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We have analysed the recent results from the observation of charged current\nu_e d \to e^- p p events from solar neutrinos by the Sudbury NeutrinoObservatory SNO assuming neutrino oscillations with three active flavours. Thedata seem to prefer a low mass-squared difference and large mixing anglesolution (the so-called LOW solution) in (12) parameter space. However, whencombined with the Gallium charged current interaction data from Gallex and GNO,distinct (1\sigma) allowed regions corresponding to the large mixing angle(LMA) and small mixing angle (SMA) appear while the LOW solution is disfavouredupto 3\sigma standard deviation. The physical electron neutrino survivalprobability corresponding to these best fit solutions are then determined andanalysed for their energy dependence.Comment: 16 pages Latex file, with 5 epsf figures; one reference adde

Implications of recent solar neutrino observations: An analysis of charged current data