Figure 7: Neutrino spectra expected in Borexino (accounting for the detector’s energy resolution). The upper line represents the neutrino signal rate in Borexino according to the most recent predictions of the standard solar model [118] including neutrino oscillations with the LMA-MSW parameters. The lower line illustrates the contribution due to Be neutrinos. The pp neutrinos contribute to the spectrum below 0.3 MeV and the edge at 1.2 MeV is due to pep neutrinos (from [119]).