Solar neutrino oscillations with a fly-by.

To date, all neutrino experiments have been conducted in a terrestrial environment. We will consider placing a low threshold neutrino detector in orbit around the sun. Advantages of such a detector include observing neutrino oscillations in real time, detecting the CNO, pp and pep neutrinos, and verification of the L-2 dependence of the flux. The ability of such a detector to overcome the background noise induced by cosmic rays will be discussed in the case of a Yb-176 detector.