  A magnetised flux rope model, "Flux Rope in 3D" (FRi3D) is used in the
framework of European Heliospheric Forecasting Information Asset (EUHFORIA) for
studying the evolution and propagation of coronal mass ejections (CME). In this
paper, we rectify the mistake in the mentioned magnetic field profile of the
FRi3D model used in Maharana et al., 2022, and we clarify the actual profile
used in that work. In addition, we provide the recent updates introduced to the
FRi3D implementation in EUHFORIA like optimising the "ai.fri3d" python package
to reduce computational time and exploring different CME leg disconnection
methods to make the numerical implementation more stable.
