The Kamiokande Solar Neutrino Experiment

1990 ◽  
Vol 121 ◽  
pp. 179-186 ◽  
Author(s):  
K. S. Hirata ◽  
T. Kajita ◽  
T. Kifune ◽  
K. Kihara ◽  
M. Nakahata ◽  
...  

AbstractThe observation of 8B solar Neutrinos in the Kamiokande-II detector is presented. Based on 450 days of data in the time period of January 1987 through May 1988, the measured flux obtained with Ee ≥ 9.3 MeV was 0.46 ± 0.13 (stat) ± 0.08 (sys) of the value predicted by the standard solar model. The detector and analysis methods were improved since June 1988 and the background level has been decreased by a factor of about three since then.

1990 ◽  
Vol 121 ◽  
pp. 171-177 ◽  
Author(s):  
R. Davis ◽  
K. Lande ◽  
C.K. Lee ◽  
B.T. Cleveland ◽  
J. Ullman

AbstractA report on the results obtained from the chlorine radiochemical solar neutrino experiment in the Homestake mine, Lead, SD. Over the period 1970-1988 a neutrino capture rate of 2.3 ± 0.3 SNU was observed. This rate is discussed in relation: to the theoretical standard solar model, the results from the Kamiokande II experiment, and variations in the solar neutrino flux.


2018 ◽  
pp. 116-119
Author(s):  
J. N. Bahcall ◽  
B. T. Cleveland ◽  
R. Davis ◽  
L. Dostrovsky ◽  
J. C. Evans ◽  
...  

Author(s):  
G. S. Hurst ◽  
S. L. Allman ◽  
C. H. Chen ◽  
S. D. Kramer ◽  
J. O. Thomson ◽  
...  

Author(s):  
R. Davis ◽  
K. Lande ◽  
C. K. Lee ◽  
B. T. Cleveland ◽  
J. Ullman

1990 ◽  
Vol 121 ◽  
pp. 201-212
Author(s):  
V. N. Gavrin ◽  
A. I. Abazov ◽  
D. N. Abdurashitov ◽  
O. L. Anosov ◽  
O. V. Bychuk ◽  
...  

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.


2012 ◽  
Vol 62 (1) ◽  
pp. 315-336 ◽  
Author(s):  
Frank Calaprice ◽  
Cristiano Galbiati ◽  
Alex Wright ◽  
Aldo Ianni

2004 ◽  
Vol 19 (08) ◽  
pp. 1167-1179 ◽  
Author(s):  
A. BELLERIVE

This paper reviews the constraints on the solar neutrino mixing parameters with data collected by the Homestake, SAGE, GALLEX, Kamiokande, SuperKamiokande, and SNO experiments. An emphasis will be given to the global solar neutrino analyses in terms of matter-enhanced oscillation of two active flavors. The results to-date, including both solar model dependent and independent measurements, indicate that electron neutrinos are changing to other active types on route to the Earth from the Sun. The total flux of solar neutrinos is found to be in very good agreement with solar model calculations. Future measurements will focus on greater accuracy for mixing parameters and on better sensitivity to low neutrino energies.


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