  This talk compares standard model predictions for solar neutrino experiments
with the results of actual observations. Here `standard model' means the
combined standard model of minimal electroweak theory plus a standard solar
model. I emphasize the importance of recent analyses in which the neutrino
fluxes are treated as free parameters, independent of any constraints from
solar models, and the stunning agreement between the predictions of standard
solar models and helioseismological measurements.
