  In this paper, we carry out a pilot parameter exploration for the
collision-induced magnetic reconnection (CMR) mechanism that forms filamentary
molecular clouds. Following Kong et al. (2021), we utilize Athena++ to model
CMR in the context of resistive magnetohydrodynamics (MHD), considering the
effect from seven physical conditions, including the Ohmic resistivity
($\eta$), the magnetic field ($B$), the cloud density ($\rho$), the cloud
radius $R$, the isothermal temperature $T$, the collision velocity $v_x$, and
the shear velocity $v_z$. Compared to their fiducial model, we consider a
higher and a lower value for each one of the seven parameters. We quantify the
exploration results with five metrics, including the density probability
distribution function ($\rho$-PDF), the filament morphology (250 $\mu$m dust
emission), the $B$-$\rho$ relation, the dominant fiber width, and the ringiness
that describes the significance of the ring-like sub-structures. The
exploration forms straight and curved CMR-filaments with rich sub-structures
that are highly variable in space and time. The variation translates to
fluctuation in all the five metrics, reflecting the chaotic nature of magnetic
reconnection in CMR. A temporary $B\propto\rho$ relation is noticeable during
the first 0.6 Myr. Overall, the exploration provides useful initial insights to
the CMR mechanism.
