  We report on temporal and spectral study of a flat spectrum radio quasar, PKS
B1222+216, in flare state to get insight into acceleration and emission
mechanisms inside the jet. This is one of the brightest and highly active
blazar in the MeV-GeV regime. Long term multi-waveband light curves of this
object showed a flaring activity in 2014 with two distinct flares. Work
presented here includes the study of flux-index variation, flare fitting,
hardness ratio and spectral modelling of both X-ray and $\gamma-$ray data. The
flux-index correlation we have found in MeV-GeV regime indicates a 'softer when
brighter' feature. Modelling of $\gamma-$ray light curves suggests that low
energy particles initiate both the flares followed by the injection of high
energy particles. The short rise time indicates the presence of Fermi first
order acceleration. Multi-waveband spectral energy distributions (SEDs)
generated for flares are fitted with a single-zone leptonic model. This SED
modelling shows the inverse Compton scattering of photon field reprocessed from
Broad Line Region (BLR) primarily accounts for GeV emission. We have also
report a shift in break-energy in the soft X-ray regime during the flaring
activity which is the consequence of a rapid change in injection spectra.
