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DTSTART;TZID=Australia/Sydney:20250416T150000
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DTSTAMP:20260519T065228
CREATED:20250414T235431Z
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UID:13733-1744815600-1744819200@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Michael Kramer (MPIfR\, Bonn)
DESCRIPTION:Exploring Unknown Territory\n\nRadio astronomy is an excellent tool for studying fundamental physics and to probe our edge of understanding. It allows to study compact objects\, black holes at all mass scales and neutron stars\, gravitational waves\, the equation of state of superdense matter\, magnetism\, cosmology\, to name but a few. This talk will give an overview of the ongoing efforts at the MPIfR in Bonn in terms of scientific projects\, instrumentation and strategic considerations\, supported by the presentation of recent results. \nJoin Event on Microsoft Teams\nLocation\n\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColloquia
URL:https://www.atnf.csiro.au/event/sa-colloquium-michael-kramer-mpifr-bonn/
LOCATION:NSW
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/png:https://www.atnf.csiro.au/wp-content/uploads/2025/04/SCR-20250415-jaei.png
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DTSTART;TZID=Australia/Sydney:20250430T150000
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DTSTAMP:20260519T065228
CREATED:20250424T013816Z
LAST-MODIFIED:20250508T064908Z
UID:13777-1746025200-1746028800@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Erik Osinga (Dunlap Institute\, University of Toronto)
DESCRIPTION:Galaxy clusters as the Universe’s largest particle accelerators\n\nAbstract \n\nMergers of galaxy clusters represent the most energetic events since the Big Bang\, releasing energies up to 1064 ergs over Gyr timescales. This energy is dissipated through shocks and turbulence in the intra-cluster medium\, transforming clusters into the Universe’s largest laboratories for studying cosmic ray acceleration and magnetic field amplification. However\, our understanding has largely been limited to massive and nearby clusters due to observational constraints. In this talk\, I will show how observations at the longest wavelengths observable from the ground are revealing new insights into both turbulence and magnetic field amplification. Additionally\, I will discuss how advances in radio polarimetry and new surveys such as POSSUM are revealing the first detailed magnetic field structures within individual clusters. \nJoin Event on Microsoft Teams\nLocation\n\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColloquiaColloquia
URL:https://www.atnf.csiro.au/event/sa-colloquium-erik-osinga-dunlap-institute-university-of-toronto/
LOCATION:CSIRO – Kensington\, Australian Resources Research Centre (ARRC)\, 26 Dick Perry Ave\, Kensington\, WA\, 6101\, Australia
CATEGORIES:Colloquia
ORGANIZER;CN="Li Wang":MAILTO:li.wang1@csiro.au
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