منابع مشابه
The ANTARES AMS Centre : A Status Report 665 progress to 9 - 10
The ANTARES accelerator mass spectrometry facility at Lucas Heights Research Laboratory is operational and AMS measurements of 14C, 26Al and Cl 36are being carried out routinely. Measurement of 129! recently commenced and capabilities for other long-lived radioisotopes such as 10Be are being established. The overall aim of the facility is to develop advanced programs in Quaternary science, glob...
متن کاملANTARES Status Report
The ANTARES Collaboration is building a neutrino telescope 2400 m below the Mediterranean sea close to the Southern French coast. The site is already linked to the shore station by a 40 km-long electro-optical cable (EOC) which transmits power and data. A prototype line and an instrumentation line for monitoring environmental parameters have been successfully deployed and connected to the EOC v...
متن کاملANTARES, Physics potential, progress and status
Observational neutrino astronomy can bring information also on particle physics that can not be obtained in other ways. In general this concerns processes at extreme energy and distance scales. Particularly of interest are cosmic accelerators, GUT phase transition remnants and dark matter annihilation. After four years of R&D the ANTARES Collaboration begins the actual construction of a neutrin...
متن کاملStatus and First Results of the Antares Neutrino Telescope
The ANTARES (Astronomy with a Neutrino Telescope and Abyss environmental RESearch) Collaboration constructed and deployed the world’s largest operational underwater neutrino telescope, optimised for the detection of Cherenkov light produced by neutrino-induced muons. The detector has an effective area of about 0.1 km and it is a first step towards a kilometric scale detector. The detector consi...
متن کاملThe ANTARES Neutrino Telescope
The ANTARES underwater neutrino telescope, at a depth of 2475 m in the Mediterranean Sea, near Toulon, is taking data in its final configuration of 12 detection lines. Each line is equipped with 75 photomultipliers (PMT) housed in glass pressure spheres arranged in 25 triplets at depths between 100 and 450 m above the sea floor. The PMTs look down at 45 to have better sensitivity to the Cherenk...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Radiocarbon
سال: 1995
ISSN: 0033-8222,1945-5755
DOI: 10.1017/s0033822200031180