Cosmic-ray muon imaging (muography) has been applied in
various fields in recent years, in which plastic scintillators are
one of the frequently selected detectors internationally. Therefore,
a triangular scintillator strip based muography detection system has
been proposed in the development of the μ Scattering and
Transmission imaging faCility (μSTC). Before the mass production
of detector units, this work studied the impacts of multiple factors
on the light collection efficiency (LCE) and the position resolution
(σ) of plastic scintillators. These factors include
configurations of wavelength shifting (WLS) fibers, fiber grooves on
scintillators, coupling optical glues and silicon photomultiplier
(SiPM) readout mode. According to the simulated results, an
empirical formula was proposed to quantitatively describe the
relation between the LCE and σ, which has seldom been studied
before. In this formula, σ reduces as a power-law function of
the LCE. The SiPM readout mode (single-end or double-end output) and
fiber groove treatments show no significant influence on the
σ-LCE relation. LCE variations due to different factors lead
to a difference in σ of less than 0.2 mm in the whole range
of LCE. Accordingly, these factors are nearly equivalent in the
improvement of detector position resolution. In comparison, the muon
hit position reconstruction method nearly halves the σ after
using angular and gap corrections. Thus, a better reconstruction
method shows greater importance than the efforts made to increase
LCEs. The simulation study in this work will provide good references
for the construction of plastic scintillators of the μSTC
platform in the near future.