  Using HINODE/XRT, GOES, SDO/AIA observations, we study a compact C-1.4 class
flare outside a major sunspot of AR 12178 on 4 October 2014. This flare is
associated with a peculiar coronal jet, which is erupted in two stages in the
overlying corona above the compact flaring region. At the time of flare
maximum, the first stage of the jet eruption occurs above the flare energy
release site, and thereafter in the second stage its magneto-plasma system
interacts with the overlying distinct magnetic field domain in its vicinity to
build further the typical jet plasma column.
