Abstract
The first stage of the AMANDA High Energy Neutrino Detector at the South Pole, the 302 PMT array AMANDA-B10, is taking data since 1997. We describe results on atmospheric neutrinos, limits on indirect WIMP detection, seasonal muon flux variation, relativistic monopole flux limits, a search for gravitational collapse neutrinos, and a depth scan of the optical ice properties. The next stage 19-string detector AMANDA-II with ∼650 PMTs will be completed in spring 2000.
Original language | English (US) |
---|---|
Pages (from-to) | 141-145 |
Number of pages | 5 |
Journal | Nuclear Physics B - Proceedings Supplements |
Volume | 85 |
Issue number | 1-3 |
DOIs | |
State | Published - May 2000 |
All Science Journal Classification (ASJC) codes
- Atomic and Molecular Physics, and Optics
- Nuclear and High Energy Physics