  We discuss the status of the solutions of the solar neutrino problem in terms
of oscillations of $\nu_e$ into active or sterile neutrinos. We present the
results of a global fit to the full data set corresponding to the latest data
presented at the $\nu$-2000 conference. We show the possible solutions in the
full parameter space including both MSW and vacuum, as well as quasi-vacuum
oscillations (QVO) and matter effects for mixing angles in the second octant
(the so called dark side). Our conclusion is that from the statistical point of
view, all solutions for oscillations into active neutrinos: LMA, LOW, SMA and
the QVO solutions are acceptable since they all provide a reasonable GOF to the
full data set. The same holds for the SMA solution for oscillations into
sterile neutrinos. LMA and LOW-QVO solutions for oscillations into active
neutrinos seem slightly favoured over SMA solutions for oscillations into
active or sterile neutrinos. We also analyze the dependence of these
conclusions on the uncertainty of the SSM $^8$B flux and on the removal of the
data from one of the experimental rates. We also present the results in the
framework of four neutrino oscillations which allows for oscillations into a
state which is a combination of active and sterile neutrino.
