From the first neutrino telescope, the antarctic muon and neutrino detector array AMANDA, to the IceCube observatory
May, 19994 pages
Contribution to:
Experiments:
Citations per year
0 Citations
Abstract:
With an effective telescope area of order 10,000 meter squared for very high energy neutrinos, a threshold near 50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe the calibration of natural deep ice as a particle detector as well as AMANDA’s performance as a neutrino telescope. We discuss its expansion to AMANDA II in the coming Antarctic summer and, subsequently, to a kilometer-scale detector ICECUBE.- talk: Venice 1999/02/23
- talk: Salt Lake City 1999/08/17
- neutrino: cosmic radiation
- Cherenkov counter: water
- muon: cosmic radiation
- IceCube
- AMANDA
References(11)
Figures(0)