  Super-Kamiokande uses neutrino-electron elastic scattering to measure the
recoil electron spectrum and zenith-angle dependence of solar $^8$B neutrinos.
SNO has measured the $^8$B neutrino--deuteron charged-current reaction rate.
The elastic scattering rate, spectrum and zenith-angle dependence in
conjunction with the charged-current reaction rate favors active neutrino
oscillations at large mixing angles by about 3$\sigma$ over the no-oscillation
hypothesis and small mixing angles. The analysis is independent of the absolute
$^8$B and {\it hep} flux and assumes two-flavor oscillations described by
mixing angle and mass$^2$ difference. Two allowed regions at large mixing are
found.
