We take another look at "just-so" solar neutrino oscillations, characterizi
ng them by the energy E-pi/2 at which the distance-varying angle is pi/2, i
nstead of by the usual Delta m(2). The rising spectrum recently observed by
the SuperKamiokande Collaboration is consistent with an E-pi/2 similar to
6-9 MeV and marginally with 48 MeV. The pp neutrinos must then be reduced t
o one-half the standard solar model prediction, and Be-7 neutrinos must mak
e up a significant part of the SAGE and GALLEX gallium signal. For E-pi/2 c
lose to 9 and 48 MeV, the Be-7 neutrinos will also show a large seasonal va
riation, emphasizing the importance of direct measurements of the Be-7 neut
rinos. [S0556-2821(99)50213-0].