Author:
Gavrin V. N.,Abazov A. I.,Abdurashitov D. N.,Anosov O. L.,Bychuk O. V.,Danshin S. N.,Eroshkina L. A.,Faizov E. L.,Gavrin V. N.,Gayevsky V. I.,Girin S. V.,Kalikhov A. V.,Kireyev S. M.,Knodel T. V.,Knyshenko I. I.,Kornoukhov V. N.,Mezentseva S. A.,Mirmov I. N.,Ostrinsky A. V.,Petukhov V. V.,Pshukov A. M.,Revzin N. E.,Shikhin A. A.,Slyusareva E. D.,Tikhonov A. A.,Timofeyev P. V.,Veretenkin E. P.,Vermul V. M.,Yantz V. E.,Zakharov Yu. I.,Zatsepin G. T.,Zhandarov V. L.,Bowles T. J.,Cleveland B. T.,Elliott S. R.,O’Brien H. A.,Wark D. L.,Wilkerson J. F.,Davis R.,Lande K.,Cherry M. L.,Kouzes R. T.
Abstract
AbstractA radiochemical 71Ga−71 Ge experiment to determine the integral flux of neutrinos from the sun has been constructed at the Baksan Neutrino Observatory in the USSR. Measurements have begun with 30 tonnes of gallium. The experiment is being expanded with the addition of another 30 tonnes. The motivation, experimental procedures, and present status of this experiment are presented.
Publisher
Cambridge University Press (CUP)
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2 articles.
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