Results from SAGE
J. N. Abdurashitov, Institute for Nuclear Research of the Russian Academy of Sciences
V. N. Gavrin, Institute for Nuclear Research of the Russian Academy of Sciences
S. V. Girin, Institute for Nuclear Research of the Russian Academy of Sciences
V. V. Gorbatchev, Institute for Nuclear Research of the Russian Academy of Sciences
A. O. Gusev, 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. N. Mirmov, Institute for Nuclear Research of the Russian Academy of Sciences
A. M. Pshukov, Institute for Nuclear Research of the Russian Academy of Sciences
A. M. Shalagin, Institute for Nuclear Research of the Russian Academy of Sciences
A. A. Shikhin, 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
V. Yants, 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
J. S. Nico, Los Alamos National Laboratory
W. A. Teasdale, Los Alamos National Laboratory
D. L. Wark, Los Alamos National Laboratory
S. R. Elliott, University of Washington
J. F. Wilkerson, University of Washington
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. W. Wildenhain, University of Pennsylvania
M. L. Cherry, Louisiana State University
Abstract
The Russian-American Gallium solar neutrino Experiment (SAGE) is described. Beginning in September 1992, SAGE II data were taken with 55 tons of Ga and with significantly reduced backgrounds. The solar neutrino flux measured by 31 extractions through October 1993 is presented. The result of 69 ± 10 +5/-7 SNU is to be compared with a Standard Solar Model prediction of 132 SNU.
