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[en] This paper proposes the construction of a solar neutrino observatory utilizing 1000 tonnes of D2O in a nickel mine near Sudbury. The rationale for such an observatory, the characteristics of the detector and its sensitivity are discussed. Recent progress in resolving some of the problems in the construction and operation of the detector are outlined. Technical measurements and engineering designs are in progress with a view to preparing detailed cost estimates
Source
Cameron, J.M.; Campbell, B.A.; Kamal, A.N.; Khanna, F.C.; Ng, J.; Poutissou, J.M; 616 p; ISBN 9971-50-302-6; 
; 1987; p. 317-344; World Scientific Pub. Co; Teaneck, NJ (United States); 2. Lake Louise winter institute on new frontiers in particle physics; Alberta (Canada); 15-21 Feb 1987; CONF-870279--; World Scientific Pub. Co., 687 Hartwell Street, Teaneck, NJ 07666 (USA)
; 1987; p. 317-344; World Scientific Pub. Co; Teaneck, NJ (United States); 2. Lake Louise winter institute on new frontiers in particle physics; Alberta (Canada); 15-21 Feb 1987; CONF-870279--; World Scientific Pub. Co., 687 Hartwell Street, Teaneck, NJ 07666 (USA)