  We present "Before and After" global oscillation solutions, as well as
predicted "Before and After" values and ranges for ten future solar neutrino
observables (for BOREXINO, KamLAND, SNO, and a generic p-p neutrino detector).
We have performed global analyses using the full SNO day-night energy spectrum
and, alternatively, just the SNO CC and NC rates and the day-night
asymmetry.The ``Before'' case includes all solar neutrino data (and some
theoretical improvements) available prior to April 20, 2002 and the ``After''
case includes, in addition, the new SNO data on the CC, NC, and day-night
asymmetry. The LMA solution is the only currently allowed MSW oscillation
solution at ~99% CL. The LOW solution is allowed only at more than 2.5 sigma,
SMA at 3.7 sigma or 4.7 sigma (depending upon analysis strategy), and pure
sterile oscillations at 4.7sigma. Small mixing angles are ``out''(pure sterile
is ``way out''); MSW with large mixing angles is definitely ``in''. Vacuum
oscillations are allowed at 3 sigma, but not a 2 sigma. Precise maximal mixing
is excluded at 3.2 sigma for MSW solutions and at 2.8 sigma for vacuum
solutions. Most of the predicted values for future observables for the
BOREXINO, KamLAND, and future SNO measurements are changed only by minor
amounts by the inclusion of the recent SNO data. In order to test the
robustness of the allowed neutrino oscillation regions and the predictions for
future observables, we have carried out calculations using a variety of
strategies to analyze the SNO and other solar neutrino data.
