  A statistical analysis of the pre-SNO solar neutrino data is made assuming
the solar neutrino deficit to be resolved by the interaction of the neutrino
magnetic moment with the solar magnetic field. Given the general
characteristics of the field profiles known to lead to the best event rate
predictions, several specific choices of profiles are assumed and fits to the
rates, to the electron recoil spectrum in SuperKamiokande and to the combined
rates and spectrum are performed. Both the rate and spectrum fits are
remarkably better than in a previous analysis of the magnetic moment solution
which used a former standard solar model and previous data, and in particular,
rate fits are far better than those from oscillations. The global analysis also
reflects the general very good quality of the fits.
