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VOLUME 57 (1993) | ISSUE 1 | PAGE 12
Correlation of neutrino fluxes in the standard Bahcall-Ulrich solar model in connection with the solar-neutrino problem
The ratios of the fluxes of solar neutrinos from the CNO cycle to those of boron neutrinos are less model-dependent than the fluxes themselves in the standard Bahcall-Ulrich solar model. The uncertainties for these ratios are calculated at the level of three standard deviations. Their importance in the overall formulation of the problem of detecting solar neutrinos is discussed.