Title

Recent results from sage

Authors

V. N. Gavrin, Institute for Nuclear Research of the Russian Academy of Sciences
E. L. Faizov, Institute for Nuclear Research of the Russian Academy of Sciences
A. V. Kalikhov, Institute for Nuclear Research of the Russian Academy of Sciences
T. V. Knodel, Institute for Nuclear Research of the Russian Academy of Sciences
I. I. Knyshenko, Institute for Nuclear Research of the Russian Academy of Sciences
V. N. Kornoukhov, Institute for Nuclear Research of the Russian Academy of Sciences
I. N. Mirmov, Institute for Nuclear Research of the Russian Academy of Sciences
A. V. Ostrinsky, Institute for Nuclear Research of the Russian Academy of Sciences
A. M. Pshukov, Institute for Nuclear Research of the Russian Academy of Sciences
A. A. Shikhin, Institute for Nuclear Research of the Russian Academy of Sciences
P. V. Timofeyev, Institute for Nuclear Research of the Russian Academy of Sciences
E. P. Veretenkin, Institute for Nuclear Research of the Russian Academy of Sciences
V. M. Vermul, Institute for Nuclear Research of the Russian Academy of Sciences
G. T. Zatsepin, Institute for Nuclear Research of the Russian Academy of Sciences
T. J. Bowles, Los Alamos National Laboratory
S. R. Elliott, Los Alamos National Laboratory
J. S. Nico, Los Alamos National Laboratory
W. A. Teasdale, Los Alamos National Laboratory
D. L. Wark, Los Alamos National Laboratory
J. F. Wilkerson, Los Alamos National Laboratory
B. T. Cleveland, University of Pennsylvania
T. Daily, University of Pennsylvania
R. Davis, University of Pennsylvania
K. Lande, University of Pennsylvania
C. K. Lee, University of Pennsylvania
P. Wildenhain, University of Pennsylvania
M. L. Cherry, Louisiana State University
R. T. Kouzes, Princeton University

Document Type

Article

Publication Date

1-1-1994

Abstract

A radiochemical 71Ga-71Ge experiment to determine the primary flux of neutrinos from the Sun began measurements of the solar neutrino flux at the Baksan Neutrino Observatory in 1990. The number of 71Ge atoms extracted from initially 30 and later 57 tons of metallic gallium was measured in fifteen runs during the period of January 1990 to May 1992. The observed capture rate is 70±19 (sta)±10 (syst) SNU. This is to be compared with 132 SNU predicted by the Standard Solar Model. © 1994.

Publication Source (Journal or Book title)

Nuclear Physics B (Proceedings Supplements)

First Page

412

Last Page

417

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