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Technology Development for a Neutrino AstrophysicalObservatory

Description/Abstract

We propose a set of technology developments relevant to the design of an optimized Cerenkov detector for the study of neutrino interactions of astrophysical interest. Emphasis is placed on signal processing innovations that enhance significantly the quality of primary data. These technical advances, combined with field experience from a follow-on test deployment, are intended to provide a basis for the engineering design for a kilometer-scale Neutrino Astrophysical Observatory.

DOI 10.2172/893196
Creator/Author: Chaloupka, V. ; Cole, T. ; Crawford, H.J. ; He, Y.D. ; Jackson, S. ; Kleinfelder, S. ; Lai, K.W. ; Learned, J. ; Ling, J. ; Liu, D. ; Lowder, D. ; Moorhead, M. ; Morookian, J.M. ; Nygren, D.R. ; Price, P.B. ; Richards, A. ; Shapiro, G. ; Shen, B. ; Smoot, George F. ; Stokstad, R.G. ; VanDalen, G. ; Wilkes, J. ; Wright, F. ; Young, K.
Publication Date:1996 Feb 01
OSTI Identifier:OSTI ID: 893196
Report Number(s):LBL--38321
DOE Contract Number:DE-AC02-05CH11231
DOI:10.2172/893196
Other Number(s):TRN: US0605960
Resource Type:Technical Report
Research Org:Ernest Orlando LawrenceBerkeley NationalLaboratory, Berkeley, CA (US)
Sponsoring Org:USDOE Director, Office of Science
Subject:72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; DESIGN; NEUTRINOS; PROCESSING
Country of Publication:United States
Language:English
Format: Size: 60
Update Date:2008 Feb 05

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