  Using the multi-temperature observations from SDO/AIA on 30th December 2019,
we provide a signature of prominence driven forced magnetic reconnection in the
corona and associated plasma dynamics during 09:20 UT to 10:38 UT. A hot
prominence segment erupts with a speed of 21 km/s and destabilises the entire
prominence system. Thereafter, it rose upward in the north during 09:28 UT to
09:48 UT with a speed of 24 km/s. The eruptive prominence stretches overlying
field lines upward with the speed of 27-28 km/s , which further undergo into
the forced reconnection. The coronal plasma also flows in southward direction
with the speed of 7 km/s, and both these inflows trigger the reconnection at
09:48 UT. Thereafter, the east and westward magnetic channels are developed and
separated. The east-west reorganization of the magnetic fields starts creating
bi-directional plasma outflows towards the limb with their respective speed of
28 km/s and 37 km/s. Their upper ends are diffused in the overlying corona,
transporting another set of upflows with the speed of 22 km/s and 19 km/s. The
multi-temperature plasma (Te=6.0-7.2) evolves and elongated upto a length of
~10^5 km on the reorganized fields. The hot plasma and remaining prominence
threads move from reconnection region towards another segment of prominence in
the eastward direction. The prominence-prominence/loop interaction and
associated reconnection generate jet-like eruptions with the speed of 178-183
km/s. After the formation of jet, the overlying magnetic channel is disappeared
in the corona.
