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We have performed a detailed study of the zenith angle dependence of theregeneration factor and distributions of events at SNO and SK for differentsolutions of the solar neutrino problem. In particular, we discuss oscillatorybehaviour and the synchronization effect in the distribution for the LMAsolution, the parametric peak for the LOW solution, etc.. Physicalinterpretation of the effects is given. We suggest a new binning of eventswhich emphasizes distinctive features of zenith angle distributions for thedifferent solutions. We also find the correlations between the integratedday-night asymmetry and the rates of events in different zenith angle bins.Study of these correlations strengthens the identification power of theanalysis.Comment: 40 pages,latex file using RevTex. 17 postscript figures. Notation  changes in Appendix and Fig. 17. To be published in Phys. Rev.

Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem