  The motivations for the magnetic moment solution to the solar neutrino
problem are briefly reviewed and the expected values for a number of
observables to be measured by the SNO experiment are calculated assuming three
different solar magnetic field profiles. The observables examined are the
charged current event rate, the ratio of the neutral current to the charged
current event rates and the charged current electron spectrum as well as their
first and second moments. The dependence of results on the hep neutrino flux is
also analysed and a comparison is made with the corresponding oscillation
results.
