The results of recent Kamiokande-II and {sup 37}Cl solar-neutrino experiments are quantitatively analyzed assuming the Mikheyev-Smirnov-Wolfenstein solution to the solar-neutrino problem. It is found that the parameter region known as the large mass'' solution to the solar-neutrino problem is disfavored by a little more than 1 {sigma} while the small mass'' and large angle'' solutions are in good agreement at this level. The implications on this analysis from time variations in the data are discussed.