  Solar neutrinos can be efficiently upscattered to MeV scale heavy neutral
leptons (HNLs) within the Earth's mantle. HNLs can then decay to
electron-positron pairs leading to energy deposition inside large-volume
detectors. In this paper we consider mass-portal upscattering of solar
neutrinos to HNLs of mass 20 MeV $\geq m_N \geq 2 m_e$. The large volume of the
Earth compensates for the long decay-length of the HNLs leading to observable
rates of $N\rightarrow \nu_\alpha e^+e^-$ in large volume detectors. We find
that searches for mantle-upscattered HNLs can set the novel limits on mixing
with third generation leptons, $|U_{\tau N}|$ for masses in the MeV regime;
sensitivity to mixing with first- and second-generation leptons is not
competitive with existing search strategies.
