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Solar neutrino measurements have recently reached a level of sensitivity such that CNO fluxes can now be experimentally determined. While these first measurements are still only sensitive to the higher energy neutrinos resulting from the β+ decays of O15 produced by the N14(p,γ)O15 reaction, future measurements will work towards detection of neutrinos from the β+ decay of N13 from the C12(p,γ)N13 reaction.
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