  Present results and future measurements of solar neutrinos are discussed. The
results to date indicate that solar electron neutrinos are changing to other
active types and that transitions solely to sterile neutrinos are disfavored.
  The flux of $^{8}B$ solar neutrinos produced in the Sun, inferred assuming
only active neutrino types, is found to be in very good agreement with solar
model calculations.
  Future measurements will focus on greater accuracy for charged current and
neutral current sensitive reactions to provide more accurate measurements of
neutrino flavour change and further studies of day-night flux differences and
spectral shape. Other experiments sensitive to lower energy solar neutrinos
will be in operation soon.
