  The neutrino long wavelength (just-so) oscillation is revisited as a solution
to the solar neutrino problem. We consider just-so scenario in various cases:
in the framework of the solar models with relaxed prediction of the boron
neutrino flux, as well as in the presence of the non-standard weak range
interactions between neutrino and matter constituents. We show that the fit of
the experimental data in the just-so scenario is not very good for any
reasonable value of the $^8B$ neutrino flux, but it substantially improves if
the non-standard $\tau$-neutrino--electron interaction is included. These new
interactions could also remove the conflict of the just-so picture with the
shape of the SN 1987A neutrino spectrum. Special attention is devoted to the
potential of the future real-time solar neutrino detectors as are
Super-Kamiokande, SNO and BOREXINO, which could provide the model independent
tests for the just-so scenario. In particular, these imply specific deformation
of the original solar neutrino energy spectra, and time variation of the
intermediate energy monochromatic neutrino ($^7Be$ and $pep$) signals.
