  In this letter we highlight the inherent problems associted with the inverted
hierarchical model of neutrinos with only three generations and suggest
possible solutions within the MSSM. we discuss the new parametrisation of the
solar mixing angle which can identify the light side and dark side of the data.
We then argue whether the inverted hierarchical neutrino mass matrix can
explain the large mixing angle(LMA) MSW solution of the solar neutrino anomaly
in the presence of an appropriate texture of charged lepton mass matrix. In
model independent way we explore such specific form of the charged lepton mass
matrix having special structure in 1-2 block. The contribution to the solar
mass splitting arising out of radiative corrections in MSSM, is calculated,
thus making the model stable under radiative corrections.
