The AMANDA Neutrino Detector

R Wischnewski,E Andres,P Askebjer,S W Barwick,R Bay,Lars Bergstrom,A Biron,J Booth,O Botner,Adam Bouchta,Staffan Carius,M Carlson,W Chinowsky,D Chirkin,D F Cowen,C G S Costa,E Dalberg,T Deyoung,Joakim Edsjo,P Ekstrom,A Goobar,L J Gray, A Hallgren,F Halzen,R Hardtke,Y He,G Hill,P O Hulth, S Hundertmark,J Jacobsen,V Kandhadai,A Karle,J Kim,H Leich,M Leuthold,P Lindahl, T M Liss, I Liubarsky,P Loaiza, D M Lowder,P Marciniewski,T Miller,P Miocinovic, P C Mock,R Morse, Mitchel Newcomer, P Niessen,D R Nygren,C Perez De Los Hcros,R Porrata,P B Price,G T Przybylski,W Rhode,Stefan Richter,J L Rodriguez,P Romenesko,D Ross,H Rubinstein,T Schmidt,E Schneider,R Schwarz, U Schwendicke,George F Smoot,M Solarz, V Sorin,C Spiering,P Steffen,R G Stokstad,O Streicher,L Thollander,T Thon,S Tilav,C Walck,C H Wiebusch,K Woschnagg,Weimin Wu,G B Yodh,Steve Young

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS（1999）

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摘要

The first stage of the AMANDA High Energy Neutrino Detector at the South Pole, the 302 PMT array AMANDA-B with an expected effective area for TeV neutrinos of similar to 10(4) m(2), has been taking data since 1997. Progress with calibration, investigation of ice properties, as well as muon and neutrino data analysis are described. The next stage 20-string detector AMANDA-II with similar to 800 PMTs will be completed in spring 2000.

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