  We present a global embedding of the Fibre inflation model in perturbative
large volume scenario (LVS) in which the inflationary potential is induced via
a combination of string-loop corrections and higher derivative F$^4$-effects.
The minimal Fibre inflation model developed in the standard LVS generically
faces some strong bounds on the inflaton field range arising from the K\"ahler
cone constraints, which subsequently creates a challenge for realising the
cosmological observables while consistently respecting the underlying
supergravity approximations. The main attractive feature of this proposal is to
naturally alleviate this issue by embedding Fibre inflation in perturbative
LVS.
