  The unwinding inflation mechanism is studied in a type IIB flux
compactification where all moduli are stabilized using flux, non-perturbative
effects, and the leading alpha' corrections of the large volume scenario. We
consider the backreaction on the geometry due to the presence of anti-D3 branes
as well as the backreaction of inflation on the Kaehler moduli, and compute the
resulting corrections to the slow-roll potential. By taking large flux numbers,
we are able to find inflationary epochs where backreaction effects are under
control, the inflaton traverses a super-Planckian field range, and the
resulting amplitude of scalar perturbations is consistent with observation.
