribute to the understanding of particle interactions at energies well beyond those explored at the Large Hadron Collider.Read moreRead less
Exploring the high energy sky with the Pierre Auger Observatory. Cosmic rays are enormously energetic particles that must originate in the most violent environments in the Universe. This work will use the 3000 sq km Pierre Auger Observatory, built in collaboration with Australian physicists, to pinpoint the origin of these rare particles, thus laying to rest one of the longest standing mysteries in astronomy.
Unlocking the universe's high energy secrets with large scale neutrino detectors at the South Pole. Some of the most violent objects in the universe produce extremely energetic radiation in the form of particles, gamma-rays and neutrinos. Innovative observatories like IceCube, a cubic kilometre of instrumented ice at the South Pole, are being used to identify these astrophysical sources and the mechanisms that produce this extreme radiation.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE180100170
Funder
Australian Research Council
Funding Amount
$159,450.00
Summary
Contribution to the AugerPrime upgrade of the Pierre Auger observatory. This project will support basic research into the properties of the highest energy particles in our Universe by contributing to the upgrade of the 3000 square kilometre Pierre Auger Observatory. A major detector upgrade (AugerPrime) is underway to enhance the sensitivity of the observatory for these high-energy cosmic rays. This follows an unexpected Auger result that indicates a significant fraction of these cosmic rays con ....Contribution to the AugerPrime upgrade of the Pierre Auger observatory. This project will support basic research into the properties of the highest energy particles in our Universe by contributing to the upgrade of the 3000 square kilometre Pierre Auger Observatory. A major detector upgrade (AugerPrime) is underway to enhance the sensitivity of the observatory for these high-energy cosmic rays. This follows an unexpected Auger result that indicates a significant fraction of these cosmic rays consist of heavy nuclei. AugerPrime will significantly improve the observatory's ability to identify the mass, and hence the charge, of the particles, allowing astrophysical source directions to be identified for the low charge particles which are less deflected by cosmic magnetic fields. The upgrade will also improve the understanding of particle physics at energies well beyond those explored at the Large Hadron Collider.Read moreRead less
A multi-messenger approach to understanding the high-energy Universe. Some of the most violent objects in the Universe produce extremely energetic radiation in the form of particles, gamma-rays and neutrinos. Innovative observatories like IceCube, a cubic kilometre of instrumented ice at the South Pole, are being used to identify these astrophysical sources and the mechanisms that produce this extreme radiation.
Building Central Asia: Linking the Growth of Asia to its Exhumation. The consumption of the Tethys Ocean and the associated collision of Gondwana-derived terranes with Eurasia resulted in the uplift of the highest mountain belt on Earth: the Himalayas. However, stresses from this collision zone propagated far into the Eurasian interior by reactivating faults and creating mountain belts along these fault zones. This project aims to map and model how and when fault (re)activation occurred by integ ....Building Central Asia: Linking the Growth of Asia to its Exhumation. The consumption of the Tethys Ocean and the associated collision of Gondwana-derived terranes with Eurasia resulted in the uplift of the highest mountain belt on Earth: the Himalayas. However, stresses from this collision zone propagated far into the Eurasian interior by reactivating faults and creating mountain belts along these fault zones. This project aims to map and model how and when fault (re)activation occurred by integrating multi-method thermochronological and structural data on major Meso-Cenozoic Central Asian fault systems. The resulting time-integrated tectonic model will aid in the understanding of the India-Eurasia collision, the building of the mountainous Central Asian landscape and its influence on the Asian climate.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE120100158
Funder
Australian Research Council
Funding Amount
$750,000.00
Summary
The Nanten2 sub-millimetre telescope. The millimetre-wavelength sky holds the key for understanding how stars form in the coldest regions of interstellar space: the molecular clouds of our Galaxy. A new frontline facility in Chile will be used in an international research endeavour to map their structures, in order to find out how they form and what causes stars to be born inside them.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE110100038
Funder
Australian Research Council
Funding Amount
$150,000.00
Summary
The NANTEN2 Observatory sub-millimetre wave telescope. The millimetre-wavelength sky holds the key to understanding how stars form in the coldest regions of interstellar space: the molecular clouds of our Galaxy. This new frontline facility in Chile will be used in an international research endeavour to map these cold regions and the stars they contain in order to find out how they form and what causes stars to be born within them.
Discovery Early Career Researcher Award - Grant ID: DE150101981
Funder
Australian Research Council
Funding Amount
$353,706.00
Summary
Investigating water and energy fluxes partitioning on heterogeneous terrain. This project aims to develop, implement and evaluate a field monitoring technique building upon new theoretical developments to quantify evaporation and transpiration from soil and vegetation using a limited number of measurements of temperature, humidity and net radiation above soil and canopies. This new technique aims to characterise in situ the effect of vegetation cover on the partitioning of energy and water fluxe ....Investigating water and energy fluxes partitioning on heterogeneous terrain. This project aims to develop, implement and evaluate a field monitoring technique building upon new theoretical developments to quantify evaporation and transpiration from soil and vegetation using a limited number of measurements of temperature, humidity and net radiation above soil and canopies. This new technique aims to characterise in situ the effect of vegetation cover on the partitioning of energy and water fluxes in areas with complex terrain and patchy vegetation. The project aims to produce new field experiment designs for optimal use of available technology and without restrictive limitations of fetch size required by traditional approaches (for example, eddy-covariance, Bowen ratio method).Read moreRead less