  We present a quantitative analysis of the flavor physics of a SUSY SO(10)
model proposed by Chang, Masiero, and Murayama, linking b -> s transitions to
the large observed atmospheric neutrino mixing. We consider B_s-B_s-bar mixing
and tau -> mu gamma and discuss their correlation paying careful attention to
their different dependences on model parameters. Our analysis shows that an
order-of-magnitude enhancement of the mass difference with respect to the
Standard Model is possible and can be reconciled with the most stringent bounds
on lepton flavor violation. The situation for various Delta B=1 decays is
discussed qualitatively.
