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Leptogenesis is an attractive scenario in which neutrino masses and baryonasymmetry of the Universe are explained together under a minimal set ofassumptions.  After formulating the problem of initial conditions and introducing thestrong thermal leptogenesis conditions as solution, we show that, within theframework provided by the \soten~model of leptogenesis, the latter lead to aset of testable predictions on the same neutrino parameters currently underexperimental investigations.  The emerging scenario selects the normal ordering of the neutrino masspattern, a large value for the reactor mixing angle, $2\deg \lesssim\theta_{13} \lesssim 20\deg$, as well as a non maximal atmospheric mixingangle, $16\deg \lesssim \theta_{23} \lesssim 41\deg$, and favours negativevalues for the Dirac phase \delta. The signature of the proposed strong thermal\soten~solutions is in the relation obtained between the effective Majoranamass and the lightest neutrino mass: $m_{ee} \approx 0.8 \, m_1 \approx 15 $meV.

Strong thermal Leptogenesis: an exploded view of the low energy neutrino parameters in the SO(10)-inspired model