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DTSTART;VALUE=DATE:20101218
DTEND;VALUE=DATE:20301219
DTSTAMP:20241211T215001Z
CREATED:20230721T092751Z
LAST-MODIFIED:20241211T215001Z
UID:92363-1292630400-1923868799@www.a3veen.nl
SUMMARY:IceCube Neutrino Observatory
DESCRIPTION:The IceCube Neutrino Observatory (or simply IceCube) is a neutrino observatory constructed at the Amundsen–Scott South Pole Station in Antarctica\, the project is a recognized CERN experiment (RE10). \nIts thousands of sensors are located under the Antarctic ice\, distributed over a cubic kilometre. Similar to its predecessor\, the Antarctic Muon And Neutrino Detector Array (AMANDA)\, IceCube consists of spherical optical sensors called Digital Optical Modules (DOMs)\, each with a photomultiplier tube (PMT) and a single-board data acquisition computer which sends digital data to the counting house on the surface above the array. IceCube was completed on 18 December 2010. DOMs are deployed on strings of 60 modules each at depths between 1\,450 and 2\,450 meters into holes melted in the ice using a hot water drill. IceCube is designed to look for point sources of neutrinos in the teraelectronvolt (TeV) range to explore the highest-energy astrophysical processes. In November 2013 it was announced that IceCube had detected 28 neutrinos that likely originated outside the Solar System. \nLinks:\nIceCube Neutrino Observatory \nIceCube: the coolest way to detect neutrinos (TV The Royal Institution) \nIceCube: the coolest way to detect neutrinos \nANITA experiment \nOur galaxy seen through a new lens: neutrinos detected by IceCube \n[LIVE] Observation of high-energy neutrinos from the Galactic plane
URL:https://www.a3veen.nl/event/icecube-neutrino-observatory/
CATEGORIES:Fysica,kennis
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Amsterdam:20231021T203000
DTEND;TZID=Europe/Amsterdam:20231021T220000
DTSTAMP:20240102T211127Z
CREATED:20240102T210554Z
LAST-MODIFIED:20240102T211127Z
UID:100989-1697920200-1697925600@www.a3veen.nl
SUMMARY:The need for fusion - with the UK Atomic Energy Authority (TV RIGB webcast)
DESCRIPTION:Join us for a captivating academic discourse on the need for fusion energy\, where audiences are invited to explore and delve into fusion energy’s complex scientific underpinnings. \nMark Maslin\, a preeminent researcher from UCL\, will initiate the event by elucidating the interplay between fusion energy’s development and its positioning in the broader energy market. In doing so\, he will provide a comprehensive understanding of how fusion can address escalating global energy demands and combat the pressing challenges of climate change. Dennis Whyte\, a respected scholar from MIT\, will delve into the formidable complexities of plasma physics\, a crucial aspect of the fusion process. Thus\, educating audiences on the remarkable progress made in overcoming the obstacles that hinder fusion’s practical development. Jenny Cane from UKAEA\, an expert in fusion engineering\, will demonstrate the importance of integrated design and materials research in fusion energy development. She will provide unique insights into the physical demands and stresses that must be considered when designing fusion power plants. This event encourages a thorough understanding of fusion energy and its potential to reshape the global energy landscape. Whether you are an esteemed academic\, a passionate researcher\, an aspiring scientist\, or an ardent student\, the evening offers an exceptional opportunity to engage with leading-edge scientific discourse. This event is in collaboration with the UK Atomic Energy Authority (UKAEA). \nLinks:\nThe need for fusion – with the UK Atomic Energy Authority
URL:https://www.a3veen.nl/event/the-need-for-fusion-with-the-uk-atomic-energy-authority-tv-rigb-webcast/
LOCATION:The Royal Institution of Great Britain\, 21 Albemarle Street\, London\, Verenigd Koninkrijk
CATEGORIES:Fysica,kennis
END:VEVENT
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