Abstract
The rate of neutrino line emission is calculated for nuclei that are usually assumed to produce only continuum neutrino emission. A convenient formula is derived that gives for solar interior conditions the ratio of the rates of neutrino line emission to continuum neutrino emission. The only significant line emission from the solar interior is expected from the $\mathrm{pep}$ and $^{7}\mathrm{Be}$-electron capture reactions.
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