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